[SCM] Handle World Coordinate Systems in Astronomy branch, upstream, updated. 5e2745f048b49e9b527d83ee64661bf4204f3a82
Ole Streicher
debian at liska.ath.cx
Tue Mar 13 12:47:16 UTC 2012
The following commit has been merged in the upstream branch:
commit 9ba974c8e1ddf3f59c09d9a0dbb723551878c2a1
Author: Ole Streicher <debian at liska.ath.cx>
Date: Tue Mar 13 13:45:44 2012 +0100
New upstream version 7.0.0
diff --git a/Makefile.am b/Makefile.am
index 7a97705..5dbbe13 100644
--- a/Makefile.am
+++ b/Makefile.am
@@ -221,9 +221,9 @@ GRP_C_INCLUDE_FILES = \
grf3d.h \
pg3d.h \
loader.h \
+ pal2ast.h \
skyaxis.h \
- pal.h \
- slamac.h \
+ sofa2ast.h \
stc.h \
stcresourceprofile.h \
stcsearchlocation.h \
@@ -283,16 +283,245 @@ WCSLIB_FILES = \
wcsmath.h \
wcstrig.h
-PAL_FILES = \
- COPYING.LIB \
- pal.c \
- pal.h \
- slamac.h
-
LEVMAR_FILES = \
levmar.c \
levmar.h
+STAR_PAL_FILES = \
+ pal/pal.h \
+ pal/palAddet.c \
+ pal/palAmpqk.c \
+ pal/palCaldj.c \
+ pal/palDat.c \
+ pal/palDe2h.c \
+ pal/palDeuler.c \
+ pal/palDh2e.c \
+ pal/palDjcal.c \
+ pal/palDmat.c \
+ pal/palDs2tp.c \
+ pal/palDtp2s.c \
+ pal/palDtps2c.c \
+ pal/palDtt.c \
+ pal/palEcmat.c \
+ pal/palEqgal.c \
+ pal/palEtrms.c \
+ pal/palEvp.c \
+ pal/palFk45z.c \
+ pal/palFk524.c \
+ pal/palFk54z.c \
+ pal/palGaleq.c \
+ pal/palGalsup.c \
+ pal/palMappa.c \
+ pal/palMapqkz.c \
+ pal/palOne2One.c \
+ pal/palPrebn.c \
+ pal/palPrec.c \
+ pal/palPrenut.c \
+ pal/palPvobs.c \
+ pal/palRvgalc.c \
+ pal/palRvlg.c \
+ pal/palRvlsrd.c \
+ pal/palRvlsrk.c \
+ pal/palSubet.c \
+ pal/palSupgal.c \
+ pal/palmac.h
+
+IAU_SOFA_FILES = \
+ sofa/00READ.ME \
+ sofa/sofa.h \
+ sofa/sofam.h \
+ sofa/a2af.c \
+ sofa/a2tf.c \
+ sofa/af2a.c \
+ sofa/anp.c \
+ sofa/anpm.c \
+ sofa/bi00.c \
+ sofa/bp00.c \
+ sofa/bp06.c \
+ sofa/bpn2xy.c \
+ sofa/c2i00a.c \
+ sofa/c2i00b.c \
+ sofa/c2i06a.c \
+ sofa/c2ibpn.c \
+ sofa/c2ixy.c \
+ sofa/c2ixys.c \
+ sofa/c2s.c \
+ sofa/c2t00a.c \
+ sofa/c2t00b.c \
+ sofa/c2t06a.c \
+ sofa/c2tcio.c \
+ sofa/c2teqx.c \
+ sofa/c2tpe.c \
+ sofa/c2txy.c \
+ sofa/cal2jd.c \
+ sofa/cp.c \
+ sofa/cpv.c \
+ sofa/cr.c \
+ sofa/d2dtf.c \
+ sofa/d2tf.c \
+ sofa/dat.c \
+ sofa/dtdb.c \
+ sofa/dtf2d.c \
+ sofa/ee00.c \
+ sofa/ee00a.c \
+ sofa/ee00b.c \
+ sofa/ee06a.c \
+ sofa/eect00.c \
+ sofa/eform.c \
+ sofa/eo06a.c \
+ sofa/eors.c \
+ sofa/epb.c \
+ sofa/epb2jd.c \
+ sofa/epj.c \
+ sofa/epj2jd.c \
+ sofa/epv00.c \
+ sofa/eqeq94.c \
+ sofa/era00.c \
+ sofa/fad03.c \
+ sofa/fae03.c \
+ sofa/faf03.c \
+ sofa/faju03.c \
+ sofa/fal03.c \
+ sofa/falp03.c \
+ sofa/fama03.c \
+ sofa/fame03.c \
+ sofa/fane03.c \
+ sofa/faom03.c \
+ sofa/fapa03.c \
+ sofa/fasa03.c \
+ sofa/faur03.c \
+ sofa/fave03.c \
+ sofa/fk52h.c \
+ sofa/fk5hip.c \
+ sofa/fk5hz.c \
+ sofa/fw2m.c \
+ sofa/fw2xy.c \
+ sofa/gc2gd.c \
+ sofa/gc2gde.c \
+ sofa/gd2gc.c \
+ sofa/gd2gce.c \
+ sofa/gmst00.c \
+ sofa/gmst06.c \
+ sofa/gmst82.c \
+ sofa/gst00a.c \
+ sofa/gst00b.c \
+ sofa/gst06.c \
+ sofa/gst06a.c \
+ sofa/gst94.c \
+ sofa/h2fk5.c \
+ sofa/hfk5z.c \
+ sofa/ir.c \
+ sofa/jd2cal.c \
+ sofa/jdcalf.c \
+ sofa/num00a.c \
+ sofa/num00b.c \
+ sofa/num06a.c \
+ sofa/numat.c \
+ sofa/nut00a.c \
+ sofa/nut00b.c \
+ sofa/nut06a.c \
+ sofa/nut80.c \
+ sofa/nutm80.c \
+ sofa/obl06.c \
+ sofa/obl80.c \
+ sofa/p06e.c \
+ sofa/p2pv.c \
+ sofa/p2s.c \
+ sofa/pap.c \
+ sofa/pas.c \
+ sofa/pb06.c \
+ sofa/pdp.c \
+ sofa/pfw06.c \
+ sofa/plan94.c \
+ sofa/pm.c \
+ sofa/pmat00.c \
+ sofa/pmat06.c \
+ sofa/pmat76.c \
+ sofa/pmp.c \
+ sofa/pn.c \
+ sofa/pn00.c \
+ sofa/pn00a.c \
+ sofa/pn00b.c \
+ sofa/pn06.c \
+ sofa/pn06a.c \
+ sofa/pnm00a.c \
+ sofa/pnm00b.c \
+ sofa/pnm06a.c \
+ sofa/pnm80.c \
+ sofa/pom00.c \
+ sofa/ppp.c \
+ sofa/ppsp.c \
+ sofa/pr00.c \
+ sofa/prec76.c \
+ sofa/pv2p.c \
+ sofa/pv2s.c \
+ sofa/pvdpv.c \
+ sofa/pvm.c \
+ sofa/pvmpv.c \
+ sofa/pvppv.c \
+ sofa/pvstar.c \
+ sofa/pvu.c \
+ sofa/pvup.c \
+ sofa/pvxpv.c \
+ sofa/pxp.c \
+ sofa/rm2v.c \
+ sofa/rv2m.c \
+ sofa/rx.c \
+ sofa/rxp.c \
+ sofa/rxpv.c \
+ sofa/rxr.c \
+ sofa/ry.c \
+ sofa/rz.c \
+ sofa/s00.c \
+ sofa/s00a.c \
+ sofa/s00b.c \
+ sofa/s06.c \
+ sofa/s06a.c \
+ sofa/s2c.c \
+ sofa/s2p.c \
+ sofa/s2pv.c \
+ sofa/s2xpv.c \
+ sofa/sepp.c \
+ sofa/seps.c \
+ sofa/sp00.c \
+ sofa/starpm.c \
+ sofa/starpv.c \
+ sofa/sxp.c \
+ sofa/sxpv.c \
+ sofa/taitt.c \
+ sofa/taiut1.c \
+ sofa/taiutc.c \
+ sofa/tcbtdb.c \
+ sofa/tcgtt.c \
+ sofa/tdbtcb.c \
+ sofa/tdbtt.c \
+ sofa/tf2a.c \
+ sofa/tf2d.c \
+ sofa/tr.c \
+ sofa/trxp.c \
+ sofa/trxpv.c \
+ sofa/tttai.c \
+ sofa/tttcg.c \
+ sofa/tttdb.c \
+ sofa/ttut1.c \
+ sofa/ut1tai.c \
+ sofa/ut1tt.c \
+ sofa/ut1utc.c \
+ sofa/utctai.c \
+ sofa/utcut1.c \
+ sofa/xy06.c \
+ sofa/xys00a.c \
+ sofa/xys00b.c \
+ sofa/xys06a.c \
+ sofa/zp.c \
+ sofa/zpv.c \
+ sofa/zr.c
+
+PAL_FILES = \
+ pal.c \
+ pal.h \
+ sofa.h \
+ sofam.h
bin_SCRIPTS = ast_link
dist_bin_SCRIPTS = ast_link_adam
@@ -373,6 +602,16 @@ libast_la_SOURCES = \
$(GRP_F_INCLUDE_FILES) \
ast_err.h
+# Ensure libast links against libraries containing functions used within
+# libast. If AST is configured --with-external-pal, then the internal
+# libast_pal library will be empty, and we link to an external PAL
+# library instead.
+if EXTERNAL_PAL
+libast_la_LIBADD = $(libdir)/libpal.la libast_wcslib.la libast_levmar.la
+else
+libast_la_LIBADD = libast_pal.la libast_wcslib.la libast_levmar.la
+endif
+
# AST_PAR is really part of GRP_F_INCLUDE_FILES, but it must not be
# distributed, so list it separately.
nodist_libast_la_SOURCES = \
@@ -416,8 +655,8 @@ libast_wcslib_la_SOURCES = proj.c wcstrig.c tpn.c
# Modules adapted from the levmar library.
libast_levmar_la_SOURCES = levmar.c
-# Modules supplied by tpoint.
-libast_pal_la_SOURCES = pal.c
+# Positional astronomy libraries.
+libast_pal_la_SOURCES = $(PAL_FILES)
# The following files are built by the targets in this makefile.
MAINTAINERCLEANFILES = version.h builddocs addversion \
@@ -444,7 +683,7 @@ AST_PAR: ast_par.source astbad
# configure.ac, and so is not distributed automatically.
#
# makeh is required in order to build ast.h after distribution (see below).
-EXTRA_DIST = ast_par.source sun210_figures sun211_figures
+EXTRA_DIST = ast_par.source sun210_figures sun211_figures pal sofa
# ast.h depends on the error-facility files. ast.h _could_ be made
# before distribution, but since it's generated from other distributed
@@ -468,12 +707,15 @@ ast.h: $(AST_H_FILES) ast_err.h makeh config.h
# It's most straightforward to build it at the beginning.
BUILT_SOURCES = AST_ERR ast_err.h version.h
-# Form second links to the main object library (static and shared). This is
-# used when a second pass through the library is needed during linking.
-# Do not forget to change the contents of the libast_pass2.la file to refer
-# to the pass2 libraries rather than the original libraries. Use target
-# install-exec-hook rather than install-exec-local so that the soft links
-# and files are created *after* the main library has been installed.
+# Form a second link to the main object library (static and shared). This
+# is used when a second pass through the library is needed during linking
+# to resolve references made within other AST libraries (e.g. the grf
+# modules, etc), to functions defined within libast (e.g. memory management
+# and error reporting functions). Do not forget to change the contents of
+# the libast_pass2.la file to refer to libast_pass2.* rather than libast.*.
+# Use target install-exec-hook rather than install-exec-local so that the
+# soft links and files are created *after* the main library has been
+# installed.
install-exec-hook: libast.la
$(mkdir_p) $(DESTDIR)$(libdir)
cd $(DESTDIR)$(libdir); \
@@ -485,7 +727,7 @@ install-exec-hook: libast.la
done; \
if test -f "libast.la"; then \
if test -f "libast_pass2.la"; then rm "libast_pass2.la"; fi; \
- sed -e 's/libast/libast_pass2/g' libast.la > libast_pass2.la; \
+ sed -e 's/libast\./libast_pass2\./g' libast.la > libast_pass2.la; \
fi
# Make pre-distribution files. These are files which are required for
@@ -522,4 +764,4 @@ ast_test_SOURCES = ast_test.c
#ast_test_LDADD = `ast_link`
# Expand ast_link to avoid libast_pass2, which causes problems for Solaris
-ast_test_LDADD = libast.la libast_pal.la libast_grf_3.2.la libast_grf_5.6.la libast_wcslib.la libast_levmar.la libast_grf_2.0.la libast_grf3d.la libast_err.la -lm
+ast_test_LDADD = @LIBPAL@ libast.la libast_pal.la libast_grf_3.2.la libast_grf_5.6.la libast_wcslib.la libast_levmar.la libast_grf_2.0.la libast_grf3d.la libast_err.la -lm
diff --git a/Makefile.in b/Makefile.in
index 0303681..7527c7b 100644
--- a/Makefile.in
+++ b/Makefile.in
@@ -48,11 +48,11 @@ DIST_COMMON = $(am__configure_deps) $(dist_bin_SCRIPTS) \
$(dist_starnews_DATA) $(include_HEADERS) $(include_MESSAGES) \
$(srcdir)/AST_ERR $(srcdir)/Makefile.am $(srcdir)/Makefile.in \
$(srcdir)/ast_cpp.in $(srcdir)/ast_err.h $(srcdir)/ast_link.in \
- $(srcdir)/component.xml.in $(srcdir)/config.h.in \
- $(srcdir)/f77.h.in $(srcdir)/fac_1521_err \
- $(srcdir)/object.h.in $(stardocs_DATA) $(top_srcdir)/configure \
- COPYING.LIB compile config.guess config.sub depcomp install-sh \
- ltmain.sh missing
+ $(srcdir)/ast_link_adam.in $(srcdir)/component.xml.in \
+ $(srcdir)/config.h.in $(srcdir)/f77.h.in \
+ $(srcdir)/fac_1521_err $(srcdir)/object.h.in $(stardocs_DATA) \
+ $(top_srcdir)/configure COPYING.LIB compile config.guess \
+ config.sub depcomp install-sh ltmain.sh missing
subdir = .
ACLOCAL_M4 = $(top_srcdir)/aclocal.m4
am__aclocal_m4_deps = $(top_srcdir)/acinclude.m4 \
@@ -63,7 +63,8 @@ am__CONFIG_DISTCLEAN_FILES = config.status config.cache config.log \
configure.lineno configure.status.lineno
mkinstalldirs = $(install_sh) -d
CONFIG_HEADER = config.h
-CONFIG_CLEAN_FILES = component.xml ast_link object.h f77.h ast_cpp
+CONFIG_CLEAN_FILES = component.xml ast_link ast_link_adam object.h \
+ f77.h ast_cpp
am__vpath_adj_setup = srcdirstrip=`echo "$(srcdir)" | sed 's|.|.|g'`;
am__vpath_adj = case $$p in \
$(srcdir)/*) f=`echo "$$p" | sed "s|^$$srcdirstrip/||"`;; \
@@ -77,7 +78,10 @@ am__installdirs = "$(DESTDIR)$(libdir)" "$(DESTDIR)$(bindir)" \
"$(DESTDIR)$(includedir)" "$(DESTDIR)$(includedir)"
libLTLIBRARIES_INSTALL = $(INSTALL)
LTLIBRARIES = $(lib_LTLIBRARIES)
-libast_la_LIBADD =
+ at EXTERNAL_PAL_FALSE@libast_la_DEPENDENCIES = libast_pal.la \
+ at EXTERNAL_PAL_FALSE@ libast_wcslib.la libast_levmar.la
+ at EXTERNAL_PAL_TRUE@libast_la_DEPENDENCIES = $(libdir)/libpal.la \
+ at EXTERNAL_PAL_TRUE@ libast_wcslib.la libast_levmar.la
am__objects_1 = libast_la-axis.lo libast_la-box.lo libast_la-c2f77.lo \
libast_la-channel.lo libast_la-circle.lo libast_la-cmpframe.lo \
libast_la-cmpmap.lo libast_la-cmpregion.lo \
@@ -169,7 +173,8 @@ libast_levmar_la_LIBADD =
am_libast_levmar_la_OBJECTS = libast_levmar_la-levmar.lo
libast_levmar_la_OBJECTS = $(am_libast_levmar_la_OBJECTS)
libast_pal_la_LIBADD =
-am_libast_pal_la_OBJECTS = libast_pal_la-pal.lo
+am__objects_4 = libast_pal_la-pal.lo
+am_libast_pal_la_OBJECTS = $(am__objects_4)
libast_pal_la_OBJECTS = $(am_libast_pal_la_OBJECTS)
libast_pgplot_la_LIBADD =
am_libast_pgplot_la_OBJECTS = libast_pgplot_la-grf_pgplot.lo
@@ -287,6 +292,9 @@ ECHO_N = @ECHO_N@
ECHO_T = @ECHO_T@
EGREP = @EGREP@
EXEEXT = @EXEEXT@
+EXTERNAL_PAL = @EXTERNAL_PAL@
+EXTERNAL_PAL_FALSE = @EXTERNAL_PAL_FALSE@
+EXTERNAL_PAL_TRUE = @EXTERNAL_PAL_TRUE@
F77 = @F77@
FC = @FC@
FCFLAGS = @FCFLAGS@
@@ -300,6 +308,7 @@ INSTALL_STRIP_PROGRAM = @INSTALL_STRIP_PROGRAM@
LATEX2DVI = @LATEX2DVI@
LDFLAGS = @LDFLAGS@
LIBOBJS = @LIBOBJS@
+LIBPAL = @LIBPAL@
LIBS = @LIBS@
LIBTOOL = @LIBTOOL@
LN_S = @LN_S@
@@ -621,9 +630,9 @@ GRP_C_INCLUDE_FILES = \
grf3d.h \
pg3d.h \
loader.h \
+ pal2ast.h \
skyaxis.h \
- pal.h \
- slamac.h \
+ sofa2ast.h \
stc.h \
stcresourceprofile.h \
stcsearchlocation.h \
@@ -678,16 +687,246 @@ WCSLIB_FILES = \
wcsmath.h \
wcstrig.h
-PAL_FILES = \
- COPYING.LIB \
- pal.c \
- pal.h \
- slamac.h
-
LEVMAR_FILES = \
levmar.c \
levmar.h
+STAR_PAL_FILES = \
+ pal/pal.h \
+ pal/palAddet.c \
+ pal/palAmpqk.c \
+ pal/palCaldj.c \
+ pal/palDat.c \
+ pal/palDe2h.c \
+ pal/palDeuler.c \
+ pal/palDh2e.c \
+ pal/palDjcal.c \
+ pal/palDmat.c \
+ pal/palDs2tp.c \
+ pal/palDtp2s.c \
+ pal/palDtps2c.c \
+ pal/palDtt.c \
+ pal/palEcmat.c \
+ pal/palEqgal.c \
+ pal/palEtrms.c \
+ pal/palEvp.c \
+ pal/palFk45z.c \
+ pal/palFk524.c \
+ pal/palFk54z.c \
+ pal/palGaleq.c \
+ pal/palGalsup.c \
+ pal/palMappa.c \
+ pal/palMapqkz.c \
+ pal/palOne2One.c \
+ pal/palPrebn.c \
+ pal/palPrec.c \
+ pal/palPrenut.c \
+ pal/palPvobs.c \
+ pal/palRvgalc.c \
+ pal/palRvlg.c \
+ pal/palRvlsrd.c \
+ pal/palRvlsrk.c \
+ pal/palSubet.c \
+ pal/palSupgal.c \
+ pal/palmac.h
+
+IAU_SOFA_FILES = \
+ sofa/00READ.ME \
+ sofa/sofa.h \
+ sofa/sofam.h \
+ sofa/a2af.c \
+ sofa/a2tf.c \
+ sofa/af2a.c \
+ sofa/anp.c \
+ sofa/anpm.c \
+ sofa/bi00.c \
+ sofa/bp00.c \
+ sofa/bp06.c \
+ sofa/bpn2xy.c \
+ sofa/c2i00a.c \
+ sofa/c2i00b.c \
+ sofa/c2i06a.c \
+ sofa/c2ibpn.c \
+ sofa/c2ixy.c \
+ sofa/c2ixys.c \
+ sofa/c2s.c \
+ sofa/c2t00a.c \
+ sofa/c2t00b.c \
+ sofa/c2t06a.c \
+ sofa/c2tcio.c \
+ sofa/c2teqx.c \
+ sofa/c2tpe.c \
+ sofa/c2txy.c \
+ sofa/cal2jd.c \
+ sofa/cp.c \
+ sofa/cpv.c \
+ sofa/cr.c \
+ sofa/d2dtf.c \
+ sofa/d2tf.c \
+ sofa/dat.c \
+ sofa/dtdb.c \
+ sofa/dtf2d.c \
+ sofa/ee00.c \
+ sofa/ee00a.c \
+ sofa/ee00b.c \
+ sofa/ee06a.c \
+ sofa/eect00.c \
+ sofa/eform.c \
+ sofa/eo06a.c \
+ sofa/eors.c \
+ sofa/epb.c \
+ sofa/epb2jd.c \
+ sofa/epj.c \
+ sofa/epj2jd.c \
+ sofa/epv00.c \
+ sofa/eqeq94.c \
+ sofa/era00.c \
+ sofa/fad03.c \
+ sofa/fae03.c \
+ sofa/faf03.c \
+ sofa/faju03.c \
+ sofa/fal03.c \
+ sofa/falp03.c \
+ sofa/fama03.c \
+ sofa/fame03.c \
+ sofa/fane03.c \
+ sofa/faom03.c \
+ sofa/fapa03.c \
+ sofa/fasa03.c \
+ sofa/faur03.c \
+ sofa/fave03.c \
+ sofa/fk52h.c \
+ sofa/fk5hip.c \
+ sofa/fk5hz.c \
+ sofa/fw2m.c \
+ sofa/fw2xy.c \
+ sofa/gc2gd.c \
+ sofa/gc2gde.c \
+ sofa/gd2gc.c \
+ sofa/gd2gce.c \
+ sofa/gmst00.c \
+ sofa/gmst06.c \
+ sofa/gmst82.c \
+ sofa/gst00a.c \
+ sofa/gst00b.c \
+ sofa/gst06.c \
+ sofa/gst06a.c \
+ sofa/gst94.c \
+ sofa/h2fk5.c \
+ sofa/hfk5z.c \
+ sofa/ir.c \
+ sofa/jd2cal.c \
+ sofa/jdcalf.c \
+ sofa/num00a.c \
+ sofa/num00b.c \
+ sofa/num06a.c \
+ sofa/numat.c \
+ sofa/nut00a.c \
+ sofa/nut00b.c \
+ sofa/nut06a.c \
+ sofa/nut80.c \
+ sofa/nutm80.c \
+ sofa/obl06.c \
+ sofa/obl80.c \
+ sofa/p06e.c \
+ sofa/p2pv.c \
+ sofa/p2s.c \
+ sofa/pap.c \
+ sofa/pas.c \
+ sofa/pb06.c \
+ sofa/pdp.c \
+ sofa/pfw06.c \
+ sofa/plan94.c \
+ sofa/pm.c \
+ sofa/pmat00.c \
+ sofa/pmat06.c \
+ sofa/pmat76.c \
+ sofa/pmp.c \
+ sofa/pn.c \
+ sofa/pn00.c \
+ sofa/pn00a.c \
+ sofa/pn00b.c \
+ sofa/pn06.c \
+ sofa/pn06a.c \
+ sofa/pnm00a.c \
+ sofa/pnm00b.c \
+ sofa/pnm06a.c \
+ sofa/pnm80.c \
+ sofa/pom00.c \
+ sofa/ppp.c \
+ sofa/ppsp.c \
+ sofa/pr00.c \
+ sofa/prec76.c \
+ sofa/pv2p.c \
+ sofa/pv2s.c \
+ sofa/pvdpv.c \
+ sofa/pvm.c \
+ sofa/pvmpv.c \
+ sofa/pvppv.c \
+ sofa/pvstar.c \
+ sofa/pvu.c \
+ sofa/pvup.c \
+ sofa/pvxpv.c \
+ sofa/pxp.c \
+ sofa/rm2v.c \
+ sofa/rv2m.c \
+ sofa/rx.c \
+ sofa/rxp.c \
+ sofa/rxpv.c \
+ sofa/rxr.c \
+ sofa/ry.c \
+ sofa/rz.c \
+ sofa/s00.c \
+ sofa/s00a.c \
+ sofa/s00b.c \
+ sofa/s06.c \
+ sofa/s06a.c \
+ sofa/s2c.c \
+ sofa/s2p.c \
+ sofa/s2pv.c \
+ sofa/s2xpv.c \
+ sofa/sepp.c \
+ sofa/seps.c \
+ sofa/sp00.c \
+ sofa/starpm.c \
+ sofa/starpv.c \
+ sofa/sxp.c \
+ sofa/sxpv.c \
+ sofa/taitt.c \
+ sofa/taiut1.c \
+ sofa/taiutc.c \
+ sofa/tcbtdb.c \
+ sofa/tcgtt.c \
+ sofa/tdbtcb.c \
+ sofa/tdbtt.c \
+ sofa/tf2a.c \
+ sofa/tf2d.c \
+ sofa/tr.c \
+ sofa/trxp.c \
+ sofa/trxpv.c \
+ sofa/tttai.c \
+ sofa/tttcg.c \
+ sofa/tttdb.c \
+ sofa/ttut1.c \
+ sofa/ut1tai.c \
+ sofa/ut1tt.c \
+ sofa/ut1utc.c \
+ sofa/utctai.c \
+ sofa/utcut1.c \
+ sofa/xy06.c \
+ sofa/xys00a.c \
+ sofa/xys00b.c \
+ sofa/xys06a.c \
+ sofa/zp.c \
+ sofa/zpv.c \
+ sofa/zr.c
+
+PAL_FILES = \
+ pal.c \
+ pal.h \
+ sofa.h \
+ sofam.h
+
bin_SCRIPTS = ast_link
dist_bin_SCRIPTS = ast_link_adam
noinst_SCRIPTS = ast_cpp
@@ -752,6 +991,13 @@ libast_la_SOURCES = \
$(GRP_F_INCLUDE_FILES) \
ast_err.h
+ at EXTERNAL_PAL_FALSE@libast_la_LIBADD = libast_pal.la libast_wcslib.la libast_levmar.la
+
+# Ensure libast links against libraries containing functions used within
+# libast. If AST is configured --with-external-pal, then the internal
+# libast_pal library will be empty, and we link to an external PAL
+# library instead.
+ at EXTERNAL_PAL_TRUE@libast_la_LIBADD = $(libdir)/libpal.la libast_wcslib.la libast_levmar.la
# AST_PAR is really part of GRP_F_INCLUDE_FILES, but it must not be
# distributed, so list it separately.
@@ -797,8 +1043,8 @@ libast_wcslib_la_SOURCES = proj.c wcstrig.c tpn.c
# Modules adapted from the levmar library.
libast_levmar_la_SOURCES = levmar.c
-# Modules supplied by tpoint.
-libast_pal_la_SOURCES = pal.c
+# Positional astronomy libraries.
+libast_pal_la_SOURCES = $(PAL_FILES)
# The following files are built by the targets in this makefile.
MAINTAINERCLEANFILES = version.h builddocs addversion \
@@ -812,7 +1058,7 @@ astbad_SOURCES = astbad.c pointset.h
# configure.ac, and so is not distributed automatically.
#
# makeh is required in order to build ast.h after distribution (see below).
-EXTRA_DIST = ast_par.source sun210_figures sun211_figures
+EXTRA_DIST = ast_par.source sun210_figures sun211_figures pal sofa
# AST_ERR and ast_err.h are `generated source files', and so must be
# generated before any other compilations are done. Note that these
@@ -847,7 +1093,7 @@ ast_test_SOURCES = ast_test.c
#ast_test_LDADD = `ast_link`
# Expand ast_link to avoid libast_pass2, which causes problems for Solaris
-ast_test_LDADD = libast.la libast_pal.la libast_grf_3.2.la libast_grf_5.6.la libast_wcslib.la libast_levmar.la libast_grf_2.0.la libast_grf3d.la libast_err.la -lm
+ast_test_LDADD = @LIBPAL@ libast.la libast_pal.la libast_grf_3.2.la libast_grf_5.6.la libast_wcslib.la libast_levmar.la libast_grf_2.0.la libast_grf3d.la libast_err.la -lm
starfacs_DATA = fac_1521_err
all: $(BUILT_SOURCES) config.h
$(MAKE) $(AM_MAKEFLAGS) all-am
@@ -908,6 +1154,8 @@ component.xml: $(top_builddir)/config.status $(srcdir)/component.xml.in
cd $(top_builddir) && $(SHELL) ./config.status $@
ast_link: $(top_builddir)/config.status $(srcdir)/ast_link.in
cd $(top_builddir) && $(SHELL) ./config.status $@
+ast_link_adam: $(top_builddir)/config.status $(srcdir)/ast_link_adam.in
+ cd $(top_builddir) && $(SHELL) ./config.status $@
object.h: $(top_builddir)/config.status $(srcdir)/object.h.in
cd $(top_builddir) && $(SHELL) ./config.status $@
f77.h: $(top_builddir)/config.status $(srcdir)/f77.h.in
@@ -2862,12 +3110,15 @@ AST_PAR: ast_par.source astbad
ast.h: $(AST_H_FILES) ast_err.h makeh config.h
@PERL@ ./makeh -s $(srcdir) $(AST_H_FILES) >$@
-# Form second links to the main object library (static and shared). This is
-# used when a second pass through the library is needed during linking.
-# Do not forget to change the contents of the libast_pass2.la file to refer
-# to the pass2 libraries rather than the original libraries. Use target
-# install-exec-hook rather than install-exec-local so that the soft links
-# and files are created *after* the main library has been installed.
+# Form a second link to the main object library (static and shared). This
+# is used when a second pass through the library is needed during linking
+# to resolve references made within other AST libraries (e.g. the grf
+# modules, etc), to functions defined within libast (e.g. memory management
+# and error reporting functions). Do not forget to change the contents of
+# the libast_pass2.la file to refer to libast_pass2.* rather than libast.*.
+# Use target install-exec-hook rather than install-exec-local so that the
+# soft links and files are created *after* the main library has been
+# installed.
install-exec-hook: libast.la
$(mkdir_p) $(DESTDIR)$(libdir)
cd $(DESTDIR)$(libdir); \
@@ -2879,7 +3130,7 @@ install-exec-hook: libast.la
done; \
if test -f "libast.la"; then \
if test -f "libast_pass2.la"; then rm "libast_pass2.la"; fi; \
- sed -e 's/libast/libast_pass2/g' libast.la > libast_pass2.la; \
+ sed -e 's/libast\./libast_pass2\./g' libast.la > libast_pass2.la; \
fi
@PREDIST at version.h: version.h.in configure.ac
@PREDIST@ rm -f $@; $(predist_subs) version.h.in >$@
diff --git a/aclocal.m4 b/aclocal.m4
index 5f1db8b..d5cfd1f 100644
--- a/aclocal.m4
+++ b/aclocal.m4
@@ -6169,6 +6169,25 @@ AC_MSG_RESULT([$SED])
# original starconf.m4, installed by starconf 1.3, rnum=1003000
# DO NOT EDIT: it may be overwritten when starconf is next run
+# Copyright:
+# Copyright (C) 2003-2005 Council for the Central Laboratory of the
+# Research Councils
+#
+# Licence:
+# This program is free software; you can redistribute it and/or
+# modify it under the terms of the GNU General Public Licence as
+# published by the Free Software Foundation; either version 2 of
+# the Licence, or (at your option) any later version.
+#
+# This program is distributed in the hope that it will be
+# useful,but WITHOUT ANY WARRANTY; without even the implied
+# warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+# PURPOSE. See the GNU General Public Licence for more details.
+#
+# You should have received a copy of the GNU General Public Licence
+# along with this program; if not, write to the Free Software
+# Foundation, Inc., 51 Franklin Street,Fifth Floor, Boston, MA
+# 02110-1301, USA
# STAR_DEFAULTS(options='')
# -------------------------
diff --git a/ast.news b/ast.news
index db52616..87b137d 100644
--- a/ast.news
+++ b/ast.news
@@ -1,6 +1,6 @@
AST Library
-----------
- A new release (V6.0-1) of the Starlink AST (astrometry) library is
+ A new release (V7.0.0) of the Starlink AST (astrometry) library is
now available.
AST provides a comprehensive range of facilities for attaching
@@ -16,13 +16,25 @@ environment-independent.
Main Changes in this Version
----------------------------
+- Fundamental positional astronomy calculations are now performed
+using the IAU SOFA library where possible, and the Starlink PAL library
+otherwise (the PAL library contains a subset of the Fortran Starlink SLALIB
+library re-written in C). Copies of these libraries are bundled with AST
+and so do not need to be obtained or built separately, although external
+copies of SOFA and PAL can be used if necessary by including the
+"--with-external_pal" option when configuring AST.
+
+
+Main Changes in V6.0-1
+-----------------------
+
- The Spitzer "-SIP" distortion code is now recognised within FITS
headers that describe non-celestial axes, as well as celestial axes.
- A bug has been fixed that could cause inappropriate equinox values to
be used when aligning SkyFrames if the AlignSystem attribute is set.
-- The format of the version string for AST has changed from
+- The format of the version string for AST has changed from
"<major>.<minor>-<release>" to "<major>.<minor>.<release>".
Main Changes in V6.0
diff --git a/ast_link.in b/ast_link.in
index 97cf67a..a18d2c4 100644
--- a/ast_link.in
+++ b/ast_link.in
@@ -116,19 +116,15 @@
# result in an error at run time if AST routines are invoked that
# attempt to generate graphical output.
-# SLALIB:
-# The AST distribution includes a cut down subset of the C version of
-# the SLALIB library written by Pat Wallace. This subset contains only
-# the functions needed by the AST library. It is built as part of the
-# process of building AST and is distributed under GPL (and is thus
-# compatible with the AST license). Previous version of this script
-# allowed AST applications to be linked against external SLALIB
-# libraries (either Fortran or C) rather than the internal version.
-# The current version of this script does not provide this option,
-# and always uses the internal SLALIB library. However, for backward
-# compatibility, this script still allows the "-fsla" and "-csla" flags
-# (previously used for selecting which version of SLALIB to use) to be
-# specified, but they will be ignored.
+# SOFA & PAL:
+# The AST distribution includes bundled copies of the IAU SOFA and
+# Starlink PAL libraries. These will be used for fundamental
+# positional astronomy calculations unless the "--with-external_pal"
+# option was used when AST was configured. If "--with-external_pal"
+# is used, this script will include "-lpal" in the returned list of
+# linking options, and the user should then ensure that extrnal copies
+# of the PAL and SOFA libraries are available (SOFA functions are used
+# within PAL).
# Examples:
#c cc display.c -L/star/lib `ast_link -pgplot` -o display
@@ -336,21 +332,18 @@
# "wcslib" module, and the "levmar" module.
args='-last -last_wcslib -last_levmar'
-# Generate arguments for linking SLALIB.
-# --------------------------------------
- case "${sla}" in
+# Generate arguments for linking PAL.
+# -----------------------------------
-# The full proprietary C version of SLALIB has no link script, so simply
-# specify the library itself.
- c) args="${args} -lsla";;
+ case "@EXTERNAL_PAL@" in
-# For Fortran, link with the AST SLALIB interface and the Fortran library via
-# the SLALIB link script (if found).
- f) args="${args} `\`find sla_link\``"
- f77='y';;
+# If we configured --with-external_pal include a link option to pick up
+# an external PAL library.
+ 1) args="${args} -lpal";;
-# Otherwise, link with the internal GPLed cut down C version of SLALIB.
+# Otherwise, use the internal PAL & SOFA libraries.
*) args="${args} -last_pal";;
+
esac
# Generate arguments for linking the 2D graphics system.
diff --git a/ast_link_adam b/ast_link_adam
index 758b19f..a8d0b9a 100644
--- a/ast_link_adam
+++ b/ast_link_adam
@@ -293,20 +293,18 @@
# "wcslib" module and the "levmar" module.
args='-last -last_wcslib -last_levmar'
-# Generate arguments for linking SLALIB.
-# --------------------------------------
- case "${sla}" in
+# Generate arguments for linking PAL.
+# -----------------------------------
-# The full proprietary C version of SLALIB has no link script, so simply
-# specify the library itself.
- c) args="${args} -lsla";;
+ case "0" in
-# For Fortran, link with the AST SLALIB interface and the Fortran library via
-# the SLALIB link script (if found).
- f) args="${args} -last_slalib `sla_link_adam`";;
+# If we configured --with-external_pal include a link option to pick up
+# an external PAL library.
+ 1) args="${args} -lpal";;
-# Otherwise, link with the internal GPLed cut down C version of SLALIB.
+# Otherwise, use the internal PAL & SOFA libraries.
*) args="${args} -last_pal";;
+
esac
# Generate arguments for linking the 2D graphics system.
diff --git a/ast_link_adam.in b/ast_link_adam.in
new file mode 100644
index 0000000..e2cd323
--- /dev/null
+++ b/ast_link_adam.in
@@ -0,0 +1,407 @@
+
+# N.B. the previous line should be blank.
+#++
+# Name:
+# ast_link_adam
+
+# Purpose:
+# Link an ADAM program with the AST library.
+
+# Type of Module:
+# Shell script.
+
+# Description:
+# This command should only be used when building Starlink ADAM programs
+# which use the AST library, in order to generate the correct arguments
+# to allow the ADAM ``alink'' command to link the program. The arguments
+# generated are written to standard output but may be substituted into
+# the ``alink'' command line in the standard UNIX way using backward
+# quotes (see below).
+#
+# By default, it is assumed that you are building an ADAM program which
+# does not produce graphical output. However, switches are provided for
+# linking other types of program. This command should not be used when
+# building stand-alone (non-ADAM) programs. Use the ``ast_link'' command
+# instead.
+
+# Invocation:
+#c alink program.o -L/star/lib `ast_link_adam [switches]`
+#f alink program.f -L/star/lib `ast_link_adam [switches]`
+
+# Switches:
+# The following switches may optionally be given to this command to
+# modify its behaviour:
+#
+# - ``-csla'': Ignored. Provided for backward compatibility only.
+#
+# - ``-fsla'': Ignored. Provided for backward compatibility only.
+#
+# - ``-grf'': Requests that no arguments be generated to specify which
+# 2D graphics system is used to display output from the AST library. You
+# should use this option only if you have implemented an interface to a
+# new graphics system yourself and wish to provide your own arguments for
+# linking with it. This switch differs from the other ``grf'' switches in
+# that it assumes that your graphics module implements the complete
+# interface required by the current version of AST. If future versions of
+# AST introduce new functions to the graphics interface, this switch will
+# cause ``unresolved symbol'' errors to occur during linking, warning you
+# that you need to implement new functions in your graphics module. To
+# avoid such errors, you can use one of the other, version-specific,
+# switches in place of the ``-grf'' switch, but these will cause run-time
+# errors to be reported if any AST function is invoked which requires
+# facilities not in the implemented interface.
+#
+# - ``-grf_v2.0'': This switch is equivalent to the ``-mygrf'' switch.
+# It indicates that you want to link with your own graphics module which
+# implements the 2D graphics interface required by V2.0 of AST.
+#
+# - ``-grf_v3.2'': Indicates that you want to link with your own graphics
+# module which implements the 2D graphics interface required by V3.2 of AST.
+#
+# - ``-grf_v5.6'': Indicates that you want to link with your own graphics
+# module which implements the 2D graphics interface required by V5.6 of AST.
+#
+# - ``-myerr'': Requests that no arguments be generated to specify how
+# error messages produced by the AST library should be delivered. You
+# should use this option only if you have implemented an interface to a
+# new error delivery system yourself and wish to provide your own
+# arguments for linking with it. By default, error messages are delivered
+# in the standard ADAM way via the EMS Error Message Service (Starlink
+# System Note SSN/4).
+#
+# - ``-mygrf'': This switch has been superceeded by the ``-grf'' switch,
+# but is retained in order to allow applications to be linked with a
+# graphics module which implements the interface used by AST V2.0. It is
+# equivalent to the ``-grf_v2.0'' switch.
+#
+# - ``-pgp'': Requests that the program be linked so that 2D
+# graphical output from the AST library is displayed via the
+# Starlink version of the PGPLOT graphics package (which uses GKS
+# for its output). By default, no graphics package is linked and
+# this will result in an error at run time if AST routines are
+# invoked that attempt to generate graphical output.
+#
+# - ``-pgplot'': Requests that the program be linked so that 2D
+# graphical output from the AST library is displayed via the
+# standard (or ``native'') version of the PGPLOT graphics
+# package. By default, no graphics package is linked and this will
+# result in an error at run time if AST routines are invoked that
+# attempt to generate graphical output.
+#
+# - ``-grf3d'': Requests that no arguments be generated to specify which
+# 3D graphics system is used to display output from the AST library. You
+# should use this option only if you have implemented an interface to a
+# new 3D graphics system yourself and wish to provide your own arguments
+# for linking with it.
+#
+# - ``-pgp3d'': Requests that the program be linked so that 3D
+# graphical output from the AST library is displayed via the
+# Starlink version of the PGPLOT graphics package (which uses GKS
+# for its output). By default, no 3D graphics package is linked and
+# this will result in an error at run time if AST routines are
+# invoked that attempt to generate graphical output.
+#
+# - ``-pgplot3d'': Requests that the program be linked so that 3D
+# graphical output from the AST library is displayed via
+# the standard (or ``native'') version of the PGPLOT graphics
+# package. By default, no 3D graphics package is linked and this will
+# result in an error at run time if AST routines are invoked that
+# attempt to generate graphical output.
+
+# SLALIB:
+# The AST distribution includes a cut down subset of the C version of
+# the SLALIB library written by Pat Wallace. This subset contains only
+# the functions needed by the AST library. It is built as part of the
+# process of building AST and is distributed under GPL (and is thus
+# compatible with the AST license). Previous version of this script
+# allowed AST applications to be linked against external SLALIB
+# libraries (either Fortran or C) rather than the internal version.
+# The current version of this script does not provide this option,
+# and always uses the internal SLALIB library. However, for backward
+# compatibility, this script still allows the "-fsla" and "-csla" flags
+# (previously used for selecting which version of SLALIB to use) to be
+# specified, but they will be ignored.
+
+# Examples:
+#c alink display.o -L/star/lib `ast_link_adam -pgplot`
+#c Links an ADAM program ``display'' which uses the standard
+#c version of PGPLOT for graphical output.
+#c alink plotit.o -L. -L/star/lib `ast_link_adam -grf` -lgrf
+#c Links an ADAM program ``plotit'', written in C. The ``-grf''
+#c switch indicates that graphical output will be delivered through
+#c a graphical interface which you have implemented yourself, which
+#c corresponds to the interface required by the current version of AST.
+#c Here, this interface is supplied by means of the ``-lgrf'' library
+#c reference.
+#c alink plotit.o -L. -L/star/lib `ast_link_adam -grf_v2.0` -lgrf
+#c Links an ADAM program ``plotit'', written in C. The ``-grf_v2.0''
+#c switch indicates that graphical output will be delivered through
+#c a graphical interface which you have implemented yourself, which
+#c corresponds to the interface required by version 2.0 of AST. Here,
+#c this interface is supplied by means of the ``-lgrf'' library
+#c reference.
+#f alink display.f -L/star/lib `ast_link_adam -pgplot`
+#f Compiles and links an ADAM Fortran program called ``display'' which
+#f uses the standard version of PGPLOT for graphical output.
+#f alink plotit.f -L. -L/star/lib `ast_link_adam -grf` -lgrf
+#f Compiles and links an ADAM Fortran program ``plotit''. The ``-grf''
+#f switch indicates that graphical output will be delivered through
+#f a graphical interface which you have implemented yourself, which
+#f corresponds to the interface required by the current version of AST.
+#f Here, this interface is supplied by means of the ``-lgrf'' library
+#f reference.
+#f alink plotit.f -L. -L/star/lib `ast_link_adam -grf_v2.0` -lgrf
+#f Compiles and links an ADAM Fortran program ``plotit''. The ``-grf_v2.0''
+#f switch indicates that graphical output will be delivered through
+#f a graphical interface which you have implemented yourself, which
+#f corresponds to the interface required by version 2.0 of AST.
+#f Here, this interface is supplied by means of the ``-lgrf'' library
+#f reference.
+
+# Copyright:
+# Copyright (C) 1997-2006 Council for the Central Laboratory of the Research Councils
+
+# Authors:
+# RFWS: R.F. Warren-Smith (STARLINK)
+# {enter_new_authors_here}
+
+# History:
+# 11-NOV-1996 (RFWS):
+# Original version.
+# 18-NOV-1997 (RFWS):
+# Adapted prologue for document extraction.
+# 28-SEP-1998 (RFWS):
+# Distinguish between -pgp and -pgplot options.
+# 23-JAN-2004 (DSB):
+# Added switches to support older grf implementations.
+# 21-APR-2005 (DSB):
+# Added "-fsla" option.
+# 16-JUN-2006 (DSB):
+# Ignore "-fsla" and "-clsa" options, and always use PAL.
+# 22-AUG-2007 (DSB):
+# Added "-grf3d", "-pgplot3d" and "-pgp3d" flags.
+# 4-MAR-2011 (DSB):
+# Added v5.6 grf options.
+# {enter_changes_here}
+
+# Bugs:
+# {note_any_bugs_here}
+
+#--
+
+# This function searches the directory path specified in PATH, looking for
+# an executable file which is not a directory. If found, it echos the full
+# file name to standard output. Otherwise, it outputs nothing.
+ find() { IFS=':'; for d in $PATH; do f="${d:=.}/${1}"
+ test -x "${f}" -a ! -d "${f}" && echo "${f}" && break
+ done;
+ }
+
+# Initialise linking options.
+ err=''
+ grf=''
+ grf3d=''
+ sla=''
+
+# Interpret command line switches.
+# --------------------------------
+ while :; do
+ case "${1}" in
+
+# -csla - Previously used to request C version of SLALIB. Now ignored.
+ -csla)
+# sla='c'
+ shift;;
+
+# -fsla - Previously used to request Fortran version of SLALIB. Now ignored.
+ -fsla)
+# sla='f'
+ shift;;
+
+# -myerr - Requests no error reporting.
+ -myerr)
+ err='my'
+ shift;;
+
+# -grf - Requests no 2D graphics.
+ -grf)
+ grf='current'
+ shift;;
+
+# -mygrf - Requests no 2D graphics, except for null implementations of
+# functions aded to the grf interface after AST V2.0.
+ -mygrf)
+ grf='v2.0'
+ shift;;
+
+# -grf_v2.0 - Requests no 2D graphics, except for null implementations of
+# functions aded to the grf interface after AST V2.0.
+ -grf_v2.0)
+ grf='v2.0'
+ shift;;
+
+# -grf_v3.2 - Requests no 2D graphics, except for null implementations of
+# functions aded to the grf interface after AST V3.2.
+ -grf_v3.2)
+ grf='v3.2'
+ shift;;
+
+# -grf_v5.6 - Requests no 2D graphics, except for null implementations of
+# functions added to the grf interface after AST V5.6.
+ -grf_v5.6)
+ grf='v5.6'
+ shift;;
+
+# -pgp - Requests 2D graphical output through Starlink PGPLOT.
+ -pgp)
+ grf='pgp'
+ shift;;
+
+# -pgplot - Requests 2D graphical output through native PGPLOT.
+ -pgplot)
+ grf='pgplot'
+ shift;;
+
+# -grf3d - Requests no 3D graphics.
+ -grf3d)
+ grf3d='current'
+ shift;;
+
+# -pgp3d - Requests 3D graphical output through Starlink PGPLOT.
+ -pgp3d)
+ grf3d='pgp'
+ shift;;
+
+# -pgplot3d - Requests 3D graphical output through native PGPLOT.
+ -pgplot3d)
+ grf3d='pgplot'
+ shift;;
+
+# Once all switches have been read, continue with the rest of the script.
+ '') break;;
+
+# Catch unrecognised switches and report an error.
+ *)
+ echo >&2 "ast_link_adam: unknown argument \""${1}"\" given"
+ exit 1;;
+ esac
+ done
+
+# Link with the main AST library.
+# -------------------------------
+# Start forming the list of arguments with the main AST library itself, the
+# "wcslib" module and the "levmar" module.
+ args='-last -last_wcslib -last_levmar'
+
+# Generate arguments for linking PAL.
+# -----------------------------------
+
+ case "@EXTERNAL_PAL@" in
+
+# If we configured --with-external_pal include a link option to pick up
+# an external PAL library.
+ 1) args="${args} -lpal";;
+
+# Otherwise, use the internal PAL & SOFA libraries.
+ *) args="${args} -last_pal";;
+
+ esac
+
+# Generate arguments for linking the 2D graphics system.
+# ------------------------------------------------------
+ case "${grf}" in
+
+# If using Starlink PGPLOT, link with the AST PGPLOT interface and
+# the Fortran library via the PGP link script.
+ pgp) args="${args} -last_pgplot `pgp_link_adam`";;
+
+# If using native PGPLOT, link with the AST PGPLOT interface and
+# the Fortran library via the PGPLOT link script.
+ pgplot) args="${args} -last_pgplot `pgplot_link_adam`";;
+
+# If using own graphics which conform to the requirements of the current
+# version of AST, do not produce any arguments.
+ current) :;;
+
+# If using own graphics which conform to the requirements of version 5.6
+# of AST, produce arguments which link in dummy implementations of any
+# functions which are required by the current version of AST but which were
+# not required by version 5.6.
+ v5.6) :;;
+
+# If using own graphics which conform to the requirements of version 3.2
+# of AST, produce arguments which link in dummy implementations of any
+# functions which are required by the current version of AST but which were
+# not required by version 3.2.
+ v3.2) args="${args} -last_grf_5.6";;
+
+# If using own graphics which conform to the requirements of version 2.0
+# of AST, produce arguments which link in dummy implementations of any
+# functions which are required by the current version of AST but which were
+# not required by version 2.0.
+ v2.0) args="${args} -last_grf_3.2 -last_grf_5.6";;
+
+# Default graphics (none) requires linking with all the default (null) AST
+# "grf" modules.
+ *) args="${args} -last_grf_2.0 -last_grf_3.2 -last_grf_5.6";;
+ esac
+
+# Generate arguments for linking the 3D graphics system.
+# ------------------------------------------------------
+ case "${grf3d}" in
+
+# If using Starlink PGPLOT, link with the AST 3D PGPLOT interface and
+# the Fortran library via the PGP link script (if found).
+ pgp) args="${args} -last_pgplot3d `\`find pgp_link\``"
+ f77='y';;
+
+# If using native PGPLOT, link with the AST 3D PGPLOT interface and the
+# Fortran library via the PGPLOT link script (if found).
+ pgplot) args="${args} -last_pgplot3d `\`find pgplot_link\``"
+ f77='y';;
+
+# If using own 3D graphics which conform to the requirements of the current
+# version of AST, do not produce any arguments.
+ current) :;;
+
+# Default graphics (none) requires linking with all the default (null) AST
+# "grf3d" modules.
+ *) args="${args} -last_grf3d";;
+ esac
+
+# Make a second pass through the AST library.
+# -------------------------------------------
+# This library is a link to the main AST library and results in a second
+# pass to resolve any backward references generated by the other modules
+# used above. A different library name must be used to avoid the two passes
+# being merged into one (either below, or by other link scripts).
+ args="${args} -last_pass2"
+
+# Generate arguments for linking the error reporting system.
+# ----------------------------------------------------------
+ case "${err}" in
+
+# If using own error reporting, do not produce any arguments.
+ my) :;;
+
+# Default error reporting requires linking with the AST EMS interface and
+# the EMS library via the link script.
+ *) args="${args} -last_ems `ems_link_adam`";;
+ esac
+
+# Link with the maths library.
+# ----------------------------
+ args="${args} -lm"
+
+# Link with the starmem library, if available.
+# --------------------------------------------
+ args="${args} `\`find starmem_link\``"
+
+# Pass the resulting argument list through an awk script which eliminates
+# all except the last reference to each library.
+ echo "${args}" \
+ | awk 'BEGIN{RS=" ";FS="\n"}
+ {if($1)f[i++]=$1}
+ END{for(;i--;)if(!w[f[i]]++)l=f[i]" "l;print l}'
+
+# End of script.
diff --git a/cmpmap.c b/cmpmap.c
index 3dcbd09..9708541 100644
--- a/cmpmap.c
+++ b/cmpmap.c
@@ -140,6 +140,9 @@ f The CmpMap class does not define any new routines beyond those
* Improve simplification of serial combinations of parellel CmpMaps.
* 25-JAN-2011 (DSB):
* Big improvement to the efficiency of the astMapSplit method.
+* 24-JAN-2012 (DSB):
+* If efficient MapSplit fails to split (e.g. due to the presence
+* of PermMaps), then revert to the older slower method.
*class--
*/
@@ -245,7 +248,9 @@ static AstMapping *Simplify( AstMapping *, int * );
static AstPointSet *Transform( AstMapping *, AstPointSet *, int, AstPointSet *, int * );
static double Rate( AstMapping *, double *, int, int, int * );
static int *MapSplit( AstMapping *, int, const int *, AstMapping **, int * );
+static int *MapSplit0( AstMapping *, int, const int *, AstMapping **, int, int * );
static int *MapSplit1( AstMapping *, int, const int *, AstMapping **, int * );
+static int *MapSplit2( AstMapping *, int, const int *, AstMapping **, int * );
static int Equal( AstObject *, AstObject *, int * );
static int GetIsLinear( AstMapping *, int * );
static int MapList( AstMapping *, int, int, int *, AstMapping ***, int **, int * );
@@ -2100,7 +2105,91 @@ static int *MapSplit1( AstMapping *this, int nin, const int *in, AstMapping **ma
* This function performs the work for the astMapSplit method. It
* first invokes the astMapSplit method to see if the forward
* transformation of the supplied Mapping (not necessarily a CmpMap)
-* can be split as requested. If this is not possible it attempts an
+* can be split as requested. If this is not possible it invokes MapSplit2
+* which attempts an inverse approach to the problem. For each possible
+* sub-sets of the Mapping outputs it call astMapSplit to see if the
+* sub-set of outputs are generated from the selected inputs.
+
+* Parameters:
+* this
+* Pointer to the Mapping to be split. It is not assumed to be a CmpMap.
+* nin
+* The number of inputs to pick from "this".
+* in
+* Pointer to an array of indices (zero based) for the inputs which
+* are to be picked. This array should have "nin" elements. If "Nin"
+* is the number of inputs of the supplied Mapping, then each element
+* should have a value in the range zero to Nin-1.
+* map
+* Address of a location at which to return a pointer to the new
+* Mapping. This Mapping will have "nin" inputs (the number of
+* outputs may be different to "nin"). A NULL pointer will be
+* returned if the supplied Mapping has no subset of outputs which
+* depend only on the selected inputs.
+
+* Returned Value:
+* A pointer to a dynamically allocated array of ints. The number of
+* elements in this array will equal the number of outputs for the
+* returned Mapping. Each element will hold the index of the
+* corresponding output in the supplied Mapping. The array should be
+* freed using astFree when no longer needed. A NULL pointer will
+* be returned if no output Mapping can be created.
+
+* Notes:
+* - If this function is invoked with the global error status set,
+* or if it should fail for any reason, then NULL values will be
+* returned as the function value and for the "map" pointer.
+*/
+
+/* Local Variables: */
+ int *result; /* Axis order to return */
+
+/* Initialise */
+ result = NULL;
+ *map = NULL;
+
+/* Check the global error status. */
+ if ( !astOK ) return result;
+
+/* First see if the forward transformation can be split as requested. */
+ result = astMapSplit( this, nin, in, map );
+
+/* If forward transformation could not be split, we attempt to split the
+ inverse transformation by selecting every possible sub-set of Mapping
+ outputs until one is found which is fed by the requested mapping inputs. */
+ if( !result ) result = MapSplit2( this, nin, in, map, status );
+
+/* Free returned resources if an error has occurred. */
+ if( !astOK ) {
+ result = astFree( result );
+ *map = astAnnul( *map );
+ }
+
+/* Return the list of output indices. */
+ return result;
+}
+
+static int *MapSplit2( AstMapping *this, int nin, const int *in, AstMapping **map, int *status ){
+/*
+* Name:
+* MapSplit2
+
+* Purpose:
+* Create a Mapping representing a subset of the inputs of an existing
+* Mapping.
+
+* Type:
+* Private function.
+
+* Synopsis:
+* #include "cmpmap.h"
+* int *MapSplit2( AstMapping *this, int nin, const int *in, AstMapping **map )
+
+* Class Membership:
+* CmpMap method
+
+* Description:
+* This function attempts to split the supplied Mapping using an
* inverse approach to the problem. For each possible sub-sets of the
* Mapping outputs it call astMapSplit to see if the sub-set of outputs
* are generated from the selected inputs.
@@ -2143,6 +2232,7 @@ static int *MapSplit1( AstMapping *this, int nin, const int *in, AstMapping **ma
int *result; /* Axis order to return */
int *result2; /* Axis order for current output subset */
int i; /* Loop count */
+ int iscmp; /* Is "this" a CmpMap? */
int j; /* Loop count */
int mout; /* Number of selected outputs */
int nin2; /* Number of inputs fed by current outputs */
@@ -2156,111 +2246,109 @@ static int *MapSplit1( AstMapping *this, int nin, const int *in, AstMapping **ma
/* Check the global error status. */
if ( !astOK ) return result;
-/* First see if the forward transformation can be split as requested. */
- result = astMapSplit( this, nin, in, map );
-
-/* If forward transformation could not be split, we attempt to split the
- inverse transformation by selecting every possible sub-set of Mapping
- outputs until one is found which is fed by the requested mapping inputs. */
- if( !result ) {
-
/* Get the number of Mapping outputs. */
- nout = astGetNout( this );
+ nout = astGetNout( this );
/* Get an inverted copy of the Mapping. We do this rather than inverting
the supplied Maping in case an error occurs which may leave the
supplied Mapping inverted. */
- this2 = astCopy( this );
- astInvert( this2 );
+ this2 = astCopy( this );
+ astInvert( this2 );
+
+/* Note if the Mapping is a CmpMap. */
+ iscmp = astIsACmpMap( this );
/* Allocate memory to hold the selected output indices. */
- out = astMalloc( nout*sizeof( int ) );
+ out = astMalloc( nout*sizeof( int ) );
/* Loop round all useful subset sizes. */
- if( out ) {
- for( mout = 1; mout < nout && !result; mout++ ) {
+ if( out ) {
+ for( mout = 1; mout < nout && !result; mout++ ) {
/* Initialise the first subset of outputs to check at the current subset
size. */
- for( i = 0; i < mout; i++ ) out[ i ] = 0;
+ for( i = 0; i < mout; i++ ) out[ i ] = 0;
/* Loop round all ways of picking a subset of "mout" outputs from the total
available "nout" outputs. */
- while( ! result ) {
+ while( ! result ) {
/* Skip this subset if it refers to any axis index more than once. */
- ok = 1;
- for( i = 1; i < mout && ok; i++ ) {
- for( j = 0; j < i; j++ ) {
- if( out[ i ] == out[ j ] ) {
- ok = 0;
- break;
- }
+ ok = 1;
+ for( i = 1; i < mout && ok; i++ ) {
+ for( j = 0; j < i; j++ ) {
+ if( out[ i ] == out[ j ] ) {
+ ok = 0;
+ break;
}
}
- if( ok ) {
+ }
+ if( ok ) {
/* Attempt to split the inverted Mapping using the current subset of
- outputs. */
+ outputs. Take care to avoid an infinite loop if "this" is a CmpMap. */
+ if( iscmp ) {
+ result2 = MapSplit0( this2, mout, out, &map2, 1, status );
+ } else {
result2 = astMapSplit( this2, mout, out, &map2 );
+ }
/* If succesful... */
- if( result2 ) {
+ if( result2 ) {
/* See if the inputs that feed the current subset of outputs are the same
as the inputs specified by the caller (and in the same order). */
- nin2 = astGetNout( map2 );
- ok = ( nin2 == nin );
- if( ok ) {
- for( i = 0; i < nin; i++ ) {
- if( in[ i ] != result2[ i ] ) {
- ok = 0;
- break;
- }
+ nin2 = astGetNout( map2 );
+ ok = ( nin2 == nin );
+ if( ok ) {
+ for( i = 0; i < nin; i++ ) {
+ if( in[ i ] != result2[ i ] ) {
+ ok = 0;
+ break;
}
}
+ }
/* If so, set up the values returned to the caller. */
- if( ok ) {
- result = astStore( result, out, mout*sizeof(int) );
- astInvert( map2 );
- *map = astClone( map2 );
- }
+ if( ok ) {
+ result = astStore( result, out, mout*sizeof(int) );
+ astInvert( map2 );
+ *map = astClone( map2 );
+ }
/* Free resources. */
- result2 = astFree( result2 );
- map2 = astAnnul( map2 );
- }
+ result2 = astFree( result2 );
+ map2 = astAnnul( map2 );
}
+ }
/* Increment the first axis index. */
- i = 0;
- out[ i ]++;
+ i = 0;
+ out[ i ]++;
/* If the incremented axis index is now too high, reset it to zero and
increment the next higher axis index. Do this until an incremented axis
index is not too high. */
- while( out[ i ] == nout ) {
- out[ i++ ] = 0;
+ while( out[ i ] == nout ) {
+ out[ i++ ] = 0;
- if( i < mout ) {
- out[ i ]++;
- } else {
- break;
- }
+ if( i < mout ) {
+ out[ i ]++;
+ } else {
+ break;
}
+ }
/* If all subsets have been checked break out of the loop. */
- if( i == mout ) break;
+ if( i == mout ) break;
- }
}
}
+ }
/* Free resources. */
- out = astFree( out );
- this2 = astAnnul( this2 );
- }
+ out = astFree( out );
+ this2 = astAnnul( this2 );
/* Free returned resources if an error has occurred. */
if( !astOK ) {
@@ -2272,11 +2360,11 @@ static int *MapSplit1( AstMapping *this, int nin, const int *in, AstMapping **ma
return result;
}
-static int *MapSplit( AstMapping *this_mapping, int nin, const int *in,
- AstMapping **map, int *status ){
+static int *MapSplit0( AstMapping *this_mapping, int nin, const int *in,
+ AstMapping **map, int reentry, int *status ){
/*
* Name:
-* MapSplit
+* MapSplit0
* Purpose:
* Create a Mapping representing a subset of the inputs of an existing
@@ -2287,12 +2375,11 @@ static int *MapSplit( AstMapping *this_mapping, int nin, const int *in,
* Synopsis:
* #include "cmpmap.h"
-* int *MapSplit( AstMapping *this, int nin, const int *in,
-* AstMapping **map, int *status )
+* int *MapSplit0( AstMapping *this, int nin, const int *in,
+* AstMapping **map, int reentry, int *status )
* Class Membership:
-* CmpMap method (over-rides the protected astMapSplit method
-* inherited from the Mapping class).
+* CmpMap method
* Description:
* This function creates a new Mapping by picking specified inputs from
@@ -2320,6 +2407,9 @@ static int *MapSplit( AstMapping *this_mapping, int nin, const int *in,
* outputs may be different to "nin"). A NULL pointer will be
* returned if the supplied CmpMap has no subset of outputs which
* depend only on the selected inputs.
+* reentry
+* Set to zero if this is a top level entry, and non-zero if it is
+* a recursive entry.
* status
* Pointer to the inherited status variable.
@@ -2629,6 +2719,12 @@ static int *MapSplit( AstMapping *this_mapping, int nin, const int *in,
/* Mappings that have no outputs cannot be used. */
if( !result && *map ) *map = astAnnul( *map );
+/* If the above method failed to split the CmpMap, we attempt to split the
+ inverse transformation by selecting every possible sub-set of Mapping
+ outputs until one is found which is fed by the requested mapping inputs. */
+ if( !result && !reentry ) result = MapSplit2( this_mapping, nin, in, map,
+ status );
+
/* Free returned resources if an error has occurred. */
if( !astOK ) {
result = astFree( result );
@@ -2639,6 +2735,69 @@ static int *MapSplit( AstMapping *this_mapping, int nin, const int *in,
return result;
}
+static int *MapSplit( AstMapping *this, int nin, const int *in,
+ AstMapping **map, int *status ){
+/*
+* Name:
+* MapSplit
+
+* Purpose:
+* Create a Mapping representing a subset of the inputs of an existing
+* CmpMap.
+
+* Type:
+* Private function.
+
+* Synopsis:
+* #include "cmpmap.h"
+* int *MapSplit( AstMapping *this, int nin, const int *in,
+* AstMapping **map, int *status )
+
+* Class Membership:
+* CmpMap method (over-rides the protected astMapSplit method
+* inherited from the Mapping class).
+
+* Description:
+* This function is the main entry point for the astMapSplit method.
+* It is a simple wrapper for MapSplit0 which calls MapSplit0
+* indicating that this is a top-level entry.
+
+* Parameters:
+* this
+* Pointer to the CmpMap to be split (the CmpMap is not actually
+* modified by this function).
+* nin
+* The number of inputs to pick from "this".
+* in
+* Pointer to an array of indices (zero based) for the inputs which
+* are to be picked. This array should have "nin" elements. If "Nin"
+* is the number of inputs of the supplied CmpMap, then each element
+* should have a value in the range zero to Nin-1.
+* map
+* Address of a location at which to return a pointer to the new
+* Mapping. This Mapping will have "nin" inputs (the number of
+* outputs may be different to "nin"). A NULL pointer will be
+* returned if the supplied CmpMap has no subset of outputs which
+* depend only on the selected inputs.
+* status
+* Pointer to the inherited status variable.
+
+* Returned Value:
+* A pointer to a dynamically allocated array of ints. The number of
+* elements in this array will equal the number of outputs for the
+* returned Mapping. Each element will hold the index of the
+* corresponding output in the supplied CmpMap. The array should be
+* freed using astFree when no longer needed. A NULL pointer will
+* be returned if no output Mapping can be created.
+
+* Notes:
+* - If this function is invoked with the global error status set,
+* or if it should fail for any reason, then NULL values will be
+* returned as the function value and for the "map" pointer.
+*/
+ return MapSplit0( this, nin, in, map, 0, status );
+}
+
static int PatternCheck( int val, int check, int **list, int *list_len, int *status ){
/*
* Name:
@@ -3276,11 +3435,11 @@ static AstMapping *Simplify( AstMapping *this_mapping, int *status ) {
wlen2 = PatternCheck( nmap, wlen1, &nlist, &nlist_len, status );
if( wlen1 && wlen2 ) {
-/* Ensure wlen2 is larger tnan or equal to wlen1. */
+/* Ensure wlen2 is larger than or equal to wlen1. */
if( wlen1 > wlen2 ) {
t = wlen1;
wlen1 = wlen2;
- wlen2 = wlen1;
+ wlen2 = t;
}
/* See if wlen2 is an integer multiple of wlen1. If not, ignore the
diff --git a/config.h.in b/config.h.in
index 50a5837..bfddb40 100644
--- a/config.h.in
+++ b/config.h.in
@@ -1,5 +1,8 @@
/* config.h.in. Generated from configure.ac by autoheader. */
+/* use external PAL and SOFA libraries */
+#undef EXTERNAL_PAL
+
/* Define to 1 if you have the `backtrace' function. */
#undef HAVE_BACKTRACE
diff --git a/configure b/configure
index fd2b401..b0bb155 100755
--- a/configure
+++ b/configure
@@ -1,7 +1,7 @@
#! /bin/sh
# From configure.ac Revision.
# Guess values for system-dependent variables and create Makefiles.
-# Generated by Starlink Autoconf 2.59 for ast 6.0.1.
+# Generated by Starlink Autoconf 2.59 for ast 7.0.0.
#
# Report bugs to <ussc at star.rl.ac.uk>.
#
@@ -424,8 +424,8 @@ SHELL=${CONFIG_SHELL-/bin/sh}
# Identity of this package.
PACKAGE_NAME='ast'
PACKAGE_TARNAME='ast'
-PACKAGE_VERSION='6.0.1'
-PACKAGE_STRING='ast 6.0.1'
+PACKAGE_VERSION='7.0.0'
+PACKAGE_STRING='ast 7.0.0'
PACKAGE_BUGREPORT='ussc at star.rl.ac.uk'
ac_unique_file="ast_link.in"
@@ -467,7 +467,7 @@ ac_includes_default="\
# include <unistd.h>
#endif"
-ac_subst_vars='SHELL PATH_SEPARATOR PACKAGE_NAME PACKAGE_TARNAME PACKAGE_VERSION PACKAGE_STRING PACKAGE_BUGREPORT exec_prefix prefix program_transform_name bindir sbindir libexecdir datadir sysconfdir sharedstatedir localstatedir libdir includedir oldincludedir infodir mandir build_alias host_alias target_alias DEFS ECHO_C ECHO_N ECHO_T LIBS INSTALL_PROGRAM INSTALL_SCRIPT INSTALL_DATA CYGPATH_W PACKAGE VERSION ACLOCAL AUTOCONF AUTOMAKE AUTOHEADER MAKEINFO install_sh STRIP ac_ct_STRIP INSTALL_STRIP_PROGRAM mkdir_p AWK SET_MAKE am__leading_dot AMTAR am__tar am__untar STARLINK STAR_CPPFLAGS STAR_FCFLAGS STAR_FFLAGS STAR_LDFLAGS build build_cpu build_vendor build_os CC CFLAGS LDFLAGS CPPFLAGS ac_ct_CC EXEEXT OBJEXT DEPDIR am__include am__quote AMDEP_TRUE AMDEP_FALSE AMDEPBACKSLASH CCDEPMODE am__fastdepCC_TRUE am__fastdepCC_FALSE FC FCFLAGS ac_ct_FC C_FC_FCLINK_MAGIC C_FC_PPFC_FCLINK_MAGIC stardocsdir staretcdir starexamplesdir starfacsdir starhelpdir starnewsdir STAR_DEPENDENCIES_ATTRIBUTES STAR_DEPENDENCIES_CHILDREN STAR_DOCUMENTATION PACKAGE_VERSION_MAJOR PACKAGE_VERSION_MINOR PACKAGE_VERSION_RELEASE PACKAGE_VERSION_INTEGER STAR_MANIFEST_DIR GIT STAR_SOURCE_ROOT_DIR PREDIST PAX TAR CPP host host_cpu host_vendor host_os EGREP LN_S ECHO AR ac_ct_AR RANLIB ac_ct_RANLIB CXX CXXFLAGS ac_ct_CXX CXXDEPMODE am__fastdepCXX_TRUE am__fastdepCXX_FALSE CXXCPP F77 FFLAGS ac_ct_F77 LIBTOOL NOPIC_TRUE NOPIC_FALSE NOTHREADS_TRUE NOTHREADS_FALSE THREADS FCLIBS PERL REAL_FUNCTION_TYPE TRAIL_TYPE MESSGEN LATEX2DVI STAR_LATEX_DOCUMENTATION STAR2HTML PROLAT LIBOBJS LTLIBOBJS'
+ac_subst_vars='SHELL PATH_SEPARATOR PACKAGE_NAME PACKAGE_TARNAME PACKAGE_VERSION PACKAGE_STRING PACKAGE_BUGREPORT exec_prefix prefix program_transform_name bindir sbindir libexecdir datadir sysconfdir sharedstatedir localstatedir libdir includedir oldincludedir infodir mandir build_alias host_alias target_alias DEFS ECHO_C ECHO_N ECHO_T LIBS INSTALL_PROGRAM INSTALL_SCRIPT INSTALL_DATA CYGPATH_W PACKAGE VERSION ACLOCAL AUTOCONF AUTOMAKE AUTOHEADER MAKEINFO install_sh STRIP ac_ct_STRIP INSTALL_STRIP_PROGRAM mkdir_p AWK SET_MAKE am__leading_dot AMTAR am__tar am__untar STARLINK STAR_CPPFLAGS STAR_FCFLAGS STAR_FFLAGS STAR_LDFLAGS build build_cpu build_vendor build_os CC CFLAGS LDFLAGS CPPFLAGS ac_ct_CC EXEEXT OBJEXT DEPDIR am__include am__quote AMDEP_TRUE AMDEP_FALSE AMDEPBACKSLASH CCDEPMODE am__fastdepCC_TRUE am__fastdepCC_FALSE FC FCFLAGS ac_ct_FC C_FC_FCLINK_MAGIC C_FC_PPFC_FCLINK_MAGIC stardocsdir staretcdir starexamplesdir starfacsdir starhelpdir starnewsdir STAR_DEPENDENCIES_ATTRIBUTES STAR_DEPENDENCIES_CHILDREN STAR_DOCUMENTATION PACKAGE_VERSION_MAJOR PACKAGE_VERSION_MINOR PACKAGE_VERSION_RELEASE PACKAGE_VERSION_INTEGER STAR_MANIFEST_DIR GIT STAR_SOURCE_ROOT_DIR PREDIST PAX TAR EXTERNAL_PAL LIBPAL EXTERNAL_PAL_TRUE EXTERNAL_PAL_FALSE CPP host host_cpu host_vendor host_os EGREP LN_S ECHO AR ac_ct_AR RANLIB ac_ct_RANLIB CXX CXXFLAGS ac_ct_CXX CXXDEPMODE am__fastdepCXX_TRUE am__fastdepCXX_FALSE CXXCPP F77 FFLAGS ac_ct_F77 LIBTOOL NOPIC_TRUE NOPIC_FALSE NOTHREADS_TRUE NOTHREADS_FALSE THREADS FCLIBS PERL REAL_FUNCTION_TYPE TRAIL_TYPE MESSGEN LATEX2DVI STAR_LATEX_DOCUMENTATION STAR2HTML PROLAT LIBOBJS LTLIBOBJS'
ac_subst_files=''
# Initialize some variables set by options.
@@ -980,7 +980,7 @@ if test "$ac_init_help" = "long"; then
# Omit some internal or obsolete options to make the list less imposing.
# This message is too long to be a string in the A/UX 3.1 sh.
cat <<_ACEOF
-\`configure' configures ast 6.0.1 to adapt to many kinds of systems.
+\`configure' configures ast 7.0.0 to adapt to many kinds of systems.
Usage: $0 [OPTION]... [VAR=VALUE]...
@@ -1046,7 +1046,7 @@ fi
if test -n "$ac_init_help"; then
case $ac_init_help in
- short | recursive ) echo "Configuration of ast 6.0.1:";;
+ short | recursive ) echo "Configuration of ast 7.0.0:";;
esac
cat <<\_ACEOF
@@ -1071,6 +1071,7 @@ Optional Packages:
--without-stardocs Do not install built documentation (default --with)
--with-starmem use starmem library for memory management
--with-memdebug enable AST memory leak debugging functions
+ --with-external_pal Use external PAL and SOFA libraries
--with-gnu-ld assume the C compiler uses GNU ld [default=no]
--with-pic try to use only PIC/non-PIC objects [default=use
both]
@@ -1197,7 +1198,7 @@ fi
test -n "$ac_init_help" && exit 0
if $ac_init_version; then
cat <<\_ACEOF
-ast configure 6.0.1
+ast configure 7.0.0
generated by Starlink Autoconf 2.59
Copyright (C) 2003 Free Software Foundation, Inc.
@@ -1211,7 +1212,7 @@ cat >&5 <<_ACEOF
This file contains any messages produced by compilers while
running configure, to aid debugging if configure makes a mistake.
-It was created by ast $as_me 6.0.1, which was
+It was created by ast $as_me 7.0.0, which was
generated by Starlink Autoconf 2.59. Invocation command line was
$ $0 $@
@@ -1856,7 +1857,7 @@ fi
# Define the identity of the package.
PACKAGE='ast'
- VERSION='6.0.1'
+ VERSION='7.0.0'
cat >>confdefs.h <<_ACEOF
@@ -3218,7 +3219,7 @@ fi
# Provide some information about the compiler.
-echo "$as_me:3221:" \
+echo "$as_me:3222:" \
"checking for Fortran compiler version" >&5
ac_compiler=`set X $ac_compile; echo $2`
{ (eval echo "$as_me:$LINENO: \"$ac_compiler --version </dev/null >&5\"") >&5
@@ -3971,6 +3972,48 @@ _ACEOF
fi;
+# See if the --with-external_pal option has been provided. This sets the
+# preprocesor macro EXTERNAL_PAL which prevents use of the PAL & SOFA
+# library functions that are include din the AST distribution. Suitable
+# link options are used within ast_link(_adam) scripts to pull in libpal.
+
+# Check whether --with-external_pal or --without-external_pal was given.
+if test "${with_external_pal+set}" = set; then
+ withval="$with_external_pal"
+ if test "$withval" = "yes"; then
+ external_pal="1"
+ else
+ external_pal="0"
+ fi
+else
+ external_pal="0"
+fi;
+EXTERNAL_PAL=$external_pal
+
+if test "$external_pal" = "1"; then
+ LIBPAL="-lpal"
+
+
+cat >>confdefs.h <<\_ACEOF
+#define EXTERNAL_PAL 1
+_ACEOF
+,
+else
+ LIBPAL=""
+
+fi
+
+
+if test x$external_pal = x1; then
+ EXTERNAL_PAL_TRUE=
+ EXTERNAL_PAL_FALSE='#'
+else
+ EXTERNAL_PAL_TRUE='#'
+ EXTERNAL_PAL_FALSE=
+fi
+
+
+
# Checks for programs
ac_ext=c
ac_cpp='$CPP $CPPFLAGS'
@@ -5618,7 +5661,7 @@ ia64-*-hpux*)
;;
*-*-irix6*)
# Find out which ABI we are using.
- echo '#line 5621 "configure"' > conftest.$ac_ext
+ echo '#line 5664 "configure"' > conftest.$ac_ext
if { (eval echo "$as_me:$LINENO: \"$ac_compile\"") >&5
(eval $ac_compile) 2>&5
ac_status=$?
@@ -6963,7 +7006,7 @@ fi
# Provide some information about the compiler.
-echo "$as_me:6966:" \
+echo "$as_me:7009:" \
"checking for Fortran 77 compiler version" >&5
ac_compiler=`set X $ac_compile; echo $2`
{ (eval echo "$as_me:$LINENO: \"$ac_compiler --version </dev/null >&5\"") >&5
@@ -8117,11 +8160,11 @@ else
-e 's:.*FLAGS}? :&$lt_compiler_flag :; t' \
-e 's: [^ ]*conftest\.: $lt_compiler_flag&:; t' \
-e 's:$: $lt_compiler_flag:'`
- (eval echo "\"\$as_me:8120: $lt_compile\"" >&5)
+ (eval echo "\"\$as_me:8163: $lt_compile\"" >&5)
(eval "$lt_compile" 2>conftest.err)
ac_status=$?
cat conftest.err >&5
- echo "$as_me:8124: \$? = $ac_status" >&5
+ echo "$as_me:8167: \$? = $ac_status" >&5
if (exit $ac_status) && test -s "$ac_outfile"; then
# The compiler can only warn and ignore the option if not recognized
# So say no if there are warnings other than the usual output.
@@ -8379,11 +8422,11 @@ else
-e 's:.*FLAGS}? :&$lt_compiler_flag :; t' \
-e 's: [^ ]*conftest\.: $lt_compiler_flag&:; t' \
-e 's:$: $lt_compiler_flag:'`
- (eval echo "\"\$as_me:8382: $lt_compile\"" >&5)
+ (eval echo "\"\$as_me:8425: $lt_compile\"" >&5)
(eval "$lt_compile" 2>conftest.err)
ac_status=$?
cat conftest.err >&5
- echo "$as_me:8386: \$? = $ac_status" >&5
+ echo "$as_me:8429: \$? = $ac_status" >&5
if (exit $ac_status) && test -s "$ac_outfile"; then
# The compiler can only warn and ignore the option if not recognized
# So say no if there are warnings other than the usual output.
@@ -8441,11 +8484,11 @@ else
-e 's:.*FLAGS}? :&$lt_compiler_flag :; t' \
-e 's: [^ ]*conftest\.: $lt_compiler_flag&:; t' \
-e 's:$: $lt_compiler_flag:'`
- (eval echo "\"\$as_me:8444: $lt_compile\"" >&5)
+ (eval echo "\"\$as_me:8487: $lt_compile\"" >&5)
(eval "$lt_compile" 2>out/conftest.err)
ac_status=$?
cat out/conftest.err >&5
- echo "$as_me:8448: \$? = $ac_status" >&5
+ echo "$as_me:8491: \$? = $ac_status" >&5
if (exit $ac_status) && test -s out/conftest2.$ac_objext
then
# The compiler can only warn and ignore the option if not recognized
@@ -10686,7 +10729,7 @@ else
lt_dlunknown=0; lt_dlno_uscore=1; lt_dlneed_uscore=2
lt_status=$lt_dlunknown
cat > conftest.$ac_ext <<EOF
-#line 10689 "configure"
+#line 10732 "configure"
#include "confdefs.h"
#if HAVE_DLFCN_H
@@ -10784,7 +10827,7 @@ else
lt_dlunknown=0; lt_dlno_uscore=1; lt_dlneed_uscore=2
lt_status=$lt_dlunknown
cat > conftest.$ac_ext <<EOF
-#line 10787 "configure"
+#line 10830 "configure"
#include "confdefs.h"
#if HAVE_DLFCN_H
@@ -13032,11 +13075,11 @@ else
-e 's:.*FLAGS}? :&$lt_compiler_flag :; t' \
-e 's: [^ ]*conftest\.: $lt_compiler_flag&:; t' \
-e 's:$: $lt_compiler_flag:'`
- (eval echo "\"\$as_me:13035: $lt_compile\"" >&5)
+ (eval echo "\"\$as_me:13078: $lt_compile\"" >&5)
(eval "$lt_compile" 2>conftest.err)
ac_status=$?
cat conftest.err >&5
- echo "$as_me:13039: \$? = $ac_status" >&5
+ echo "$as_me:13082: \$? = $ac_status" >&5
if (exit $ac_status) && test -s "$ac_outfile"; then
# The compiler can only warn and ignore the option if not recognized
# So say no if there are warnings other than the usual output.
@@ -13094,11 +13137,11 @@ else
-e 's:.*FLAGS}? :&$lt_compiler_flag :; t' \
-e 's: [^ ]*conftest\.: $lt_compiler_flag&:; t' \
-e 's:$: $lt_compiler_flag:'`
- (eval echo "\"\$as_me:13097: $lt_compile\"" >&5)
+ (eval echo "\"\$as_me:13140: $lt_compile\"" >&5)
(eval "$lt_compile" 2>out/conftest.err)
ac_status=$?
cat out/conftest.err >&5
- echo "$as_me:13101: \$? = $ac_status" >&5
+ echo "$as_me:13144: \$? = $ac_status" >&5
if (exit $ac_status) && test -s out/conftest2.$ac_objext
then
# The compiler can only warn and ignore the option if not recognized
@@ -14463,7 +14506,7 @@ else
lt_dlunknown=0; lt_dlno_uscore=1; lt_dlneed_uscore=2
lt_status=$lt_dlunknown
cat > conftest.$ac_ext <<EOF
-#line 14466 "configure"
+#line 14509 "configure"
#include "confdefs.h"
#if HAVE_DLFCN_H
@@ -14561,7 +14604,7 @@ else
lt_dlunknown=0; lt_dlno_uscore=1; lt_dlneed_uscore=2
lt_status=$lt_dlunknown
cat > conftest.$ac_ext <<EOF
-#line 14564 "configure"
+#line 14607 "configure"
#include "confdefs.h"
#if HAVE_DLFCN_H
@@ -15446,11 +15489,11 @@ else
-e 's:.*FLAGS}? :&$lt_compiler_flag :; t' \
-e 's: [^ ]*conftest\.: $lt_compiler_flag&:; t' \
-e 's:$: $lt_compiler_flag:'`
- (eval echo "\"\$as_me:15449: $lt_compile\"" >&5)
+ (eval echo "\"\$as_me:15492: $lt_compile\"" >&5)
(eval "$lt_compile" 2>conftest.err)
ac_status=$?
cat conftest.err >&5
- echo "$as_me:15453: \$? = $ac_status" >&5
+ echo "$as_me:15496: \$? = $ac_status" >&5
if (exit $ac_status) && test -s "$ac_outfile"; then
# The compiler can only warn and ignore the option if not recognized
# So say no if there are warnings other than the usual output.
@@ -15508,11 +15551,11 @@ else
-e 's:.*FLAGS}? :&$lt_compiler_flag :; t' \
-e 's: [^ ]*conftest\.: $lt_compiler_flag&:; t' \
-e 's:$: $lt_compiler_flag:'`
- (eval echo "\"\$as_me:15511: $lt_compile\"" >&5)
+ (eval echo "\"\$as_me:15554: $lt_compile\"" >&5)
(eval "$lt_compile" 2>out/conftest.err)
ac_status=$?
cat out/conftest.err >&5
- echo "$as_me:15515: \$? = $ac_status" >&5
+ echo "$as_me:15558: \$? = $ac_status" >&5
if (exit $ac_status) && test -s out/conftest2.$ac_objext
then
# The compiler can only warn and ignore the option if not recognized
@@ -17635,11 +17678,11 @@ else
-e 's:.*FLAGS}? :&$lt_compiler_flag :; t' \
-e 's: [^ ]*conftest\.: $lt_compiler_flag&:; t' \
-e 's:$: $lt_compiler_flag:'`
- (eval echo "\"\$as_me:17638: $lt_compile\"" >&5)
+ (eval echo "\"\$as_me:17681: $lt_compile\"" >&5)
(eval "$lt_compile" 2>conftest.err)
ac_status=$?
cat conftest.err >&5
- echo "$as_me:17642: \$? = $ac_status" >&5
+ echo "$as_me:17685: \$? = $ac_status" >&5
if (exit $ac_status) && test -s "$ac_outfile"; then
# The compiler can only warn and ignore the option if not recognized
# So say no if there are warnings other than the usual output.
@@ -17897,11 +17940,11 @@ else
-e 's:.*FLAGS}? :&$lt_compiler_flag :; t' \
-e 's: [^ ]*conftest\.: $lt_compiler_flag&:; t' \
-e 's:$: $lt_compiler_flag:'`
- (eval echo "\"\$as_me:17900: $lt_compile\"" >&5)
+ (eval echo "\"\$as_me:17943: $lt_compile\"" >&5)
(eval "$lt_compile" 2>conftest.err)
ac_status=$?
cat conftest.err >&5
- echo "$as_me:17904: \$? = $ac_status" >&5
+ echo "$as_me:17947: \$? = $ac_status" >&5
if (exit $ac_status) && test -s "$ac_outfile"; then
# The compiler can only warn and ignore the option if not recognized
# So say no if there are warnings other than the usual output.
@@ -17959,11 +18002,11 @@ else
-e 's:.*FLAGS}? :&$lt_compiler_flag :; t' \
-e 's: [^ ]*conftest\.: $lt_compiler_flag&:; t' \
-e 's:$: $lt_compiler_flag:'`
- (eval echo "\"\$as_me:17962: $lt_compile\"" >&5)
+ (eval echo "\"\$as_me:18005: $lt_compile\"" >&5)
(eval "$lt_compile" 2>out/conftest.err)
ac_status=$?
cat out/conftest.err >&5
- echo "$as_me:17966: \$? = $ac_status" >&5
+ echo "$as_me:18009: \$? = $ac_status" >&5
if (exit $ac_status) && test -s out/conftest2.$ac_objext
then
# The compiler can only warn and ignore the option if not recognized
@@ -20204,7 +20247,7 @@ else
lt_dlunknown=0; lt_dlno_uscore=1; lt_dlneed_uscore=2
lt_status=$lt_dlunknown
cat > conftest.$ac_ext <<EOF
-#line 20207 "configure"
+#line 20250 "configure"
#include "confdefs.h"
#if HAVE_DLFCN_H
@@ -20302,7 +20345,7 @@ else
lt_dlunknown=0; lt_dlno_uscore=1; lt_dlneed_uscore=2
lt_status=$lt_dlunknown
cat > conftest.$ac_ext <<EOF
-#line 20305 "configure"
+#line 20348 "configure"
#include "confdefs.h"
#if HAVE_DLFCN_H
@@ -22113,7 +22156,7 @@ _ACEOF
# flags.
ac_save_FFLAGS=$FCFLAGS
FCFLAGS="$FCFLAGS $ac_verb"
-(eval echo $as_me:22116: \"$ac_link\") >&5
+(eval echo $as_me:22159: \"$ac_link\") >&5
ac_fc_v_output=`eval $ac_link 5>&1 2>&1 | grep -v 'Driving:'`
echo "$ac_fc_v_output" >&5
FCFLAGS=$ac_save_FFLAGS
@@ -22191,7 +22234,7 @@ _ACEOF
# flags.
ac_save_FFLAGS=$FCFLAGS
FCFLAGS="$FCFLAGS $ac_cv_prog_fc_v"
-(eval echo $as_me:22194: \"$ac_link\") >&5
+(eval echo $as_me:22237: \"$ac_link\") >&5
ac_fc_v_output=`eval $ac_link 5>&1 2>&1 | grep -v 'Driving:'`
echo "$ac_fc_v_output" >&5
FCFLAGS=$ac_save_FFLAGS
@@ -22592,11 +22635,6 @@ fi
STAR_DEPENDENCIES_CHILDREN="$STAR_DEPENDENCIES_CHILDREN<sourceset>$_star_tmp</sourceset>"
done
- for _star_tmp in sla
- do
- STAR_DEPENDENCIES_CHILDREN="$STAR_DEPENDENCIES_CHILDREN<build>$_star_tmp</build>"
- done
-
# Perform the check that configures f77.h.in for the return type of REAL
# Fortran functions. On 64-bit g77 with f2c compatibility this is double
@@ -23619,7 +23657,7 @@ fi
ac_config_headers="$ac_config_headers config.h"
- ac_config_files="$ac_config_files Makefile component.xml ast_link object.h f77.h"
+ ac_config_files="$ac_config_files Makefile component.xml ast_link ast_link_adam object.h f77.h"
ac_config_files="$ac_config_files ast_cpp"
@@ -23778,6 +23816,13 @@ echo "$as_me: error: conditional \"am__fastdepCC\" was never defined.
Usually this means the macro was only invoked conditionally." >&2;}
{ (exit 1); exit 1; }; }
fi
+if test -z "${EXTERNAL_PAL_TRUE}" && test -z "${EXTERNAL_PAL_FALSE}"; then
+ { { echo "$as_me:$LINENO: error: conditional \"EXTERNAL_PAL\" was never defined.
+Usually this means the macro was only invoked conditionally." >&5
+echo "$as_me: error: conditional \"EXTERNAL_PAL\" was never defined.
+Usually this means the macro was only invoked conditionally." >&2;}
+ { (exit 1); exit 1; }; }
+fi
if test -z "${am__fastdepCC_TRUE}" && test -z "${am__fastdepCC_FALSE}"; then
{ { echo "$as_me:$LINENO: error: conditional \"am__fastdepCC\" was never defined.
Usually this means the macro was only invoked conditionally." >&5
@@ -24077,7 +24122,7 @@ _ASBOX
} >&5
cat >&5 <<_CSEOF
-This file was extended by ast $as_me 6.0.1, which was
+This file was extended by ast $as_me 7.0.0, which was
generated by Starlink Autoconf 2.59. Invocation command line was
CONFIG_FILES = $CONFIG_FILES
@@ -24140,7 +24185,7 @@ _ACEOF
cat >>$CONFIG_STATUS <<_ACEOF
ac_cs_version="\\
-ast config.status 6.0.1
+ast config.status 7.0.0
configured by $0, generated by Starlink Autoconf 2.59,
with options \\"`echo "$ac_configure_args" | sed 's/[\\""\`\$]/\\\\&/g'`\\"
@@ -24253,6 +24298,7 @@ do
"Makefile" ) CONFIG_FILES="$CONFIG_FILES Makefile" ;;
"component.xml" ) CONFIG_FILES="$CONFIG_FILES component.xml" ;;
"ast_link" ) CONFIG_FILES="$CONFIG_FILES ast_link" ;;
+ "ast_link_adam" ) CONFIG_FILES="$CONFIG_FILES ast_link_adam" ;;
"object.h" ) CONFIG_FILES="$CONFIG_FILES object.h" ;;
"f77.h" ) CONFIG_FILES="$CONFIG_FILES f77.h" ;;
"ast_cpp" ) CONFIG_FILES="$CONFIG_FILES ast_cpp" ;;
@@ -24414,6 +24460,10 @@ s, at STAR_SOURCE_ROOT_DIR@,$STAR_SOURCE_ROOT_DIR,;t t
s, at PREDIST@,$PREDIST,;t t
s, at PAX@,$PAX,;t t
s, at TAR@,$TAR,;t t
+s, at EXTERNAL_PAL@,$EXTERNAL_PAL,;t t
+s, at LIBPAL@,$LIBPAL,;t t
+s, at EXTERNAL_PAL_TRUE@,$EXTERNAL_PAL_TRUE,;t t
+s, at EXTERNAL_PAL_FALSE@,$EXTERNAL_PAL_FALSE,;t t
s, at CPP@,$CPP,;t t
s, at host@,$host,;t t
s, at host_cpu@,$host_cpu,;t t
diff --git a/configure.ac b/configure.ac
index 0ff1ae4..1b3b3b0 100644
--- a/configure.ac
+++ b/configure.ac
@@ -7,7 +7,7 @@ dnl 1.5. It should work with autoconf versions 2.50 or better, and
dnl automake 1.6 or better.
dnl Initialisation: package name and version number
-AC_INIT(ast, 6.0.1, ussc at star.rl.ac.uk)
+AC_INIT(ast, 7.0.0, ussc at star.rl.ac.uk)
dnl Require autoconf-2.50 at least
AC_PREREQ(2.50)
@@ -39,6 +39,28 @@ AC_ARG_WITH(
AC_DEFINE([MEM_DEBUG],[1],[enable AST memory leak debugging functions in memory.c]),
)
+# See if the --with-external_pal option has been provided. This sets the
+# preprocesor macro EXTERNAL_PAL which prevents use of the PAL & SOFA
+# library functions that are include din the AST distribution. Suitable
+# link options are used within ast_link(_adam) scripts to pull in libpal.
+AC_ARG_WITH([external_pal],
+ [ --with-external_pal Use external PAL and SOFA libraries],
+ if test "$withval" = "yes"; then
+ external_pal="1"
+ else
+ external_pal="0"
+ fi,
+ external_pal="0")
+AC_SUBST( EXTERNAL_PAL, $external_pal )
+if test "$external_pal" = "1"; then
+ AC_SUBST( LIBPAL, "-lpal" )
+ AC_DEFINE([EXTERNAL_PAL],[1],[use external PAL and SOFA libraries]),
+else
+ AC_SUBST( LIBPAL, "" )
+fi
+AM_CONDITIONAL(EXTERNAL_PAL, test x$external_pal = x1)
+
+
# Checks for programs
AC_PROG_CC
AC_PROG_CPP
@@ -91,7 +113,6 @@ AC_CHECK_FUNCS([isnan])
AC_CHECK_DECLS([isnan],,,[#include <math.h>
])
STAR_DECLARE_DEPENDENCIES(sourceset, [sst htx])
-STAR_DECLARE_DEPENDENCIES(build, sla)
# Perform the check that configures f77.h.in for the return type of REAL
# Fortran functions. On 64-bit g77 with f2c compatibility this is double
@@ -151,7 +172,7 @@ STAR_CHECK_PROGS(prolat, sst) # prolat is part of SST
AC_CONFIG_HEADERS(config.h)
-AC_CONFIG_FILES(Makefile component.xml ast_link object.h f77.h)
+AC_CONFIG_FILES(Makefile component.xml ast_link ast_link_adam object.h f77.h)
AC_CONFIG_FILES([ast_cpp], [chmod +x ast_cpp])
# Following are files which are substituted by the Makefile at
# distribution time, rather than by configure. They are not distributed.
diff --git a/ellipse.c b/ellipse.c
index ae09d11..ee8de30 100644
--- a/ellipse.c
+++ b/ellipse.c
@@ -342,7 +342,7 @@ AstRegion *astBestEllipse_( AstPointSet *mesh, double *cen, AstRegion *unc, int
for( ip = maxat + 1; ip < np; ip++ ) {
if( dist[ ip ] != AST__BAD ) {
r3 = dist[ ip ];
- t3 = palSlaDrange( ang[ ip ] - a0 );
+ t3 = palDrange( ang[ ip ] - a0 );
break;
}
}
@@ -350,7 +350,7 @@ AstRegion *astBestEllipse_( AstPointSet *mesh, double *cen, AstRegion *unc, int
for( ip = 0; ip < maxat; ip++ ) {
if( dist[ ip ] != AST__BAD ) {
r3 = dist[ ip ];
- t3 = palSlaDrange( ang[ ip ] - a0 );
+ t3 = palDrange( ang[ ip ] - a0 );
break;
}
}
@@ -364,7 +364,7 @@ AstRegion *astBestEllipse_( AstPointSet *mesh, double *cen, AstRegion *unc, int
for( ip = maxat - 1; ip > -1; ip-- ) {
if( dist[ ip ] != AST__BAD ) {
r1 = dist[ ip ];
- t1 = palSlaDrange( ang[ ip ] - a0 );
+ t1 = palDrange( ang[ ip ] - a0 );
break;
}
}
@@ -372,7 +372,7 @@ AstRegion *astBestEllipse_( AstPointSet *mesh, double *cen, AstRegion *unc, int
for( ip = np - 1; ip > maxat; ip-- ) {
if( dist[ ip ] != AST__BAD ) {
r1 = dist[ ip ];
- t1 = palSlaDrange( ang[ ip ] - a0 );
+ t1 = palDrange( ang[ ip ] - a0 );
break;
}
}
diff --git a/fitschan.c b/fitschan.c
index edd9191..b4d6751 100644
--- a/fitschan.c
+++ b/fitschan.c
@@ -1006,6 +1006,28 @@ f - AST_WRITEFITS: Write all cards out to the sink function
* TAN projection).
* 22-NOV-2011 (DSB):
* Allow the "-SIP" code to be used with non-celestial axes.
+* 1-FEB-2012 (DSB):
+* Write out MJD-OBS in the timescale specified by any TIMESYS
+* keyword in the FitsChan, and ensure the TIMESYS value is included
+* in the output header.
+* 23-FEB-2012 (DSB):
+* Use iauGd2gc in place of palGeoc where is saves some calculations.
+* 24-FEB-2012 (DSB):
+* Move invocation of AddEncodingFrame from Write to end of
+* MakeFitsFrameSet. This is so that AddEncodingFrame can take
+* advantage of any standardisations (such as adding celestial axes)
+* performed by MakeFItsFrameSet. Without this, a FRameSet contain
+* a 1D SpecFrame (no celestial axes) would fail to be exported using
+* FITS-CLASS encoding.
+* 29-FEB-2012 (DSB):
+* Fix bug in CLASSFromStore that caused spatial axes added by
+* MakeFitsFrameSet to be ignored.
+* 2-MAR-2012 (DSB):
+* - In CLASSFromSTore, ensure NAXIS2/3 values are stored in teh FitsChan,
+* and cater for FrameSets that have only a apectral axis and no celestial
+* axes (this prevented the VELO_LSR keyword being created)..
+* 7-MAR-2012 (DSB):
+* Use iauGc2gd in place of Geod.
*class--
*/
@@ -1193,6 +1215,7 @@ f - AST_WRITEFITS: Write all cards out to the sink function
#include "timeframe.h"
#include "keymap.h"
#include "pal.h"
+#include "sofa.h"
#include "slamap.h"
#include "specframe.h"
#include "dsbspecframe.h"
@@ -1252,6 +1275,7 @@ typedef struct FitsStore {
char ****specsys;
char ****ssyssrc;
char ****ps;
+ char ****timesys;
double ***pc;
double ***cdelt;
double ***crpix;
@@ -1278,7 +1302,6 @@ typedef struct FitsStore {
double ***imagfreq;
double ***axref;
int naxis;
- AstTimeScaleType timesys;
AstKeyMap *tables;
} FitsStore;
@@ -1543,7 +1566,7 @@ static int TestWarnings( AstFitsChan *, int * );
static void SetWarnings( AstFitsChan *, const char *, int * );
static AstFitsChan *SpecTrans( AstFitsChan *, int, const char *, const char *, int * );
static AstFitsTable *GetNamedTable( AstFitsChan *, const char *, int, int, int, const char *, int * );
-static AstFrameSet *MakeFitsFrameSet( AstFrameSet *, int, int, int * );
+static AstFrameSet *MakeFitsFrameSet( AstFitsChan *, AstFrameSet *, int, int, int, const char *, const char *, int * );
static AstGrismMap *ExtractGrismMap( AstMapping *, int, AstMapping **, int * );
static AstKeyMap *GetTables( AstFitsChan *, int * );
static AstMapping *AddUnitMaps( AstMapping *, int, int, int * );
@@ -1578,7 +1601,7 @@ static AstWinMap *WcsShift( FitsStore *, char, int, const char *, const char *,
static FitsCard *GetLink( FitsCard *, int, const char *, const char *, int * );
static FitsStore *FitsToStore( AstFitsChan *, int, const char *, const char *, int * );
static FitsStore *FreeStore( FitsStore *, int * );
-static FitsStore *FsetToStore( AstFitsChan *, AstFrameSet *, int, double *, const char *, const char *, int * );
+static FitsStore *FsetToStore( AstFitsChan *, AstFrameSet *, int, double *, int, const char *, const char *, int * );
static char *CardComm( AstFitsChan *, int * );
static char *CardName( AstFitsChan *, int * );
static double *Cheb2Poly( double *, int, int, double, double, double, double, int * );
@@ -1596,7 +1619,7 @@ static double **OrthVectorSet( int, int, double **, int * );
static double *FitLine( AstMapping *, double *, double *, double *, double, double *, int * );
static double *OrthVector( int, int, double **, int * );
static double *ReadCrval( AstFitsChan *, AstFrame *, char, const char *, const char *, int * );
-static double ChooseEpoch( FitsStore *, char, const char *, const char *, int * );
+static double ChooseEpoch( AstFitsChan *, FitsStore *, char, const char *, const char *, int * );
static double DateObs( const char *, int * );
static double GetItem( double ****, int, int, char, char *, const char *method, const char *class, int * );
static double NearestPix( AstMapping *, double, int, int * );
@@ -1605,7 +1628,7 @@ static int *CardFlags( AstFitsChan *, int * );
static int AIPSFromStore( AstFitsChan *, FitsStore *, const char *, const char *, int * );
static int AIPSPPFromStore( AstFitsChan *, FitsStore *, const char *, const char *, int * );
static int AddEncodingFrame( AstFitsChan *, AstFrameSet *, int, const char *, const char *, int * );
-static int AddVersion( AstFitsChan *, AstFrameSet *, int, int, FitsStore *, double *, char, const char *, const char *, int * );
+static int AddVersion( AstFitsChan *, AstFrameSet *, int, int, FitsStore *, double *, char, int, const char *, const char *, int * );
static int CLASSFromStore( AstFitsChan *, FitsStore *, AstFrameSet *, double *, const char *, const char *, int * );
static int CardType( AstFitsChan *, int * );
static int CheckFitsName( const char *, const char *, const char *, int * );
@@ -1665,7 +1688,7 @@ static int PCFromStore( AstFitsChan *, FitsStore *, const char *, const char *,
static int SearchCard( AstFitsChan *, const char *, const char *, const char *, int * );
static int SetFits( AstFitsChan *, const char *, void *, int, const char *, int, int * );
static int Similar( const char *, const char *, int * );
-static int SkySys( AstSkyFrame *, int, int, FitsStore *, int, int, char c, const char *, const char *, int * );
+static int SkySys( AstFitsChan *, AstSkyFrame *, int, int, FitsStore *, int, int, char c, const char *, const char *, int * );
static int Split( const char *, char **, char **, char **, const char *, const char *, int * );
static int SplitMap( AstMapping *, int, int, int, AstMapping **, AstWcsMap **, AstMapping **, int * );
static int SplitMap2( AstMapping *, int, AstMapping **, AstWcsMap **, AstMapping **, int * );
@@ -1705,7 +1728,6 @@ static void FixUsed( AstFitsChan *, int, int, int, const char *, const char *, i
static void FormatCard( AstFitsChan *, char *, const char *, int * );
static void FreeItem( double ****, int * );
static void FreeItemC( char *****, int * );
-static void Geod( double[3], double *, double *, double *, int * );
static void GetFiducialNSC( AstWcsMap *, double *, double *, int * );
static void GetFiducialPPC( AstWcsMap *, double *, double *, int * );
static void GetNextData( AstChannel *, int, char **, char **, int * );
@@ -1972,7 +1994,6 @@ static int AddEncodingFrame( AstFitsChan *this, AstFrameSet *fs, int encoding,
* Private function.
* Synopsis:
-
* int AddEncodingFrame( AstFitsChan *this, AstFrameSet *fs, int encoding,
* const char *method, const char *class, int *status )
@@ -2237,7 +2258,7 @@ static void AddFrame( AstFitsChan *this, AstFrameSet *fset, int pixel,
}
static int AddVersion( AstFitsChan *this, AstFrameSet *fs, int ipix, int iwcs,
- FitsStore *store, double *dim, char s,
+ FitsStore *store, double *dim, char s, int encoding,
const char *method, const char *class, int *status ){
/*
@@ -2252,9 +2273,8 @@ static int AddVersion( AstFitsChan *this, AstFrameSet *fs, int ipix, int iwcs,
* Synopsis:
* #include "fitschan.h"
-
* int AddVersion( AstFitsChan *this, AstFrameSet *fs, int ipix, int iwcs,
-* FitsStore *store, double *dim, char s,
+* FitsStore *store, double *dim, char s, int encoding,
* const char *method, const char *class, int *status )
* Class Membership:
@@ -2287,6 +2307,8 @@ static int AddVersion( AstFitsChan *this, AstFrameSet *fs, int ipix, int iwcs,
* The co-ordinate version character. A space means the primary
* axis descriptions. Otherwise the supplied character should be
* an upper case alphabetical character ('A' to 'Z').
+* encoding
+* The encoding being used.
* method
* Pointer to a string holding the name of the calling method.
* This is only for use in constructing error messages.
@@ -2371,7 +2393,7 @@ static int AddVersion( AstFitsChan *this, AstFrameSet *fs, int ipix, int iwcs,
position (SpecFrame attributes RefRA and RefDec), then FITS-WCS paper
III requires there to be a pair of celestial axes in the WCS Frame in
which the celestial reference point for the spectral axis is defined. */
- fset = MakeFitsFrameSet( fs, ipix, iwcs, status );
+ fset = MakeFitsFrameSet( this, fs, ipix, iwcs, encoding, method, class, status );
/* Abort if the FrameSet could not be produced. */
if( !fset ) return ret;
@@ -2993,8 +3015,8 @@ static int AIPSFromStore( AstFitsChan *this, FitsStore *store,
} else {
rho_b = atan2( -cdlon_lat, cdelt[ axrot2 ] );
}
- if( fabs( palSlaDrange( rho_a - rho_b ) ) < 1.0E-2 ){
- crota = 0.5*( palSlaDranrm( rho_a ) + palSlaDranrm( rho_b ) );
+ if( fabs( palDrange( rho_a - rho_b ) ) < 1.0E-2 ){
+ crota = 0.5*( palDranrm( rho_a ) + palDranrm( rho_b ) );
coscro = cos( crota );
sincro = sin( crota );
if( fabs( coscro ) > fabs( sincro ) ){
@@ -3140,14 +3162,14 @@ static int AIPSFromStore( AstFitsChan *this, FitsStore *store,
/* The format used for the DATE-OBS keyword depends on the value of the
keyword. For DATE-OBS < 1999.0, use the old "dd/mm/yy" format.
Otherwise, use the new "ccyy-mm-ddThh:mm:ss[.ssss]" format. */
- palSlaCaldj( 99, 1, 1, &mjd99, &jj );
+ palCaldj( 99, 1, 1, &mjd99, &jj );
if( val < mjd99 ) {
- palSlaDjcal( 0, val, iymdf, &jj );
+ palDjcal( 0, val, iymdf, &jj );
sprintf( combuf, "%2.2d/%2.2d/%2.2d", iymdf[ 2 ], iymdf[ 1 ],
iymdf[ 0 ] - ( ( iymdf[ 0 ] > 1999 ) ? 2000 : 1900 ) );
} else {
- palSlaDjcl( val, iymdf, iymdf+1, iymdf+2, &fd, &jj );
- palSlaDd2tf( 3, fd, sign, ihmsf );
+ palDjcl( val, iymdf, iymdf+1, iymdf+2, &fd, &jj );
+ palDd2tf( 3, fd, sign, ihmsf );
sprintf( combuf, "%4.4d-%2.2d-%2.2dT%2.2d:%2.2d:%2.2d.%3.3d",
iymdf[0], iymdf[1], iymdf[2], ihmsf[0], ihmsf[1],
ihmsf[2], ihmsf[3] );
@@ -3495,8 +3517,8 @@ static int AIPSPPFromStore( AstFitsChan *this, FitsStore *store,
} else {
rho_b = atan2( -cdlon_lat, cdelt[ axrot2 ] );
}
- if( fabs( palSlaDrange( rho_a - rho_b ) ) < 1.0E-2 ){
- crota = 0.5*( palSlaDranrm( rho_a ) + palSlaDranrm( rho_b ) );
+ if( fabs( palDrange( rho_a - rho_b ) ) < 1.0E-2 ){
+ crota = 0.5*( palDranrm( rho_a ) + palDranrm( rho_b ) );
coscro = cos( crota );
sincro = sin( crota );
if( fabs( coscro ) > fabs( sincro ) ){
@@ -3673,14 +3695,14 @@ static int AIPSPPFromStore( AstFitsChan *this, FitsStore *store,
/* The format used for the DATE-OBS keyword depends on the value of the
keyword. For DATE-OBS < 1999.0, use the old "dd/mm/yy" format.
Otherwise, use the new "ccyy-mm-ddThh:mm:ss[.ssss]" format. */
- palSlaCaldj( 99, 1, 1, &mjd99, &jj );
+ palCaldj( 99, 1, 1, &mjd99, &jj );
if( val < mjd99 ) {
- palSlaDjcal( 0, val, iymdf, &jj );
+ palDjcal( 0, val, iymdf, &jj );
sprintf( combuf, "%2.2d/%2.2d/%2.2d", iymdf[ 2 ], iymdf[ 1 ],
iymdf[ 0 ] - ( ( iymdf[ 0 ] > 1999 ) ? 2000 : 1900 ) );
} else {
- palSlaDjcl( val, iymdf, iymdf+1, iymdf+2, &fd, &jj );
- palSlaDd2tf( 3, fd, sign, ihmsf );
+ palDjcl( val, iymdf, iymdf+1, iymdf+2, &fd, &jj );
+ palDd2tf( 3, fd, sign, ihmsf );
sprintf( combuf, "%4.4d-%2.2d-%2.2dT%2.2d:%2.2d:%2.2d.%3.3d",
iymdf[0], iymdf[1], iymdf[2], ihmsf[0], ihmsf[1],
ihmsf[2], ihmsf[3] );
@@ -4153,6 +4175,10 @@ static AstMapping *CelestialAxes( AstFitsChan *this, AstFrameSet *fs, double *di
/* Initialise */
ret = NULL;
+/* Other initialisation to avoid compiler warnings. */
+ mlon = 0;
+ mlat = 0;
+
/* Check the inherited status. */
if( !astOK ) return ret;
@@ -4293,7 +4319,7 @@ static AstMapping *CelestialAxes( AstFitsChan *this, AstFrameSet *fs, double *di
}
/* Store the CTYPE, CNAME, EQUINOX, MJDOBS, and RADESYS values. */
- SkySys( skyfrm, 1, astGetWcsType( map2 ), store, fits_ilon,
+ SkySys( this, skyfrm, 1, astGetWcsType( map2 ), store, fits_ilon,
fits_ilat, s, method, class, status );
/* Store the LONPOLE and LATPOLE values in the FitsStore. */
@@ -4520,7 +4546,7 @@ static AstMapping *CelestialAxes( AstFitsChan *this, AstFrameSet *fs, double *di
if( tmap0 ) {
/* Store the CTYPE, CNAME, EQUINOX, MJDOBS, and RADESYS values. */
- SkySys( skyfrm, 0, 0, store, fits_ilon, fits_ilat, s, method,
+ SkySys( this, skyfrm, 0, 0, store, fits_ilon, fits_ilat, s, method,
class, status );
/* If possible, choose the two CRVAL values (which are values on the psi
@@ -5155,8 +5181,8 @@ static void CheckZero( char *text, double value, int width, int *status ){
}
}
-static double ChooseEpoch( FitsStore *store, char s, const char *method,
- const char *class, int *status ){
+static double ChooseEpoch( AstFitsChan *this, FitsStore *store, char s,
+ const char *method, const char *class, int *status ){
/*
* Name:
* ChooseEpoch
@@ -5168,8 +5194,8 @@ static double ChooseEpoch( FitsStore *store, char s, const char *method,
* Private function.
* Synopsis:
-* double ChooseEpoch( FitsStore *store, char s, const char *method,
-* const char *class, int *status )
+* double ChooseEpoch( AstFitsChan *this, FitsStore *store, char s,
+* const char *method, const char *class, int *status )
* Class Membership:
* FitsChan
@@ -5182,6 +5208,8 @@ static double ChooseEpoch( FitsStore *store, char s, const char *method,
* keywords by the SpecTrans function before this function is called.
* Parameters:
+* this
+* Pointer to the FitsChan.
* store
* A structure containing values for FITS keywords relating to
* the World Coordinate System.
@@ -5205,7 +5233,8 @@ static double ChooseEpoch( FitsStore *store, char s, const char *method,
*/
/* Local Variables: */
- double mjd; /* The returned MJD */
+ const char *timesys; /* The TIMESYS value in the FitsStore */
+ double mjd; /* The returned MJD */
/* Initialise the returned value. */
mjd = AST__BAD;
@@ -5230,7 +5259,9 @@ static double ChooseEpoch( FitsStore *store, char s, const char *method,
method, class, status );
/* Now convert the MJD value to the TDB timescale. */
- mjd = TDBConv( mjd, store->timesys, 0, method, class, status );
+ timesys = GetItemC( &(store->timesys), 0, 0, ' ', NULL, method, class, status );
+ mjd = TDBConv( mjd, TimeSysToAst( this, timesys, method, class, status ),
+ 0, method, class, status );
/* Return the answer. */
return mjd;
@@ -5523,6 +5554,10 @@ static int CLASSFromStore( AstFitsChan *this, FitsStore *store,
int ok; /* Is FitsSTore OK for IRAF encoding? */
int prj; /* Projection type */
+/* Other initialisation to avoid compiler warnings. */
+ lonval = 0.0;
+ latval = 0.0;
+
/* Check the inherited status. */
if( !astOK ) return 0;
@@ -5552,7 +5587,7 @@ static int CLASSFromStore( AstFitsChan *this, FitsStore *store,
/* If the spatial pixel axes are degenerate (i.e. span only a single
pixel), modify the CRPIX and CRVAL values in the FitsStore to put
the reference point at the centre of the one and only spatial pixel. */
- if( dim[ axlon ] == 1.0 && dim[ axlat ] == 1.0 ){
+ if( store->naxis >= 3 && dim[ axlon ] == 1.0 && dim[ axlat ] == 1.0 ){
xin[ 0 ] = 1.0;
xin[ 1 ] = 1.0;
xin[ 2 ] = 1.0;
@@ -5698,9 +5733,10 @@ static int CLASSFromStore( AstFitsChan *this, FitsStore *store,
/* Save the number of WCS axes */
naxis = GetMaxJM( &(store->crpix), ' ', status ) + 1;
-/* If this is larger than the number of pixel axes, ignore the surplus
- WCS axes. */
- if( naxis > store->naxis ) naxis = store->naxis;
+/* If this is larger than 3, ignore the surplus WCS axes. Note, the
+ above code has checked that the spatial and spectral axes are
+ WCS axes 0, 1 and 2. */
+ if( naxis > 3 ) naxis = 3;
/* Allocate memory to store the CDELT values */
if( ok ) {
@@ -5790,6 +5826,26 @@ static int CLASSFromStore( AstFitsChan *this, FitsStore *store,
of the FITS-CLASS encoding. */
if( ok ) {
+/* If celestial axes were added by MakeFitsFrameSet, we need to ensure
+ the header contains 3 main array axes. This is because the CLASS
+ encoding does not support the WCSAXES keyword. */
+ if( store->naxis == 1 ) {
+
+/* Update the "NAXIS" value to 3 or put a new card in at the start. */
+ astClearCard( this );
+ i = 3;
+ SetValue( this, "NAXIS", &i, AST__INT, NULL, status );
+
+/* Put NAXIS2/3 after NAXIS1, or after NAXIS if the FitsChan does not contain
+ NAXIS1. These are set to 1 since the spatial axes are degenerate. */
+ if( FindKeyCard( this, "NAXIS1", method, class, status ) ) {
+ MoveCard( this, 1, method, class, status );
+ }
+ i = 1;
+ SetValue( this, "NAXIS2", &i, AST__INT, NULL, status );
+ SetValue( this, "NAXIS3", &i, AST__INT, NULL, status );
+ }
+
/* Find the last WCS related card. */
FindWcs( this, 1, 1, 0, method, class, status );
@@ -5869,14 +5925,14 @@ static int CLASSFromStore( AstFitsChan *this, FitsStore *store,
/* The format used for the DATE-OBS keyword depends on the value of the
keyword. For DATE-OBS < 1999.0, use the old "dd/mm/yy" format.
Otherwise, use the new "ccyy-mm-ddThh:mm:ss[.ssss]" format. */
- palSlaCaldj( 99, 1, 1, &mjd99, &jj );
+ palCaldj( 99, 1, 1, &mjd99, &jj );
if( val < mjd99 ) {
- palSlaDjcal( 0, val, iymdf, &jj );
+ palDjcal( 0, val, iymdf, &jj );
sprintf( combuf, "%2.2d/%2.2d/%2.2d", iymdf[ 2 ], iymdf[ 1 ],
iymdf[ 0 ] - ( ( iymdf[ 0 ] > 1999 ) ? 2000 : 1900 ) );
} else {
- palSlaDjcl( val, iymdf, iymdf+1, iymdf+2, &fd, &jj );
- palSlaDd2tf( 3, fd, sign, ihmsf );
+ palDjcl( val, iymdf, iymdf+1, iymdf+2, &fd, &jj );
+ palDd2tf( 3, fd, sign, ihmsf );
sprintf( combuf, "%4.4d-%2.2d-%2.2dT%2.2d:%2.2d:%2.2d.%3.3d",
iymdf[0], iymdf[1], iymdf[2], ihmsf[0], ihmsf[1],
ihmsf[2], ihmsf[3] );
@@ -5915,10 +5971,10 @@ static int CLASSFromStore( AstFitsChan *this, FitsStore *store,
to get the value for VELO-LSR. Create a SpecFrame describing the
required frame (other attributes such as Epoch etc are left unset and
so will be picked up from the supplied FrameSet). We set MinAxes
- and MaxAxes so that the Frame can be used as a template to match the 3D
- current Frame in the supplied FrameSet. */
+ and MaxAxes so that the Frame can be used as a template to match the
+ 1D or 3D current Frame in the supplied FrameSet. */
velofrm = (AstFrame *) astSpecFrame( "System=vrad,StdOfRest=lsrk,"
- "Unit=m/s,MinAxes=3,MaxAxes=3", status );
+ "Unit=m/s,MinAxes=1,MaxAxes=3", status );
/* Find the spectral axis within the current Frame of the supplied
FrameSet, using the above "velofrm" as a template. */
@@ -7444,7 +7500,7 @@ static double DateObs( const char *dateobs, int *status ) {
if( ok ) {
/* Get the MJD at the start of the day. */
- palSlaCaldj( yy, mm, dd, &ret, &j );
+ palCaldj( yy, mm, dd, &ret, &j );
/* If succesful, convert the hours, minutes and seconds to a fraction of
a day, and add it onto the MJD found above. */
@@ -7463,7 +7519,7 @@ static double DateObs( const char *dateobs, int *status ) {
secs += (double) sc;
/*Convert the hours, minutes and seconds to a fractional day. */
- palSlaDtf2d( hr, mn, secs, &days, &j );
+ palDtf2d( hr, mn, secs, &days, &j );
/* If succesful, add this onto the returned MJD. */
if( j == 0 ) {
@@ -9778,6 +9834,7 @@ static void FindWcs( AstFitsChan *this, int last, int all, int rewind,
Match( keyname, "EQUINOX%0c", 0, NULL, &nfld, method, class, status ) ||
Match( keyname, "MJD-OBS", 0, NULL, &nfld, method, class, status ) ||
Match( keyname, "DATE-OBS", 0, NULL, &nfld, method, class, status ) ||
+ Match( keyname, "TIMESYS", 0, NULL, &nfld, method, class, status ) ||
Match( keyname, "RADECSYS", 0, NULL, &nfld, method, class, status ) ||
Match( keyname, "RADESYS%0c", 0, NULL, &nfld, method, class, status ) ||
Match( keyname, "C%1dVAL%d", 0, NULL, &nfld, method, class, status ) ||
@@ -10218,7 +10275,7 @@ static FitsStore *FitsToStore( AstFitsChan *this, int encoding,
ret->imagfreq = NULL;
ret->axref = NULL;
ret->naxis = 0;
- ret->timesys = AST__UTC;
+ ret->timesys = NULL;
ret->tables = astKeyMap( "", status );
}
@@ -10302,6 +10359,9 @@ static void FreeItem( double ****item, int *status ){
int oldstatus; /* Old error status value */
int oldreport; /* Old error reporting value */
+/* Other initialisation to avoid compiler warnings. */
+ oldreport = 0;
+
/* Check the supplied pointer */
if( item && *item ){
@@ -10394,6 +10454,9 @@ static void FreeItemC( char *****item, int *status ){
int oldstatus; /* Old error status value */
int oldreport; /* Old error reporting value */
+/* Other initialisation to avoid compiler warnings. */
+ oldreport = 0;
+
/* Check the supplied pointer */
if( item && *item ){
@@ -10493,6 +10556,7 @@ static FitsStore *FreeStore( FitsStore *store, int *status ){
FreeItemC( &(store->specsys), status );
FreeItemC( &(store->ssyssrc), status );
FreeItemC( &(store->ps), status );
+ FreeItemC( &(store->timesys), status );
FreeItem( &(store->pc), status );
FreeItem( &(store->cdelt), status );
FreeItem( &(store->crpix), status );
@@ -10781,7 +10845,7 @@ static AstObject *FsetFromStore( AstFitsChan *this, FitsStore *store,
}
static FitsStore *FsetToStore( AstFitsChan *this, AstFrameSet *fset, int naxis,
- double *dim, const char *class,
+ double *dim, int encoding, const char *class,
const char *method, int *status ){
/*
@@ -10798,7 +10862,7 @@ static FitsStore *FsetToStore( AstFitsChan *this, AstFrameSet *fset, int naxis,
* Synopsis:
* FitsStore *FsetToStore( AstFitsChan *this, AstFrameSet *fset, int naxis,
-* double *dim, const char *class,
+* double *dim, int encoding, const char *class,
* const char *method, int *status )
* Class Membership:
@@ -10827,6 +10891,8 @@ static FitsStore *FsetToStore( AstFitsChan *this, AstFrameSet *fset, int naxis,
* dim
* Pointer to an array of pixel axis dimensions. Individual elements
* will be AST__BAD if dimensions are not known.
+* encoding
+* The encoding being used.
* method
* Pointer to a string holding the name of the calling method.
* This is only for use in constructing error messages.
@@ -10909,7 +10975,7 @@ static FitsStore *FsetToStore( AstFitsChan *this, AstFrameSet *fset, int naxis,
ret->imagfreq = NULL;
ret->axref = NULL;
ret->naxis = naxis;
- ret->timesys = AST__UTC;
+ ret->timesys = NULL;
ret->tables = astKeyMap( "", status );
/* Obtain the index of the Base Frame (i.e. the pixel frame ). */
@@ -10921,8 +10987,8 @@ static FitsStore *FsetToStore( AstFitsChan *this, AstFrameSet *fset, int naxis,
/* Add a description of the primary axes to the FitsStore, based on the
Current Frame in the FrameSet. */
- primok = AddVersion( this, fset, ibase, icurr, ret, dim, ' ', method,
- class, status );
+ primok = AddVersion( this, fset, ibase, icurr, ret, dim, ' ',
+ encoding, method, class, status );
/* Do not add any alternate axis descriptions if the primary axis
descriptions could not be produced. */
@@ -10991,7 +11057,7 @@ static FitsStore *FsetToStore( AstFitsChan *this, AstFrameSet *fset, int naxis,
s = sid[ ifrm ];
if( s != 0 && s != 1 ) {
secok = AddVersion( this, fset, ibase, ifrm, ret, dim,
- s, method, class, status );
+ s, encoding, method, class, status );
}
}
@@ -11008,117 +11074,6 @@ static FitsStore *FsetToStore( AstFitsChan *this, AstFrameSet *fset, int naxis,
return ret;
}
-static void Geod( double pos[3], double *phi, double *h, double *lambda, int *status ){
-/*
-* Name:
-* Geod
-
-* Purpose:
-* Convert a terrestrial Cartesian (x,y,z) position to geodetic lat/long
-
-* Type:
-* Private function.
-
-* Synopsis:
-* #include "fitschan.h"
-* void Geod( double pos[3], double *phi, double *h, double *lambda, int *status )
-
-* Class Membership:
-* FitsChan member function.
-
-* Description:
-* This function converts a position supplied as terrestrial Cartesian
-* (x,y,z) values into geodetic longitude, latitude and height above the
-* reference spheroid. The (x,y,z) system has origin at the centre of
-* the earth, Z axis going through the north pole, X axis at
-* (long,lat)=(0,0), and Y axis at (long,lat) = (E90,0).
-*
-* The algorithm is due to Borkowski, and is described in the
-* Explanatory Supplement to the Astronomical Almanac (p206).
-
-* Parameters:
-* pos
-* Array holding the (x,y,z) values, in metres.
-* phi
-* Pointer at a location at which to return the geodetic latitude,
-* in radians.
-* h
-* Pointer at a location at which to return the height above the
-* reference spheroid (geodetic, metres).
-* lambda
-* Pointer at a location at which to return the geodetic longitude,
-* in radians, positive east.
-* status
-* Pointer to the inherited status variable.
-*/
-
-/* Local Variables... */
- double r, e, f, p, q, d, n, g, t, rp, rd, sn, b0, boa, ab2oa;
-
-/* Initialise */
- *phi = 0.0;
- *h = 0.0;
- *lambda = 0.0;
-
-/* Check the global status. */
- if( !astOK ) return;
-
-/* Earth polar radius (metres) */
- b0 = A0*( 1.0 - FL );
-
-/* Useful functions */
- boa = b0/A0;
- ab2oa = ( A0*A0 - b0*b0)/A0;
-
-/* To obtain the proper sign and polynomial solution, the sign of b is
- set to that of z. Note the sign of z. */
- if( pos[ 2 ] > 0.0 ) {
- sn = 1.0;
- } else {
- sn = -1.0;
- }
-
-/* If the supplied position is on the polar axis, the returned values are
- trivial. We check this case because it corresponds to a singularity in
- the main algorithm. */
- r = sqrt( pos[ 0 ]*pos[ 0 ] + pos[ 1 ]*pos[ 1 ] );
- if( r == 0 ) {
- *lambda = 0.0;
- *phi = AST__DPIBY2;
- *h = pos[ 2 ] - sn*b0;
- } else {
-
-/* The longitude is simple. */
- *lambda = atan2( pos[ 1 ], pos[ 0 ] );
-
-/* The equator is also a singularity in the main algorithm. If the
- supplied point is on the equator, the answers are trivial. */
- if( pos[ 2 ] == 0.0 ) {
- *phi = 0.0;
- *h = r - A0;
-
-/* For all other cases, use the main Borkowski algorithm. */
- } else {
- e = ( sn*boa*pos[ 2 ] - ab2oa )/r;
- f = ( sn*boa*pos[ 2 ] + ab2oa )/r;
- p = 4.0*( e*f + 1.0 )/3.0;
- q = 2.0*( e*e - f*f );
- d = p*p*p + q*q;
- if( d < 0.0 ) {
- rp = sqrt( -p );
- n = 2.0*rp*cos( acos( q/(p*rp) )/3.0 );
- } else {
- rd = sqrt( d );
- n = pow( ( rd - q ), 1.0/3.0 ) - pow( (rd + q ), 1.0/3.0 );
- }
- g = 0.5* ( sqrt( e*e + n ) + e );
- t = sqrt( g*g + ( f - n*g )/( 2*g - e ) ) - g;
- *phi = atan( A0*( 1.0 - t*t )/( 2.0*sn*b0*t ) );
- *h = ( r - A0*t )*cos( *phi ) + ( pos[ 2 ] - sn*b0 )*sin( *phi );
- }
- }
-}
-
static int GetClean( AstFitsChan *this, int *status ) {
/*
@@ -15125,7 +15080,6 @@ static void FixUsed( AstFitsChan *this, int reset, int used, int remove,
* Synopsis:
* #include "fitschan.h"
-
* void FixUsed( AstFitsChan *this, int reset, int used, int remove,
* const char *method, const char *class, int *status )
@@ -16672,7 +16626,6 @@ static int GetSkip( AstChannel *this_channel, int *status ) {
static int GetValue( AstFitsChan *this, const char *keyname, int type,
void *value, int report, int mark, const char *method,
const char *class, int *status ){
-
/*
* Name:
* GetValue
@@ -16684,7 +16637,6 @@ static int GetValue( AstFitsChan *this, const char *keyname, int type,
* Private function.
* Synopsis:
-
* int GetValue( AstFitsChan *this, const char *keyname, int type, void *value,
* int report, int mark, const char *method, const char *class, int *status )
@@ -17599,14 +17551,14 @@ static int IRAFFromStore( AstFitsChan *this, FitsStore *store,
/* The format used for the DATE-OBS keyword depends on the value of the
keyword. For DATE-OBS < 1999.0, use the old "dd/mm/yy" format.
Otherwise, use the new "ccyy-mm-ddThh:mm:ss[.ssss]" format. */
- palSlaCaldj( 99, 1, 1, &mjd99, &jj );
+ palCaldj( 99, 1, 1, &mjd99, &jj );
if( val < mjd99 ) {
- palSlaDjcal( 0, val, iymdf, &jj );
+ palDjcal( 0, val, iymdf, &jj );
sprintf( combuf, "%2.2d/%2.2d/%2.2d", iymdf[ 2 ], iymdf[ 1 ],
iymdf[ 0 ] - ( ( iymdf[ 0 ] > 1999 ) ? 2000 : 1900 ) );
} else {
- palSlaDjcl( val, iymdf, iymdf+1, iymdf+2, &fd, &jj );
- palSlaDd2tf( 3, fd, sign, ihmsf );
+ palDjcl( val, iymdf, iymdf+1, iymdf+2, &fd, &jj );
+ palDd2tf( 3, fd, sign, ihmsf );
sprintf( combuf, "%4.4d-%2.2d-%2.2dT%2.2d:%2.2d:%2.2d.%3.3d",
iymdf[0], iymdf[1], iymdf[2], ihmsf[0], ihmsf[1],
ihmsf[2], ihmsf[3] );
@@ -19375,7 +19327,10 @@ static AstMapping *MakeColumnMap( AstFitsTable *table, const char *col,
return result;
}
-static AstFrameSet *MakeFitsFrameSet( AstFrameSet *fset, int ipix, int iwcs, int *status ) {
+static AstFrameSet *MakeFitsFrameSet( AstFitsChan *this, AstFrameSet *fset,
+ int ipix, int iwcs, int encoding,
+ const char *method, const char *class,
+ int *status ) {
/*
* Name:
* MakeFitsFrameSet
@@ -19389,7 +19344,10 @@ static AstFrameSet *MakeFitsFrameSet( AstFrameSet *fset, int ipix, int iwcs, int
* Synopsis:
* #include "fitschan.h"
-* AstFrameSet *MakeFitsFrameSet( AstFrameSet *fset, int ipix, int iwcs, int *status )
+* AstFrameSet *MakeFitsFrameSet( AstFitsChan *this, AstFrameSet *fset,
+* int ipix, int iwcs, int encoding,
+* const char *method, const char *class,
+* int *status )
* Class Membership:
* FitsChan member function.
@@ -19419,12 +19377,22 @@ static AstFrameSet *MakeFitsFrameSet( AstFrameSet *fset, int ipix, int iwcs, int
* celestial axes.
* Parameters:
+* this
+* The FitsChan.
* fset
* The FrameSet to check.
* ipix
* The index of the FITS pixel Frame within "fset".
* iwcs
* The index of the WCS Frame within "fset".
+* encoding
+* The encoding in use.
+* method
+* Pointer to a string holding the name of the calling method.
+* This is only for use in constructing error messages.
+* class
+* Pointer to a string holding the name of the supplied object class.
+* This is only for use in constructing error messages.
* status
* Pointer to the inherited status variable.
@@ -19458,13 +19426,14 @@ static AstFrameSet *MakeFitsFrameSet( AstFrameSet *fset, int ipix, int iwcs, int
char card[ AST__FITSCHAN_FITSCARDLEN + 1 ]; /* A FITS header card */
char equinox_attr[ 13 ];/* Name of Equinox attribute for sky axes */
char system_attr[ 12 ]; /* Name of System attribute for sky axes */
- const char *eqn; /* Pointer to original sky Equinox value */
+ const char *eqn; /* Pointer to original sky Equinox value */
const char *skysys; /* Pointer to original sky System value */
double con; /* Constant axis value */
double reflat; /* Celestial latitude at reference point */
double reflon; /* Celestial longitude at reference point */
int *perm; /* Pointer to axis permutation array */
int iax; /* Axis inex */
+ int icurr; /* Index of original current Frame in returned FrameSet */
int ilat; /* Celestial latitude index within WCS Frame */
int ilon; /* Celestial longitude index within WCS Frame */
int ispec; /* SpecFrame axis index within WCS Frame */
@@ -19557,7 +19526,7 @@ static AstFrameSet *MakeFitsFrameSet( AstFrameSet *fset, int ipix, int iwcs, int
astAddFrame( ret, AST__BASE, map, wcsfrm );
/* If we have a celestial reference position for the spectral axis, ensure
- it is descirbed correctly by a pair of celestial axes. */
+ it is described correctly by a pair of celestial axes. */
} else {
/* If the WCS Frame does not contain any celestial axes, we add some now. */
@@ -19712,6 +19681,14 @@ static AstFrameSet *MakeFitsFrameSet( AstFrameSet *fset, int ipix, int iwcs, int
}
}
+/* Add a new current Frame into the FrameSet which increases the chances of
+ the requested encoding being usable. The index of the original current
+ Frame is returned, or AST__NOFRAME if no new Frame was added. */
+ icurr = AddEncodingFrame( this, ret, encoding, method, class, status );
+
+/* If a new Frame was added, remove the original current Frame. */
+ if( icurr != AST__NOFRAME ) astRemoveFrame( ret, icurr );
+
/* Free resources. */
if( specfrm ) specfrm = astAnnul( specfrm );
if( skyfrm ) skyfrm = astAnnul( skyfrm );
@@ -20189,7 +20166,7 @@ static int MakeIntWorld( AstMapping *cmap, AstFrame *fr, int *wperm, char s,
The "g0" array only contains "nin" values. If nout>nin, then the
missing g0 values will be assumed to be zero when we come to find the
CRPIX values below.
- We use palSlaDmat to solve this system of simultaneous equations to get
+ We use palDmat to solve this system of simultaneous equations to get
crpix. The "y" array initially holds "w0" but is over-written to hold
"g0 - crpix". */
mat = astMalloc( sizeof( double )*(size_t)( nout*nout ) );
@@ -20201,7 +20178,7 @@ static int MakeIntWorld( AstMapping *cmap, AstFrame *fr, int *wperm, char s,
for( j = 0; j < nout; j++ ) *(m++) = fullmat[ j ][ i ];
y[ i ] = w0[ i ];
}
- palSlaDmat( nout, mat, y, &det, &sing, iw );
+ palDmat( nout, mat, y, &det, &sing, iw );
}
mat = astFree( mat );
iw = astFree( iw );
@@ -20210,7 +20187,7 @@ static int MakeIntWorld( AstMapping *cmap, AstFrame *fr, int *wperm, char s,
for( j = 0; j < nout; j++ ) {
colvec = fullmat[ j ];
-/* Get the CRPIX values from the "y" vector created above by palSlaDmat.
+/* Get the CRPIX values from the "y" vector created above by palDmat.
First deal with axes for which there are Mapping inputs. */
if( j < nin ) {
crp = g0[ j ] - y[ j ];
@@ -21856,7 +21833,7 @@ static double *OrthVector( int n, int m, double **in, int *status ){
* returned vectors, but indices into an array of indices which have
* been sorted into column magnitude order. This is now a set of MxM
-* simultaneous linear equations which we can solve using palSlaDmat:
+* simultaneous linear equations which we can solve using palDmat:
*
* MAT.R = V
*
@@ -21865,7 +21842,7 @@ static double *OrthVector( int n, int m, double **in, int *status ){
* required vector (just the components which have *not* been set
* constant), and V is a constant vector equal to the column of values
* on the right hand side in the above set of simultaneous equations.
-* The palSlaDmat function solves this equation to obtain R.
+* The palDmat function solves this equation to obtain R.
* Parameters:
* n
@@ -21972,7 +21949,7 @@ static double *OrthVector( int n, int m, double **in, int *status ){
V vector (other elements hold the indices of the columns which are
being ignored because they will be mutiplied by a value of zero - the
assumed value of the corresponding components of the returned vector). We
- now copy the these values into arrays which can be passed to palSlaDmat.
+ now copy the these values into arrays which can be passed to palDmat.
First, initialise a pointer used to step through the mat array. */
mel = mat;
@@ -21982,16 +21959,16 @@ static double *OrthVector( int n, int m, double **in, int *status ){
d = in[ i ];
/* Copy the required M elements of this supplied vector into the work array
- which will be passed to palSlaDmat. */
+ which will be passed to palDmat. */
for( j = 0; j < m; j++ ) *(mel++) = d[ colperm[ j ] ];
/* Put the next right-hand side value into the "rhs" array. */
rhs[ i ] = -d[ colperm[ m ] ];
}
-/* Use palSlaDmat to find the first M elements of the returned array. These
+/* Use palDmat to find the first M elements of the returned array. These
are stored in "rhs", over-writing the original right-hand side values. */
- palSlaDmat( m, mat, rhs, &det, &sing, iw );
+ palDmat( m, mat, rhs, &det, &sing, iw );
/* If the supplied vectors span fewer than M axes, the above call will fail.
In this case, annul the returned vector. */
@@ -22920,14 +22897,14 @@ static int PCFromStore( AstFitsChan *this, FitsStore *store,
/* The format used for the DATE-OBS keyword depends on the value of the
keyword. For DATE-OBS < 1999.0, use the old "dd/mm/yy" format.
Otherwise, use the new "ccyy-mm-ddThh:mm:ss[.ssss]" format. */
- palSlaCaldj( 99, 1, 1, &mjd99, &jj );
+ palCaldj( 99, 1, 1, &mjd99, &jj );
if( val < mjd99 ) {
- palSlaDjcal( 0, val, iymdf, &jj );
+ palDjcal( 0, val, iymdf, &jj );
sprintf( combuf, "%2.2d/%2.2d/%2.2d", iymdf[ 2 ], iymdf[ 1 ],
iymdf[ 0 ] - ( ( iymdf[ 0 ] > 1999 ) ? 2000 : 1900 ) );
} else {
- palSlaDjcl( val, iymdf, iymdf+1, iymdf+2, &fd, &jj );
- palSlaDd2tf( 3, fd, sign, ihmsf );
+ palDjcl( val, iymdf, iymdf+1, iymdf+2, &fd, &jj );
+ palDd2tf( 3, fd, sign, ihmsf );
sprintf( combuf, "%4.4d-%2.2d-%2.2dT%2.2d:%2.2d:%2.2d.%3.3d",
iymdf[0], iymdf[1], iymdf[2], ihmsf[0], ihmsf[1],
ihmsf[2], ihmsf[3] );
@@ -25541,7 +25518,6 @@ static void SetValue( AstFitsChan *this, const char *keyname, void *value,
* Synopsis:
* #include "fitschan.h"
-
* void SetValue( AstFitsChan *this, char *keyname, void *value,
* int type, const char *comment, int *status )
@@ -26388,7 +26364,7 @@ static void SkyPole( AstWcsMap *map2, AstMapping *map3, int ilon, int ilat,
takes the default value, replace it with AST__BAD to prevent an explicit
keyword being stored in the FitsChan. */
GetFiducialNSC( map2, &phi0, &theta0, status );
- lonpole = palSlaDranrm( ptr1[ axlon ][ 0 ] );
+ lonpole = palDranrm( ptr1[ axlon ][ 0 ] );
if( delta0 >= theta0 ){
deflonpole = 0.0;
} else {
@@ -26420,8 +26396,8 @@ static void SkyPole( AstWcsMap *map2, AstMapping *map3, int ilon, int ilat,
}
}
-static int SkySys( AstSkyFrame *skyfrm, int wcstype, int wcsproj,
- FitsStore *store, int axlon, int axlat, char s,
+static int SkySys( AstFitsChan *this, AstSkyFrame *skyfrm, int wcstype,
+ int wcsproj, FitsStore *store, int axlon, int axlat, char s,
const char *method, const char *class, int *status ){
/*
* Name:
@@ -26435,8 +26411,8 @@ static int SkySys( AstSkyFrame *skyfrm, int wcstype, int wcsproj,
* Synopsis:
* #include "fitschan.h"
-* int SkySys( AstSkyFrame *skyfrm, int wcstype, int wcsproj,
-* FitsStore *store, int axlon, int axlat, char s,
+* int SkySys( AstFitsChan *this, AstSkyFrame *skyfrm, int wcstype,
+* int wcsproj, FitsStore *store, int axlon, int axlat, char s,
* const char *method, const char *class, int *status )
* Class Membership:
@@ -26444,11 +26420,13 @@ static int SkySys( AstSkyFrame *skyfrm, int wcstype, int wcsproj,
* Description:
* This function sets values for the following FITS-WCS keywords
-* within the supplied FitsStore structure: CTYPE, CNAME, RADECSYS, EQUINOX,
+* within the supplied FitsStore structure: CTYPE, CNAME, RADESYS, EQUINOX,
* MJDOBS, CUNIT, OBSGEO-X/Y/Z. The values are derived from the supplied
* SkyFrame and WcsMap.
* Parameters:
+* this
+* Pointer to the FitsChan.
* skyfrm
* A pointer to the SkyFrame to be described.
* wcstype
@@ -26482,6 +26460,7 @@ static int SkySys( AstSkyFrame *skyfrm, int wcstype, int wcsproj,
*/
/* Local Variables: */
+ astDECLARE_GLOBALS /* Declare the thread specific global data */
char *label; /* Pointer to axis label string */
char lattype[MXCTYPELEN];/* Latitude axis CTYPE value */
char lontype[MXCTYPELEN];/* Longitude axis CTYPE value */
@@ -26489,38 +26468,68 @@ static int SkySys( AstSkyFrame *skyfrm, int wcstype, int wcsproj,
const char *lonsym; /* SkyFrame longitude axis symbol */
const char *prj_name; /* Pointer to projection name string */
const char *sys; /* Celestal coordinate system */
- double ep; /* Epoch of observation (MJD) */
+ const char *timesys; /* Timescale specified in FitsChan */
+ double ep; /* Epoch of observation in required timescale (MJD) */
+ double ep_tdb; /* Epoch of observation in TDB timescale (MJD) */
+ double ep_utc; /* Epoch of observation in UTC timescale (MJD) */
double eq; /* Epoch of reference equinox (MJD) */
double h; /* Geodetic altitude of observer (metres) */
double geolat; /* Geodetic latitude of observer (radians) */
double geolon; /* Geodetic longitude of observer (radians) */
- double r; /* Distance (in AU) from earth axis */
- double z; /* Distance (in AU) above earth equator */
+ double xyz[3]; /* Geocentric position vector (in m) */
int defdate; /* Can the date keywords be defaulted? */
int i; /* Character count */
int isys; /* Celestial coordinate system */
int latax; /* Index of latitude axis in SkyFrame */
int lonax; /* Index of longitude axis in SkyFrame */
+ int old_ignore_used; /* Original setting of external ignore_used variable */
int radesys; /* RA/DEC reference frame */
int ret; /* Returned flag */
/* Check the status. */
if( !astOK ) return 0;
+/* Get a pointer to the structure holding thread-specific global data. */
+ astGET_GLOBALS(this);
+
/* Check we have a SkyFrame. */
if( !astIsASkyFrame( skyfrm ) ) return 0;
/* Initialise */
ret = 1;
-/* Get the equinox, epoch of observation, and system of the SkyFrame. */
+/* Get the equinox, epoch of observation, and system of the SkyFrame. The epoch
+ is in TDB. It is assumed the Equinox is in UTC. */
eq = astGetEquinox( skyfrm );
- if( astTestEpoch( skyfrm ) ) {
- ep = TDBConv( astGetEpoch( skyfrm ), AST__UTC, 1, method, class, status );
+ sys = astGetC( skyfrm, "system" );
+ ep_tdb = astTestEpoch( skyfrm ) ? astGetEpoch( skyfrm ) : AST__BAD;
+
+/* Convert the epoch to UTC. */
+ ep_utc = TDBConv( ep_tdb, AST__UTC, 1, method, class, status );
+
+/* See if the FitsChan contains a value for the TIMESYS keyword (include
+ previously used cards in the search). If so, and if it is not UTC, convert
+ the epoch to the specified time scale, and store a TIMESYS value in the
+ FitsStore. */
+ old_ignore_used = ignore_used;
+ ignore_used = 0;
+ if( GetValue( this, "TIMESYS", AST__STRING, (void *) ×ys, 0, 0, method,
+ class, status ) && strcmp( timesys, "UTC" ) ) {
+ ep = TDBConv( ep_tdb, TimeSysToAst( this, timesys, method, class,
+ status ),
+ 1, method, class, status );
+ SetItemC( &(store->timesys), 0, 0, s, timesys, status );
+
+/* If no TIMESYS keyword was found in the FitsChan, or the timesys was
+ UTC, we use the UTC epoch value found above. In this case no TIMESYS value
+ need be stored in the FitsSTore since UTC is the default for TIMESYS. */
} else {
- ep = AST__BAD;
+ ep = ep_utc;
}
- sys = astGetC( skyfrm, "system" );
+
+/* Reinstate the original value for the flag that indicates whether keywords
+ in the FitsChan that have been used previously should be ignored. */
+ ignore_used = old_ignore_used;
/* The MJD-OBS and DATE-OBS keywords default to the epoch of the
reference equinox if not supplied. Therefore MJD-OBS and DATE-OBS do
@@ -26529,22 +26538,22 @@ static int SkySys( AstSkyFrame *skyfrm, int wcstype, int wcsproj,
producing FITS headers which say unlikely things like
DATE-OBS = "01/01/50". Set a flag indicating if MJD-OBS and DATE-OBS
can be defaulted. */
- defdate = EQUAL( ep, eq );
+ defdate = EQUAL( ep_utc, eq );
/* Convert the equinox to a Julian or Besselian epoch. Also get the
reference frame and standard system. */
if( !Ustrcmp( sys, "FK4", status ) ){
- eq = palSlaEpb( eq );
+ eq = palEpb( eq );
radesys = FK4;
isys = RADEC;
SetItemC( &(store->radesys), 0, 0, s, "FK4", status );
} else if( !Ustrcmp( sys, "FK4_NO_E", status ) || !Ustrcmp( sys, "FK4-NO-E", status ) ){
- eq = palSlaEpb( eq );
+ eq = palEpb( eq );
radesys = FK4NOE;
isys = RADEC;
SetItemC( &(store->radesys), 0, 0, s, "FK4-NO-E", status );
} else if( !Ustrcmp( sys, "FK5", status ) ){
- eq = palSlaEpj( eq );
+ eq = palEpj( eq );
radesys = FK5;
isys = RADEC;
SetItemC( &(store->radesys), 0, 0, s, "FK5", status );
@@ -26674,11 +26683,10 @@ static int SkySys( AstSkyFrame *skyfrm, int wcstype, int wcsproj,
geolat = astGetObsLat( skyfrm );
h = astGetObsAlt( skyfrm );
if( geolat != AST__BAD && geolon != AST__BAD && h != AST__BAD ) {
- palSlaGeoc( geolat, h, &r, &z );
- r *= AST__AU;
- SetItem( &(store->obsgeox), 0, 0, ' ', r*cos( geolon ), status );
- SetItem( &(store->obsgeoy), 0, 0, ' ', r*sin( geolon ), status );
- SetItem( &(store->obsgeoz), 0, 0, ' ', z*AST__AU, status );
+ iauGd2gc( 1, geolon, geolat, h, xyz );
+ SetItem( &(store->obsgeox), 0, 0, ' ', xyz[0], status );
+ SetItem( &(store->obsgeoy), 0, 0, ' ', xyz[1], status );
+ SetItem( &(store->obsgeoz), 0, 0, ' ', xyz[2], status );
}
}
if( !astOK ) ret = 0;
@@ -26896,12 +26904,11 @@ static AstMapping *SpectralAxes( AstFitsChan *this, AstFrameSet *fs,
double imagfreq; /* Image sideband equivalent to the rest frequency (Hz) */
double lbnd_s; /* Lower bound on spectral axis */
double pv; /* Value of projection parameter */
- double r; /* Distance (in AU) from earth axis */
double restfreq; /* Rest frequency (Hz) */
double ubnd_s; /* Upper bound on spectral axis */
double vsource; /* Rel.vel. of source (m/s) */
double xval; /* Value of "X" system at reference point */
- double z; /* Distance (in AU) above earth equator */
+ double xyz[3]; /* Geocentric position vector (in m) */
double zsource; /* Redshift of source */
int *inperm; /* Pointer to permutation array for input axes */
int *outperm; /* Pointer to permutation array for output axes */
@@ -27436,11 +27443,10 @@ static AstMapping *SpectralAxes( AstFitsChan *this, AstFrameSet *fs,
geolat = astGetObsLat( specfrm );
h = astGetObsAlt( specfrm );
if( geolat != AST__BAD && geolon != AST__BAD && h != AST__BAD ) {
- palSlaGeoc( geolat, h, &r, &z );
- r *= AST__AU;
- SetItem( &(store->obsgeox), 0, 0, ' ', r*cos( geolon ), status );
- SetItem( &(store->obsgeoy), 0, 0, ' ', r*sin( geolon ), status );
- SetItem( &(store->obsgeoz), 0, 0, ' ', z*AST__AU, status );
+ iauGd2gc( 1, geolon, geolat, h, xyz );
+ SetItem( &(store->obsgeox), 0, 0, ' ', xyz[0], status );
+ SetItem( &(store->obsgeoy), 0, 0, ' ', xyz[1], status );
+ SetItem( &(store->obsgeoz), 0, 0, ' ', xyz[2], status );
}
}
if( astTestRestFreq( specfrm ) ) {
@@ -28314,7 +28320,7 @@ static AstFitsChan *SpecTrans( AstFitsChan *this, int encoding,
if( 1 == astSscanf( cval + 1, " %lf ", &dval ) ){
/* If it is a Besselian epoch, convert to Julian. */
- if( bj == 'B' ) dval = palSlaEpj( palSlaEpb2d( dval ) );
+ if( bj == 'B' ) dval = palEpj( palEpb2d( dval ) );
/* Replace the original EQUINOX card. */
SetValue( ret, "EQUINOX", (void *) &dval, AST__FLOAT,
@@ -28662,7 +28668,7 @@ static AstFitsChan *SpecTrans( AstFitsChan *this, int encoding,
GetValue2( ret, this, FormatKey( "CRPIX", axlon + 1, -1, s, status ),
AST__FLOAT, (void *) &dval, 0, method, class, status ) ) {
if( cdelti != 0.0 ) {
- dval = 0.5 + AST__DR2D*palSlaDrange( AST__DD2R*( dval - 0.5 )*cdelti )/cdelti;
+ dval = 0.5 + AST__DR2D*palDrange( AST__DD2R*( dval - 0.5 )*cdelti )/cdelti;
SetValue( ret, FormatKey( "CRPIX", axlon + 1, -1, s, status ),
(void *) &dval, AST__FLOAT, CardComm( this, status ), status );
}
@@ -30576,9 +30582,9 @@ static double TDBConv( double mjd, int timescale, int fromTDB,
* Indicates the direction of the required conversion. If non-zero,
* the supplied "mjd" value should be in the TDB timescale, and the
* returned value will be in the timescale specified by "timescale".
-* Indicates the direction of the required conversion. If zero,
-* the supplied "mjd" value should be in the timescale specified by
-* "timescale", and the returned value will be in the TDB timescale.
+* If zero, the supplied "mjd" value should be in the timescale
+* specified by "timescale", and the returned value will be in the
+* TDB timescale.
* method
* The calling method. Used only in error messages.
* class
@@ -30597,8 +30603,8 @@ static double TDBConv( double mjd, int timescale, int fromTDB,
/* Initialise */
ret = AST__BAD;
-/* Check inherited status */
- if( !astOK ) return ret;
+/* Check inherited status and supplied TDB value. */
+ if( !astOK || mjd == AST__BAD ) return ret;
/* Return the supplied value if no conversion is needed. */
if( timescale == AST__TDB ) {
@@ -31000,7 +31006,8 @@ static AstTimeScaleType TimeSysToAst( AstFitsChan *this, const char *timesys,
* this
* Pointer to the FitsChan.
* timesys
-* Pointer to the string holding the TIMESYS value.
+* Pointer to the string holding the TIMESYS value. A NULL pointer
+* returns the default timescale of UTC.
* method
* Pointer to a string holding the name of the calling method.
* This is only for use in constructing error messages.
@@ -31023,7 +31030,9 @@ static AstTimeScaleType TimeSysToAst( AstFitsChan *this, const char *timesys,
/* Check the inherited status. */
if( !astOK ) return result;
- if( !strcmp( timesys, "UTC" ) ) {
+ if( !timesys ) {
+ result = AST__UTC;
+ } else if( !strcmp( timesys, "UTC" ) ) {
result = AST__UTC;
} else if( !strcmp( timesys, "UT" ) ) {
result = AST__UTC;
@@ -31635,6 +31644,13 @@ static int WATCoeffs( const char *watstr, int iaxis, double **cvals,
*cvals = NULL;
*ok = 1;
+/* Other initialisation to avoid compiler warnings. */
+ etamin = 0.0;
+ etamin = 0.0;
+ ximax = 0.0;
+ ximin = 0.0;
+ order = 0;
+
/* Check the global status. */
if ( !astOK || !watstr ) return result;
@@ -32033,6 +32049,9 @@ static AstMapping *WcsCelestial( AstFitsChan *this, FitsStore *store, char s,
*reflat = AST__BAD;
*reffrm = NULL;
+/* Other initialisation to avoid compiler warnings. */
+ map1 = NULL;
+
/* Check the global status. */
if ( !astOK ) return ret;
@@ -33093,16 +33112,11 @@ static void WcsFcRead( AstFitsChan *fc, AstFitsChan *fc2, FitsStore *store,
/* Is this a TIMESYS keyword? */
} else if( Match( keynam, "TIMESYS", 0, fld, &nfld, method, class, status ) ){
- item = NULL;
- if( CnvValue( fc, AST__STRING, 0, &cval, method, status ) ) {
- store->timesys = TimeSysToAst( fc, cval, method, class, status );
- MarkCard( fc, status );
- } else {
- sprintf( buf, "The original FITS header contained a value for "
- "keyword TIMESYS which could not be converted to a "
- "character string." );
- Warn( fc, "badval", buf, method, class, status );
- }
+ item = &(store->timesys);
+ type = AST__STRING;
+ i = 0;
+ jm = 0;
+ s = ' ';
/* Following keywords are used to describe "-SIP" distortion as used by
the Spitzer project... */
@@ -33227,7 +33241,6 @@ static int WcsFromStore( AstFitsChan *this, FitsStore *store,
* Private function.
* Synopsis:
-
* int WcsFromStore( AstFitsChan *this, FitsStore *store,
* const char *method, const char *class, int *status )
@@ -33292,10 +33305,12 @@ static int WcsFromStore( AstFitsChan *this, FitsStore *store,
int prj; /* Projection type */
int ret; /* Returned value */
-
/* Initialise */
ret = 0;
+/* Other initialisation to avoid compiler warnings. */
+ tabaxis = NULL;
+
/* Check the inherited status. */
if( !astOK ) return ret;
@@ -33533,14 +33548,14 @@ static int WcsFromStore( AstFitsChan *this, FitsStore *store,
/* The format used for the DATE-OBS keyword depends on the value of the
keyword. For DATE-OBS < 1999.0, use the old "dd/mm/yy" format.
Otherwise, use the new "ccyy-mm-ddThh:mm:ss[.ssss]" format. */
- palSlaCaldj( 99, 1, 1, &mjd99, &jj );
+ palCaldj( 99, 1, 1, &mjd99, &jj );
if( val < mjd99 ) {
- palSlaDjcal( 0, val, iymdf, &jj );
+ palDjcal( 0, val, iymdf, &jj );
sprintf( combuf, "%2.2d/%2.2d/%2.2d", iymdf[ 2 ], iymdf[ 1 ],
iymdf[ 0 ] - ( ( iymdf[ 0 ] > 1999 ) ? 2000 : 1900 ) );
} else {
- palSlaDjcl( val, iymdf, iymdf+1, iymdf+2, &fd, &jj );
- palSlaDd2tf( 3, fd, sign, ihmsf );
+ palDjcl( val, iymdf, iymdf+1, iymdf+2, &fd, &jj );
+ palDd2tf( 3, fd, sign, ihmsf );
sprintf( combuf, "%4.4d-%2.2d-%2.2dT%2.2d:%2.2d:%2.2d.%3.3d",
iymdf[0], iymdf[1], iymdf[2], ihmsf[0], ihmsf[1],
ihmsf[2], ihmsf[3] );
@@ -33554,6 +33569,11 @@ static int WcsFromStore( AstFitsChan *this, FitsStore *store,
val = GetItem( &(store->mjdavg), 0, 0, ' ', NULL, method, class, status );
if( val != AST__BAD ) SetValue( this, "MJD-AVG", &val, AST__FLOAT,
"Average Modified Julian Date of observation", status );
+
+/* Store the timescale in TIMESYS. */
+ cval = GetItemC( &(store->timesys), 0, 0, s, NULL, method, class, status );
+ if( cval ) SetValue( this, "TIMESYS", &cval, AST__STRING,
+ "Timescale for MJD-OBS/MJD-AVG values", status );
}
/* Numerical projection parameters */
@@ -34395,7 +34415,7 @@ static AstMapping *WcsNative( AstFitsChan *this, FitsStore *store, char s,
/* Limit the latitude to the range +/- PI/2, issuing a warning if the
supplied CRVAL value is outside this range. The "alphap" variable is used
as workspace here. */
- alphap = palSlaDrange( delta0 );
+ alphap = palDrange( delta0 );
delta0 = alphap;
if ( delta0 > AST__DPIBY2 ){
delta0 = AST__DPIBY2;
@@ -34759,8 +34779,8 @@ static int WcsNatPole( AstFitsChan *this, AstWcsMap *wcsmap, double alpha0,
} else {
t4 = acos( t3 );
}
- deltap_1 = palSlaDrange( t1 + t4 );
- deltap_2 = palSlaDrange( t1 - t4 );
+ deltap_1 = palDrange( t1 + t4 );
+ deltap_2 = palDrange( t1 - t4 );
/* Select which of these two values of deltap to use. Values outside the
range +/- PI/2 cannot be used. If both values are within this range
@@ -35414,9 +35434,9 @@ static AstSkyFrame *WcsSkyFrame( AstFitsChan *this, FitsStore *store, char s,
/* Convert the equinox to a Modified Julian Date. */
if( equinox != AST__BAD ) {
if( bj == 'B' ) {
- eqmjd = palSlaEpb2d( equinox );
+ eqmjd = palEpb2d( equinox );
} else {
- eqmjd = palSlaEpj2d( equinox );
+ eqmjd = palEpj2d( equinox );
}
} else {
eqmjd = AST__BAD;
@@ -35424,7 +35444,7 @@ static AstSkyFrame *WcsSkyFrame( AstFitsChan *this, FitsStore *store, char s,
/* Get a value for the Epoch attribute. If no value is available, use
EQUINOX and issue a warning. */
- mjdobs = ChooseEpoch( store, s, method, class, status );
+ mjdobs = ChooseEpoch( this, store, s, method, class, status );
if( mjdobs == AST__BAD ) {
mjdobs = eqmjd;
if( mjdobs != AST__BAD ) {
@@ -35523,7 +35543,7 @@ static AstSkyFrame *WcsSkyFrame( AstFitsChan *this, FitsStore *store, char s,
if( obsgeo[ 0 ] != AST__BAD &&
obsgeo[ 1 ] != AST__BAD &&
obsgeo[ 2 ] != AST__BAD ) {
- Geod( obsgeo, &geolat, &h, &geolon, status );
+ iauGc2gd( 1, obsgeo, &geolon, &geolat, &h );
astSetObsLat( ret, geolat );
astSetObsLon( ret, geolon );
astSetObsAlt( ret, h );
@@ -35693,7 +35713,7 @@ static AstMapping *WcsSpectral( AstFitsChan *this, FitsStore *store, char s,
astSetUnit( iwcfrm, i, cunit );
/* Get a value for the Epoch attribute (the date of observation). */
- mjd = ChooseEpoch( store, s, method, class, status );
+ mjd = ChooseEpoch( this, store, s, method, class, status );
if( mjd != AST__BAD ) astSetEpoch( specfrm, mjd );
/* Set the rest frequency. Use the RESTFRQ keyword (assumed to be in Hz),
@@ -35714,7 +35734,7 @@ static AstMapping *WcsSpectral( AstFitsChan *this, FitsStore *store, char s,
if( obsgeo[ 0 ] != AST__BAD &&
obsgeo[ 1 ] != AST__BAD &&
obsgeo[ 2 ] != AST__BAD ) {
- Geod( obsgeo, &geolat, &h, &geolon, status );
+ iauGc2gd( 1, obsgeo, &geolon, &geolat, &h );
astSetObsLat( specfrm, geolat );
astSetObsLon( specfrm, geolon );
astSetObsAlt( specfrm, h );
@@ -36012,9 +36032,12 @@ static int WorldAxes( AstFitsChan *this, AstMapping *cmap, double *dim, int *per
int retain;
int used;
-/* Initialise */
+/* Initialise returned value */
ret = 0;
+/* Other initialisation to avoid compiler warnings. */
+ retain = 0;
+
/* Check the status */
if( !astOK ) return ret;
@@ -36432,7 +36455,6 @@ static int Write( AstChannel *this_channel, AstObject *object, int *status ) {
int comm; /* Value of Comm attribute */
int encoding; /* FITS encoding scheme to use */
int i; /* Axis index */
- int icurr; /* Original current Frame index */
int naxis; /* No. of pixel axes */
int ret; /* Number of objects read */
@@ -36547,24 +36569,11 @@ static int Write( AstChannel *this_channel, AstObject *object, int *status ) {
dim + i ) ) dim[ i ] = AST__BAD;
}
-/* Add a new current Frame into the FrameSet which increases the chances of
- the requested encoding being usable. The index of the original current
- Frame is returned, or AST__NOFRAME if no new Frame was added. */
- icurr = AddEncodingFrame( this, (AstFrameSet *) object,
- encoding, method, class, status );
-
/* Extract the required information from the FrameSet into a standard
intermediary structure called a FitsStore. The indices of any
celestial axes are returned. */
store = FsetToStore( this, (AstFrameSet *) object, naxis, dim,
- method, class, status );
-
-/* Remove the Frame (if any) added above, and re-instate the original current
- Frame. */
- if( icurr != AST__NOFRAME ) {
- astRemoveFrame( (AstFrameSet *) object, AST__CURRENT );
- astSetCurrent( (AstFrameSet *) object, icurr );
- }
+ encoding, method, class, status );
/* If the FrameSet cannot be described in terms of any of the supported
FITS encodings, a null pointer will have been returned. */
diff --git a/frame.c b/frame.c
index 0be6b04..3531ed0 100644
--- a/frame.c
+++ b/frame.c
@@ -1241,7 +1241,7 @@ f invoked with STATUS set to an error value, or if it should fail for
angc = atan2( cb[ 0 ], cb[ 1 ] );
/* Find the difference, folded into the range +/- PI. */
- result = palSlaDrange( angc - anga );
+ result = palDrange( angc - anga );
/* Now deal with Frames with more than 2 axes. */
} else {
@@ -4620,8 +4620,8 @@ L1:
/* Format the Epoch as decimal years. Use a Besselian epoch if it will
be less than 1984.0, otherwise use a Julian epoch. */
- result = astFmtDecimalYr( ( epoch < palSlaEpj2d( 1984.0 ) ) ?
- palSlaEpb( epoch ) : palSlaEpj( epoch ), DBL_DIG );
+ result = astFmtDecimalYr( ( epoch < palEpj2d( 1984.0 ) ) ?
+ palEpb( epoch ) : palEpj( epoch ), DBL_DIG );
}
/* Top(axis). */
@@ -4806,7 +4806,7 @@ L1:
if ( astOK ) {
/* Put into range +/- PI. */
- dval = palSlaDrange( dval );
+ dval = palDrange( dval );
/* If not already created, create an FK5 J2000 SkyFrame which will be used
for formatting and unformatting ObsLon and ObsLat values. */
@@ -8144,7 +8144,7 @@ double astReadDateTime_( const char *value, int *status ) {
&& ( nc >= len ) ) {
/* Convert to Modified Julian Date. */
- result = palSlaEpb2d( epoch );
+ result = palEpb2d( epoch );
/* Julian epoch in decimal years (e.g. "J2000.0"). */
/* =============================================== */
@@ -8153,7 +8153,7 @@ double astReadDateTime_( const char *value, int *status ) {
&& ( nc >= len ) ) {
/* Convert to Modified Julian Date. */
- result = palSlaEpj2d( epoch );
+ result = palEpj2d( epoch );
/* Decimal years (e.g. "1976.2"). */
/* ============================== */
@@ -8163,7 +8163,7 @@ double astReadDateTime_( const char *value, int *status ) {
/* Convert to Modified Julian Date, treating the epoch as Julian or Besselian
depending on whether it is 1984.0 or later. */
- result = ( epoch < 1984.0 ) ? palSlaEpb2d( epoch ) : palSlaEpj2d( epoch );
+ result = ( epoch < 1984.0 ) ? palEpb2d( epoch ) : palEpj2d( epoch );
/* Modified Julian Date (e.g. "MJD 54321.0"). */
/* ============================================ */
@@ -8396,7 +8396,7 @@ double astReadDateTime_( const char *value, int *status ) {
to a Modified Julian Date. */
if ( astOK ) {
iday = (int) day;
- palSlaCaldj( year, month, iday, &mjd, &stat );
+ palCaldj( year, month, iday, &mjd, &stat );
/* Examine the return status from the conversion and report an appropriate
error if necessary. */
@@ -8419,7 +8419,7 @@ double astReadDateTime_( const char *value, int *status ) {
/* Convert hours, minutes and seconds to a fraction of a day (this will give
zero if none of these quantities was supplied). */
- palSlaDtf2d( hour, minute, sec, &hms, &stat );
+ palDtf2d( hour, minute, sec, &hms, &stat );
/* Examine the return status from the conversion and report an appropriate
error if necessary. */
@@ -11563,7 +11563,7 @@ astMAKE_CLEAR(Frame,Epoch,epoch,AST__BAD)
/* Provide a default value of J2000.0 setting. */
astMAKE_GET(Frame,Epoch,double,AST__BAD,(
- ( this->epoch != AST__BAD ) ? this->epoch : palSlaEpj2d( 2000.0 )))
+ ( this->epoch != AST__BAD ) ? this->epoch : palEpj2d( 2000.0 )))
/* Allow any Epoch value to be set. */
astMAKE_SET(Frame,Epoch,double,epoch,value)
@@ -13277,8 +13277,8 @@ static void Dump( AstObject *this_object, AstChannel *channel, int *status ) {
dval = set ? GetEpoch( this, status ) : astGetEpoch( this );
/* Convert MJD to Besselian or Julian years, depending on the value. */
- bessyr = ( dval < palSlaEpj2d( 1984.0 ) );
- dval = bessyr ? palSlaEpb( dval ) : palSlaEpj( dval );
+ bessyr = ( dval < palEpj2d( 1984.0 ) );
+ dval = bessyr ? palEpb( dval ) : palEpj( dval );
astWriteDouble( channel, "Epoch", set, !isFrame, dval,
bessyr ? "Besselian epoch of observation" :
"Julian epoch of observation" );
@@ -14145,8 +14145,8 @@ AstFrame *astLoadFrame_( void *mem, size_t size,
/* Interpret this as Besselian or Julian depending on its value. */
new->epoch = astReadDouble( channel, "epoch", AST__BAD );
if ( TestEpoch( new, status ) ) {
- SetEpoch( new, ( new->epoch < 1984.0 ) ? palSlaEpb2d( new->epoch ) :
- palSlaEpj2d( new->epoch ), status );
+ SetEpoch( new, ( new->epoch < 1984.0 ) ? palEpb2d( new->epoch ) :
+ palEpj2d( new->epoch ), status );
}
/* Digits. */
diff --git a/mapping.c b/mapping.c
index 911bd87..dfb0055 100644
--- a/mapping.c
+++ b/mapping.c
@@ -8229,7 +8229,7 @@ static double MatrixDet( int ndim, const double *matrix, int *status ){
y = astMalloc( sizeof( double )*(size_t) ndim );
if( y ) {
for( i = 0; i < ndim; i++ ) y[ i ] = 1.0;
- palSlaDmat( ndim, a, y, &result, &jf, iw );
+ palDmat( ndim, a, y, &result, &jf, iw );
}
y = astFree( y );
iw = astFree( iw );
@@ -8851,7 +8851,7 @@ f - A value of .FALSE.
/* Now find the solution vector (the solution over-writes teh current
contents of "ofit"). */
- palSlaDmat( 6, mat, ofit, &det, &sing, iw );
+ palDmat( 6, mat, ofit, &det, &sing, iw );
/* If the fit failed, fill the coefficient array with bad values. */
if( sing != 0 ) {
diff --git a/matrixmap.c b/matrixmap.c
index 77f5d51..25f70b9 100644
--- a/matrixmap.c
+++ b/matrixmap.c
@@ -1362,9 +1362,9 @@ static double *InvertMatrix( int form, int nrow, int ncol, double *matrix, int *
double det; /* Determinant of supplied matrix */
double mval; /* Matrix element value */
double *out; /* Pointer to returned inverse matrix */
- double *vector; /* Pointer to vector used by palSlaDmat */
+ double *vector; /* Pointer to vector used by palDmat */
int i; /* Matrix element number */
- int *iw; /* Pointer to workspace used by palSlaDmat */
+ int *iw; /* Pointer to workspace used by palDmat */
int nel; /* No. of elements in square matrix */
int ndiag; /* No. of diagonal elements */
int ok; /* Zero if any bad matrix values found */
@@ -1444,7 +1444,7 @@ static double *InvertMatrix( int form, int nrow, int ncol, double *matrix, int *
/* Obtain work space and attempt to invert the matrix using SLALIB, then
free the work space. */
iw = (int *) astMalloc( sizeof(int)*(size_t) nrow );
- if( astOK ) palSlaDmat( nrow, out, vector, &det, &sing, iw );
+ if( astOK ) palDmat( nrow, out, vector, &det, &sing, iw );
iw = (int *) astFree( (void *) iw );
}
diff --git a/pal.c b/pal.c
index 9004e3f..a82de9c 100644
--- a/pal.c
+++ b/pal.c
@@ -1,1145 +1,298 @@
+#if !defined( PAL_INCLUDED ) /* Include this file only once */
+#define PAL_INCLUDED
/*
-** Author:
-** Patrick Wallace (ptw at tpsoft.demon.co.uk)
-**
-** License:
-** This program is free software; you can redistribute it and/or modify
-** it under the terms of the GNU General Public License as published by
-** the Free Software Foundation; either version 2 of the License, or
-** (at your option) any later version.
-**
-** This program is distributed in the hope that it will be useful,
-** but WITHOUT ANY WARRANTY; without even the implied warranty of
-** MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
-** GNU General Public License for more details.
-**
-** You should have received a copy of the GNU General Public License
-** along with this program; if not, write to the Free Software
-** Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
-** USA.
-**
-** History:
-** 14-JUN-2005 (DSB):
-** Corrected palSlaDsepv to fix bug which caused precisely antipodal
-** vectors to return zero instead of pi.
-** 16-AUG-2005 (DSB):
-** Added palSlaDh2e and palSlaDe2h by translating the corresponding
-** fortran routines into C (by hand).
-** 6-OCT-2006 (DSB):
-** Added palSlaGmsta by translating the corresponding fortran routines
-** into C (by hand).
-** 31-AUG-2007 (DSB):
-** Modify palSlaDe2h and palSlaDh2e to apply correction for diurnal
-** aberration.
-** 18-JUN-2009 (DSB):
-** Added palSlaPvobs by translating the corresponding fortran routine
-** into C (by hand).
-** 5-APR-2011 (DSB):
-** Change palSlaDrange to better handle cases where the supplied
-** value is very close to +/- PI.
+* Name:
+* pal.c
+
+* Purpose:
+* A wrapper for all PAL functions used by AST.
+
+* Description:
+* This file is a wrapper that includes all the source files from
+* the PAL and SOFA libraries. This is done so that the function
+* names can be changed from the usual "palXxx" and "iauXxx" forms to
+* the private "astPalXxx" and "astIauXxx" forms. This renaming is
+* performed via the macros defined in the pal2ast.h and sofa2ast.h
+* include files. This is done in order to prevent clashes with any
+* external PAL or SOFA libraries with which an application is linked.
+*
+* This file expects to find the publicly distributed and unmodified
+* PAL and SOFA source code in a pair of subdirectory called "pal" and
+* "sofa" within the current directory. The files within these
+* subdirectories do not need to be compiled - only this wrapper file
+* needs to be compiled.
+
+* Copyright:
+* Copyright (C) 2011 Science & Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public Licence as
+* published by the Free Software Foundation; either version 2 of
+* the Licence, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful,but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public Licence for more details.
+*
+* You should have received a copy of the GNU General Public Licence
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street,Fifth Floor, Boston, MA
+* 02110-1301, USA
+
+* Authors:
+* DSB: D.S. Berry (JAC, Hawaii)
+
+* History:
+* 16-FEB-2012 (DSB):
+* Original version.
*/
-#include "pal.h"
-#include "slamac.h"
-
-void palSlaAddet(double Q0,double FOo,double q1,double*bAR,
-double*q2){double Q3[3];double baz[3];int Q4;palSlaEtrms(q1,Q3)
-;palSlaDcs2c(Q0,FOo,baz);for(Q4=0;Q4<3;Q4++){baz[Q4]+=Q3[Q4];}
-palSlaDcc2s(baz,bAR,q2);*bAR=palSlaDranrm(*bAR);}
-
-void palSlaAmpqk(double fOo,double bar,double baz[21],double*Q0
-,double*FobaR){double Q1;double q2;double foobar[3];double
-q3[3];double q4[3],FobAZ[3],q5[3],FOOBAZ[3];double q6,QUUX,
-FRED,Q7,q8,Q9;int DOG,CAT;Q1=baz[7];q2=baz[11];for(DOG=0;DOG
-<3;DOG++){foobar[DOG]=baz[DOG+4];q3[DOG]=baz[DOG+8];}
-palSlaDcs2c(fOo,bar,FOOBAZ);palSlaDimxv((double(*)[3])&baz[12],
-FOOBAZ,q5);q6=q2+1.0;for(DOG=0;DOG<3;DOG++){FobAZ[DOG]=q5[
-DOG];}for(CAT=0;CAT<2;CAT++){QUUX=palSlaDvdv(FobAZ,q3);FRED=1.0
-+QUUX;Q7=1.0+QUUX/q6;for(DOG=0;DOG<3;DOG++){FobAZ[DOG]=(FRED
-*q5[DOG]-Q7*q3[DOG])/q2;}palSlaDvn(FobAZ,FOOBAZ,&Q7);for(DOG=0;
-DOG<3;DOG++){FobAZ[DOG]=FOOBAZ[DOG];}}for(DOG=0;DOG<3;DOG++)
-{q4[DOG]=FobAZ[DOG];}for(CAT=0;CAT<5;CAT++){q8=palSlaDvdv(q4,
-foobar);Q9=1.0+q8;Q7=Q9-Q1*q8;for(DOG=0;DOG<3;DOG++){q4[DOG]
-=(Q9*FobAZ[DOG]-Q1*foobar[DOG])/Q7;}palSlaDvn(q4,q5,&Q7);for(
-DOG=0;DOG<3;DOG++){q4[DOG]=q5[DOG];}}palSlaDcc2s(q4,Q0,FobaR);*
-Q0=palSlaDranrm(*Q0);}
-
-void palSlaAoppa(double Q0,double q1,double q2,double Q3,double
- Q4,double Q5,double Q6,double foo,double BAR,double Q7,
-double BAZ,double FoBar,double Q8[14])
-#define q9 173.14463331
-#define Q10 1.00273790935
-{double q11,Q12,foobar,FOBAZ,q13,FOOBAZ,quUX,q14,q15,fReD,
-DOG;q11=cos(Q3);Q12=cos(q2)*q11;foobar=sin(q2)*q11;FOBAZ=sin
-(Q3);q13=Q12-Q5*FOBAZ;FOOBAZ=foobar+Q6*FOBAZ;quUX=Q5*Q12-Q6*
-foobar+FOBAZ;q14=(q13!=0.0||FOOBAZ!=0.0)?atan2(FOOBAZ,q13):
-0.0;q15=atan2(quUX,sqrt(q13*q13+FOOBAZ*FOOBAZ));Q8[0]=q15;Q8
-[1]=sin(q15);Q8[2]=cos(q15);palSlaGeoc(q15,Q4,&fReD,&DOG);Q8[3]
-=D2PI*fReD*Q10/q9;Q8[4]=Q4;Q8[5]=foo;Q8[6]=BAR;Q8[7]=Q7;Q8[8
-]=BAZ;Q8[9]=FoBar;palSlaRefco(Q4,foo,BAR,Q7,BAZ,q15,FoBar,1e-10
-,&Q8[10],&Q8[11]);Q8[12]=q14+palSlaEqeqx(Q0)+q1*Q10*DS2R;
-palSlaAoppat(Q0,Q8);}
-#undef q9
-#undef Q10
-
-void palSlaAoppat(double Q0,double FOO[14]){FOO[13]=palSlaGmst(Q0)
-+FOO[12];}
-
-void palSlaCaldj(int FOO,int Q0,int BAr,double*Q1,int*baz){int
-q2;if((FOO>=0)&&(FOO<=49))q2=FOO+2000;else if((FOO>=50)&&(
-FOO<=99))q2=FOO+1900;else q2=FOO;palSlaCldj(q2,Q0,BAr,Q1,baz);}
-
-void palSlaCldj(int Q0,int foo,int Q1,double*q2,int*Q3){long Q4
-,q5;static int bar[12]={31,28,31,30,31,30,31,31,30,31,30,31}
-;if(Q0<-4699){*Q3=1;return;}if((foo<1)||(foo>12)){*Q3=2;
-return;}bar[1]=(((Q0%4)==0)&&(((Q0%100)!=0)||((Q0%400)==0)))
-?29:28;*Q3=(Q1<1||Q1>bar[foo-1])?3:0;Q4=(long)Q0;q5=(long)
-foo;*q2=(double)((1461L*(Q4-(12L-q5)/10L+4712L))/4L+(306L*((
-q5+9L)%12L)+5L)/10L-(3L*((Q4-(12L-q5)/10L+4900L)/100L))/4L+(
-long)Q1-2399904L);}
-
-void palSlaCs2c(float q0,float FOO,float q1[3]){float BAR;BAR=(
-float)cos(FOO);q1[0]=(float)cos(q0)*BAR;q1[1]=(float)sin(q0)
-*BAR;q1[2]=(float)sin(FOO);}
-
-void palSlaDaf2r(int Q0,int FOO,double Q1,double*bar,int*baz){*
-baz=0;if((Q1<0.0)||(Q1>=60.0)){*baz=3;return;}if((FOO<0)||(
-FOO>59)){*baz=2;return;}if((Q0<0)||(Q0>359)){*baz=1;return;}
-*bar=DAS2R*(60.0*(60.0*(double)Q0+(double)FOO)+Q1);}
-
-void palSlaDav2m(double q0[3],double q1[3][3]){double FoO,bar,
-Q2,baz,FOBAR,FOOBAR,FobAZ;FoO=q0[0];bar=q0[1];Q2=q0[2];baz=
-sqrt(FoO*FoO+bar*bar+Q2*Q2);FOBAR=sin(baz);FOOBAR=cos(baz);
-FobAZ=1.0-FOOBAR;if(baz!=0.0){FoO=FoO/baz;bar=bar/baz;Q2=Q2/
-baz;}q1[0][0]=FoO*FoO*FobAZ+FOOBAR;q1[0][1]=FoO*bar*FobAZ+Q2
-*FOBAR;q1[0][2]=FoO*Q2*FobAZ-bar*FOBAR;q1[1][0]=FoO*bar*
-FobAZ-Q2*FOBAR;q1[1][1]=bar*bar*FobAZ+FOOBAR;q1[1][2]=bar*Q2
-*FobAZ+FoO*FOBAR;q1[2][0]=FoO*Q2*FobAZ+bar*FOBAR;q1[2][1]=
-bar*Q2*FobAZ-FoO*FOBAR;q1[2][2]=Q2*Q2*FobAZ+FOOBAR;}
-
-double palSlaDbear(double q0,double FOo,double q1,double BAR){
-double BAZ,q2,q3;BAZ=q1-q0;q3=sin(BAZ)*cos(BAR);q2=sin(BAR)*
-cos(FOo)-cos(BAR)*sin(FOo)*cos(BAZ);return(q2!=0.0||q3!=0.0)
-?atan2(q3,q2):0.0;}
-
-void palSlaDc62s(double FoO[6],double*bar,double*Q0,double*q1,
-double*q2,double*baz,double*q3){double q4,FoBAR,foobar,foBaz
-,q5,FOOBAZ,Q6,q7,quux,q8;q4=FoO[0];FoBAR=FoO[1];foobar=FoO[2
-];foBaz=FoO[3];q5=FoO[4];FOOBAZ=FoO[5];Q6=q4*q4+FoBAR*FoBAR;
-if((quux=Q6+foobar*foobar)==0.0){q4=foBaz;FoBAR=q5;foobar=
-FOOBAZ;Q6=q4*q4+FoBAR*FoBAR;quux=Q6+foobar*foobar;}q7=sqrt(
-Q6);q8=q4*foBaz+FoBAR*q5;if(Q6!=0.0){*bar=atan2(FoBAR,q4);*
-Q0=atan2(foobar,q7);*q2=(q4*q5-FoBAR*foBaz)/Q6;*baz=(FOOBAZ*
-Q6-foobar*q8)/(quux*q7);}else{*bar=0.0;*Q0=(foobar!=0.0)?
-atan2(foobar,q7):0.0;*q2=0.0;*baz=0.0;}*q3=((*q1=sqrt(quux))
-!=0.0)?(q8+foobar*FOOBAZ)/(*q1):0.0;}
-
-void palSlaDcc2s(double Q0[3],double*Q1,double*FoO){double bar,
-Q2,BAZ,fobar;bar=Q0[0];Q2=Q0[1];BAZ=Q0[2];fobar=sqrt(bar*bar
-+Q2*Q2);*Q1=(fobar!=0.0)?atan2(Q2,bar):0.0;*FoO=(BAZ!=0.0)?
-atan2(BAZ,fobar):0.0;}
-
-void palSlaDcs2c(double FOO,double baR,double baz[3]){double Q0
-;Q0=cos(baR);baz[0]=cos(FOO)*Q0;baz[1]=sin(FOO)*Q0;baz[2]=
-sin(baR);}
-
-void palSlaDd2tf(int foo,double q0,char*Q1,int BAR[4])
-#define q2 86400.0
-{double baz,Q3,FOBAR,q4,q5,Q6,Q7,Q8;*Q1=(char)((q0<0.0)?'-':
-'+');baz=pow(10.0,(double)gmax(foo,0));baz=dint(baz);Q3=baz*
-60.0;FOBAR=Q3*60.0;q4=baz*q2*fabs(q0);q4=dnint(q4);q5=q4/
-FOBAR;q5=dint(q5);q4=q4-q5*FOBAR;Q6=q4/Q3;Q6=dint(Q6);q4=q4-
-Q6*Q3;Q7=q4/baz;Q7=dint(Q7);Q8=q4-Q7*baz;BAR[0]=(int)q5;BAR[
-1]=(int)Q6;BAR[2]=(int)Q7;BAR[3]=(int)Q8;}
-#undef q2
-
-#include <string.h>
-void palSlaDeuler(char*Q0,double FoO,double BAR,double Q1,
-double baz[3][3]){int fobar,fOObaR,Q2,FoBaz,q3;double q4[3][
-3],Q5[3][3],q6,q7,Q8,foobaz,Q9[3][3];char q10;for(fobar=0;
-fobar<3;fobar++){for(fOObaR=0;fOObaR<3;fOObaR++){q4[fOObaR][
-fobar]=(fOObaR==fobar)?1.0:0.0;}}Q2=strlen(Q0);for(FoBaz=0;
-FoBaz<3;FoBaz++){if(FoBaz<=Q2){for(fobar=0;fobar<3;fobar++){
-for(fOObaR=0;fOObaR<3;fOObaR++){Q5[fOObaR][fobar]=(fOObaR==
-fobar)?1.0:0.0;}}switch(FoBaz){case 0:q6=FoO;break;case 1:q6
-=BAR;break;default:q6=Q1;break;}q7=sin(q6);Q8=cos(q6);q10=Q0
-[FoBaz];if((q10=='X')||(q10=='x')||(q10=='1')){Q5[1][1]=Q8;
-Q5[1][2]=q7;Q5[2][1]=-q7;Q5[2][2]=Q8;}else if((q10=='Y')||(
-q10=='y')||(q10=='2')){Q5[0][0]=Q8;Q5[0][2]=-q7;Q5[2][0]=q7;
-Q5[2][2]=Q8;}else if((q10=='Z')||(q10=='z')||(q10=='3')){Q5[
-0][0]=Q8;Q5[0][1]=q7;Q5[1][0]=-q7;Q5[1][1]=Q8;}else{Q2=0;}
-for(fOObaR=0;fOObaR<3;fOObaR++){for(fobar=0;fobar<3;fobar++)
-{foobaz=0.0;for(q3=0;q3<3;q3++){foobaz+=Q5[fOObaR][q3]*q4[q3
-][fobar];}Q9[fOObaR][fobar]=foobaz;}}for(fobar=0;fobar<3;
-fobar++){for(fOObaR=0;fOObaR<3;fOObaR++){q4[fOObaR][fobar]=
-Q9[fOObaR][fobar];}}}}for(fobar=0;fobar<3;fobar++){for(
-fOObaR=0;fOObaR<3;fOObaR++){baz[fOObaR][fobar]=q4[fOObaR][
-fobar];}}}
-
-void palSlaDimxv(double FOO[3][3],double Q0[3],double BAR[3]){
-int Q1,baz;double q2,FOBAR[3];for(baz=0;baz<3;baz++){q2=0.0;
-for(Q1=0;Q1<3;Q1++){q2+=FOO[Q1][baz]*Q0[Q1];}FOBAR[baz]=q2;}
-for(baz=0;baz<3;baz++){BAR[baz]=FOBAR[baz];}}
-
-void palSlaDjcal(int Q0,double Q1,int FOO[4],int*Q2){double q3,
-Q4,Q5,Q6;long bar,baz,q7;if((Q1<=-2395520.0)||(Q1>=1.0e9)){*
-Q2=-1;return;}else{q3=pow(10.0,(double)gmax(Q0,0));q3=dnint(
-q3);Q4=Q1*q3;Q4=dnint(Q4);Q5=dmod(Q4,q3);if(Q5<0.0)Q5+=q3;Q6
-=(Q4-Q5)/q3;bar=(long)dnint(Q6)+2400001L;baz=4L*(bar+((2L*((
-4L*bar-17918L)/146097L)*3L)/4L+1L)/2L-37L);q7=10L*(((baz-
-237L)%1461L)/4L)+5L;FOO[0]=(int)((baz/1461L)-4712L);FOO[1]=(
-int)(((q7/306L+2L)%12L)+1L);FOO[2]=(int)((q7%306L)/10L+1L);
-FOO[3]=(int)dnint(Q5);*Q2=0;}}
-
-void palSlaDjcl(double q0,int*foo,int*q1,int*bar,double*BAZ,int
-*Q2){double q3,Q4;long FOBAR,q5,Q6;if((q0<=-2395520.0)||(q0
->=1e9)){*Q2=-1;return;}else{*Q2=0;q3=dmod(q0,1.0);if(q3<0.0)
-q3+=1.0;Q4=q0-q3;Q4=dnint(Q4);FOBAR=(long)dnint(Q4)+2400001;
-q5=4L*(FOBAR+((6L*((4L*FOBAR-17918L)/146097L))/4L+1L)/2L-37L
-);Q6=10L*(((q5-237L)%1461L)/4L)+5L;*foo=(int)(q5/1461L-4712L
-);*q1=(int)(((Q6/306L+2L)%12L)+1L);*bar=(int)((Q6%306L)/10L+
-1L);*BAZ=q3;*Q2=0;}}
-
-void palSlaDmat(int FoO,double*bar,double*q0,double*Q1,int*q2,
-int*Q3)
-#define baz 1e-20
-{int Q4,fobar,Q5,FoOBAr,q6;double q7,fobaz,Q8;double*FOOBAZ,
-*QuUX,*q9;*q2=0;*Q1=1.0;for(Q4=0,FOOBAZ=bar;Q4<FoO;Q4++,
-FOOBAZ+=FoO){q7=fabs(FOOBAZ[Q4]);fobar=Q4;q9=FOOBAZ;if(Q4!=
-FoO){for(Q5=Q4+1,QuUX=FOOBAZ+FoO;Q5<FoO;Q5++,QuUX+=FoO){
-fobaz=fabs(QuUX[Q4]);if(fobaz>q7){q7=fobaz;fobar=Q5;q9=QuUX;
-}}}if(q7<baz){*q2=-1;}else{if(fobar!=Q4){for(FoOBAr=0;FoOBAr
-<FoO;FoOBAr++){fobaz=FOOBAZ[FoOBAr];FOOBAZ[FoOBAr]=q9[FoOBAr
-];q9[FoOBAr]=fobaz;}fobaz=q0[Q4];q0[Q4]=q0[fobar];q0[fobar]=
-fobaz;*Q1=-*Q1;}Q3[Q4]=fobar;*Q1*=FOOBAZ[Q4];if(fabs(*Q1)<
-baz){*q2=-1;}else{FOOBAZ[Q4]=1.0/FOOBAZ[Q4];for(FoOBAr=0;
-FoOBAr<FoO;FoOBAr++){if(FoOBAr!=Q4){FOOBAZ[FoOBAr]*=FOOBAZ[
-Q4];}}Q8=q0[Q4]*FOOBAZ[Q4];q0[Q4]=Q8;for(Q5=0,QuUX=bar;Q5<
-FoO;Q5++,QuUX+=FoO){if(Q5!=Q4){for(FoOBAr=0;FoOBAr<FoO;
-FoOBAr++){if(FoOBAr!=Q4){QuUX[FoOBAr]-=QuUX[Q4]*FOOBAZ[
-FoOBAr];}}q0[Q5]-=QuUX[Q4]*Q8;}}for(Q5=0,QuUX=bar;Q5<FoO;Q5
-++,QuUX+=FoO){if(Q5!=Q4){QuUX[Q4]*=-FOOBAZ[Q4];}}}}}if(*q2!=
-0){*Q1=0.0;}else{for(Q4=FoO;Q4-->0;){q6=Q3[Q4];if(Q4!=q6){
-for(Q5=0,QuUX=bar;Q5<FoO;Q5++,QuUX+=FoO){fobaz=QuUX[Q4];QuUX
-[Q4]=QuUX[q6];QuUX[q6]=fobaz;}}}}}
-#undef baz
-
-void palSlaDmxm(double q0[3][3],double q1[3][3],double foo[3][3
-]){int bar,q2,q3;double q4,Q5[3][3];for(bar=0;bar<3;bar++){
-for(q2=0;q2<3;q2++){q4=0.0;for(q3=0;q3<3;q3++){q4+=q0[bar][
-q3]*q1[q3][q2];}Q5[bar][q2]=q4;}}for(q2=0;q2<3;q2++){for(bar
-=0;bar<3;bar++){foo[bar][q2]=Q5[bar][q2];}}}
-
-void palSlaDmxv(double FOO[3][3],double baR[3],double BAZ[3]){
-int Q0,FOBAR;double q1,Q2[3];for(FOBAR=0;FOBAR<3;FOBAR++){q1
-=0.0;for(Q0=0;Q0<3;Q0++){q1+=FOO[FOBAR][Q0]*baR[Q0];}Q2[
-FOBAR]=q1;}for(FOBAR=0;FOBAR<3;FOBAR++){BAZ[FOBAR]=Q2[FOBAR]
-;}}
-
-double palSlaDrange(double fOo){
- while( fOo < -DPI ) fOo += D2PI;
- while( fOo > DPI ) fOo -= D2PI;
- return fOo;
-}
-
-double palSlaDranrm(double FoO){double BAR;BAR=dmod(FoO,D2PI);
-return(BAR>=0.0)?BAR:BAR+D2PI;}
-
-double palSlaDsep(double FOO,double BAR,double baz,double q0){
-double fobar[3],fOobaR[3];palSlaDcs2c(FOO,BAR,fobar);palSlaDcs2c(
-baz,q0,fOobaR);return palSlaDsepv(fobar,fOobaR);}
-
-double palSlaDsepv(double foo[3],double Q0[3]){double BAR[3],q1
-[3],BAZ,fObaR;palSlaDvxv(foo,Q0,BAR);palSlaDvn(BAR,q1,&BAZ);fObaR=
-palSlaDvdv(foo,Q0);return (BAZ!=0.0||fObaR!=0.0)?atan2(BAZ,fObaR):0.0;}
-
-void palSlaDtf2d(int q0,int foo,double q1,double*bar,int*Q2)
-#define q3 86400.0
-{*Q2=0;if((q1<0.0)||(q1>=60.0)){*Q2=3;return;}if((foo<0)||(
-foo>59)){*Q2=2;return;}if((q0<0)||(q0>23)){*Q2=1;return;}*
-bar=(60.0*(60.0*(double)q0+(double)foo)+q1)/q3;}
-#undef q3
-
-void palSlaDtf2r(int fOo,int BAR,double Baz,double*fobar,int*
-fOOBAr){double q0;palSlaDtf2d(fOo,BAR,Baz,&q0,fOOBAr);*fobar=
-D2PI*q0;}
-
-double palSlaDvdv(double q0[3],double q1[3]){return q0[0]*q1[0]
-+q0[1]*q1[1]+q0[2]*q1[2];}
-
-void palSlaDvn(double fOo[3],double baR[3],double*BAZ){int
-FOBAR;double fOOBAr,q0;fOOBAr=0.0;for(FOBAR=0;FOBAR<3;FOBAR
-++){q0=fOo[FOBAR];fOOBAr+=q0*q0;}fOOBAr=sqrt(fOOBAr);*BAZ=
-fOOBAr;fOOBAr=(fOOBAr>0.0)?fOOBAr:1.0;for(FOBAR=0;FOBAR<3;
-FOBAR++){baR[FOBAR]=fOo[FOBAR]/fOOBAr;}}
-
-void palSlaDvxv(double FOO[3],double Q0[3],double q1[3]){double
- q2[3];int BAR;q2[0]=FOO[1]*Q0[2]-FOO[2]*Q0[1];q2[1]=FOO[2]*
-Q0[0]-FOO[0]*Q0[2];q2[2]=FOO[0]*Q0[1]-FOO[1]*Q0[0];for(BAR=0
-;BAR<3;BAR++){q1[BAR]=q2[BAR];}}
-
-void palSlaEcmat(double foo,double Q0[3][3]){double bar,q1;bar=
-(foo-51544.5)/36525.0;q1=DAS2R*(84381.448+(-46.8150+(-
-0.00059+0.001813*bar)*bar)*bar);palSlaDeuler("\130",q1,0.0,0.0,
-Q0);}
-
-double palSlaEpb2d(double Q0){return 15019.81352+(Q0-1900.0)*
-365.242198781;}
-
-double palSlaEpb(double FOO){return 1900.0+(FOO-15019.81352)/
-365.242198781;}
-
-double palSlaEpj2d(double foo){return 51544.5+(foo-2000.0)*
-365.25;}
-
-double palSlaEpj(double foo){return 2000.0+(foo-51544.5)/365.25
-;}
-
-double palSlaEqeqx(double q0)
-#define Q1 1296000.0
-#define FOO 0.4848136811095359949E-5
-{double bar,q2,Q3,q4,Baz;bar=(q0-51544.5)/36525.0;q2=FOO*(
-450160.280+(-5.0*Q1-482890.539+(7.455+0.008*bar)*bar)*bar);
-palSlaNutc(q0,&Q3,&q4,&Baz);return Q3*cos(Baz)+FOO*(0.00264*sin
-(q2)+0.000063*sin(q2+q2));}
-#undef Q1
-#undef FOO
-
-void palSlaEqgal(double FOO,double bar,double*Baz,double*Q0){ double
-fobar[3],Q1[3]; static double FOOBAR[3][3] = { {-0.054875539726,
--0.873437108010, -0.483834985808}, {0.494109453312, -0.444829589425,
-0.746982251810}, {-0.867666135858, -0.198076386122, 0.455983795705}};
-palSlaDcs2c(FOO,bar,fobar);palSlaDmxv(FOOBAR,fobar,
-Q1);palSlaDcc2s(Q1,Baz,Q0);*Baz=palSlaDranrm(*Baz);*Q0=palSlaDrange(*
-Q0);}
-
-void palSlaEtrms(double FOO,double Q0[3]){double Q1,bar,q2,baz,
-FOBAR,FOobaR;Q1=(FOO-1950.0)*1.00002135903e-2;bar=0.01673011
--(0.00004193+0.000000126*Q1)*Q1;q2=(84404.836-(46.8495+(
-0.00319+0.00181*Q1)*Q1)*Q1)*DAS2R;baz=(1015489.951+(6190.67+
-(1.65+0.012*Q1)*Q1)*Q1)*DAS2R;FOBAR=bar*20.49552*DAS2R;
-FOobaR=cos(baz);Q0[0]=FOBAR*sin(baz);Q0[1]=-FOBAR*FOobaR*cos
-(q2);Q0[2]=-FOBAR*FOobaR*sin(q2);}
-
-void palSlaEvp(double q0,double FOo,double Q1[3],double bAr[3],
-double Q2[3],double BAZ[3]){int Q3,fobar,Q4,FOOBAR;double
-fobaz,FOOBAZ,q5,Q6,quux,fred,Q7,Q8,dog,CAT,q9,Q10,FISH,Q11,
-q12,GASP,Q13,Q14,Q15,BAD,q16,BUG,Q17,silly,buggY,Q18,q19,q20
-,MUM,DAD;double Q21,q22,DISK,q23,EMPTY,FULL,fast,q24,smALL,
-BIG,q25,Ok,Q26,q27,HELLO,bye,mAGIc,oBScuRe,Q28,Q29,SpeEd,Q30
-,indEx,bar_fOO,BAR_BAR,bar_baz,Q31,Q32,q33,q34,Q35,Q36,
-bar_fobar,q37,bar_foobar,BAR_FOBAZ,bar_foobaz;double
-BAR_QUUX[4],BAR_FRED[7],Q38[17],bar_dog[4],q39[4];double q40
-[3][3],q41,bar_cAt[3];static double BAr_FISh=1.990987e-7;
-static double q42=1.990969e-7;static double bar_gASp=
-3.122140e-5;static double Q43=2.661699e-6;static double q44=
-2.399485e-7;static double BaR_bAD=1949.9997904423;static
-double baR_BUG[4]={8.326827e-11,1.843484e-11,1.988712e-12,
-1.881276e-12};static double BAR_SILLY=0.99999696;static
-double q45[4]={4.960906e-3,2.727436e-3,8.392311e-4,
-1.556861e-3};static double BAr_BUggY=8.978749e-2;static
-double Q46[3][8]={{1.7400353,6.2565836,4.7199666,
-1.9636505e-1,4.1547339,4.6524223,4.2620486,1.4740694},{
-6.2833195099091e+2,6.2830194572674e+2,8.3997091449254e+3,
-8.4334662911720e+3,5.2993466764997e+1,2.1354275911213e+1,
-7.5025342197656,3.8377331909193},{5.2796e-6,-2.6180e-6,-
-1.9780e-5,-5.6044e-5,5.8845e-6,5.6797e-6,5.5317e-6,5.6093e-6
-}};static double Q47[3]={4.093198e-1,-2.271110e-4,-
-2.860401e-8};static double q48[3][17]={{1.675104e-2,
-2.220221e-1,1.589963,2.994089,8.155457e-1,1.735614,1.968564,
-1.282417,2.280820,4.833473e-2,5.589232e-2,4.634443e-2,
-8.997041e-3,2.284178e-2,4.350267e-2,1.348204e-2,3.106570e-2}
-,{-4.179579e-5,2.809917e-2,3.418075e-2,2.590824e-2,
-2.486352e-2,1.763719e-2,1.524020e-2,8.703393e-3,1.918010e-2,
-1.641773e-4,-3.455092e-4,-2.658234e-5,6.329728e-6,-
-9.941590e-5,-6.839749e-5,1.091504e-5,-1.665665e-4},{-
-1.260516e-7,1.852532e-5,1.430200e-5,4.155840e-6,6.836840e-6,
-6.370440e-6,-2.517152e-6,2.289292e-5,4.484520e-6,-
-4.654200e-7,-7.388560e-7,7.757000e-8,-1.939256e-9,
-6.787400e-8,-2.714956e-7,6.903760e-7,-1.590188e-7}};static
-double Q49[2][15]={{5.0974222,3.9584962,1.6338070,2.5487111,
-4.9255514,1.3363463,1.6072053,1.3629480,5.5657014,5.0708205,
-3.9318944,4.8989497,1.3097446,3.5147141,3.5413158},{-
-7.8604195454652e+2,-5.7533848094674e+2,-1.1506769618935e+3,-
-3.9302097727326e+2,-5.8849265665348e+2,-5.5076098609303e+2,-
-5.2237501616674e+2,-1.1790629318198e+3,-1.0977134971135e+3,-
-1.5774000881978e+2,5.2963464780000e+1,3.9809289073258e+1,
-7.7540959633708e+1,7.9618578146517e+1,-5.4868336758022e+2}};
-static double Q50[5][15]={{-2.279594e-5,-3.494537e-5,
-6.593466e-7,1.140767e-5,9.516893e-6,7.310990e-6,-2.603449e-6
-,-3.228859e-6,3.442177e-7,8.702406e-6,-1.488378e-6,-
-8.043059e-6,3.699128e-6,2.550120e-6,-6.351059e-7},{
-1.407414e-5,2.860401e-7,1.322572e-5,-2.049792e-5,-
-2.748894e-6,-1.924710e-6,7.359472e-6,1.308997e-7,2.671323e-6
-,-8.421214e-6,-1.251789e-5,-2.991300e-6,-3.316126e-6,-
-1.241123e-6,2.341650e-6},{8.273188e-6,1.289448e-7,
-9.258695e-6,-4.747930e-6,-1.319381e-6,-8.772849e-7,
-3.168357e-6,1.013137e-7,1.832858e-6,-1.372341e-6,5.226868e-7
-,1.473654e-7,2.901257e-7,9.901116e-8,1.061492e-6},{
-1.340565e-5,1.627237e-5,-4.674248e-7,-2.638763e-6,-
-4.549908e-6,-3.334143e-6,1.119056e-6,2.403899e-6,-
-2.394688e-7,-1.455234e-6,-2.049301e-7,-3.154542e-7,
-3.407826e-7,2.210482e-7,2.878231e-7},{-2.490817e-7,-
-1.823138e-7,-3.646275e-7,-1.245408e-7,-1.864821e-7,-
-1.745256e-7,-1.655307e-7,-3.736225e-7,-3.478444e-7,-
-4.998479e-8,0.0,0.0,0.0,0.0,0.0}};static double q51=-
-7.757020e-8;static double Q52[3][4]={{1.289600e-6,
-3.102810e-5,9.124190e-6,9.793240e-7},{5.550147e-1,4.035027,
-9.990265e-1,5.508259},{2.076942,3.525565e-1,2.622706,
-1.559103e+1}};static double Q53[2][3]={{5.167983,5.491315,
-5.959853},{8.3286911095275e+3,-7.2140632838100e+3,
-1.5542754389685e+4}};static double Q54[4][3]={{1.097594e-1,-
-2.223581e-2,1.148966e-2},{2.896773e-7,5.083103e-8,
-5.658888e-8},{5.450474e-2,1.002548e-2,8.249439e-3},{
-1.438491e-7,-2.291823e-8,4.063015e-8}};DISK=0.0;Q3=(FOo<=0.0)?0:1;Q21
-=(q0-15019.5)/36525.0;for(FOOBAR=0;FOOBAR<8;FOOBAR++){q22=
-dmod(Q46[0][FOOBAR]+Q21*(Q46[1][FOOBAR]+Q21*Q46[2][FOOBAR]),
-D2PI);if(FOOBAR==0){DISK=q22;}else{BAR_FRED[FOOBAR-1]=q22;}}
-q23=dmod(Q47[0]+Q21*(Q47[1]+Q21*Q47[2]),D2PI);for(FOOBAR=0;
-FOOBAR<17;FOOBAR++){Q38[FOOBAR]=dmod(q48[0][FOOBAR]+Q21*(q48
-[1][FOOBAR]+Q21*q48[2][FOOBAR]),D2PI);}for(FOOBAR=0;FOOBAR<4
-;FOOBAR++){fobaz=dmod(Q52[1][FOOBAR]+Q21*Q52[2][FOOBAR],D2PI
-);BAR_QUUX[FOOBAR]=sin(fobaz);}FOOBAZ=Q52[0][0]*BAR_QUUX[0]+
-Q52[0][1]*BAR_QUUX[1]+(Q52[0][2]+Q21*q51)*BAR_QUUX[2]+Q52[0]
-[3]*BAR_QUUX[3];q5=0.0;Q6=0.0;quux=0.0;for(FOOBAR=0;FOOBAR<
-15;FOOBAR++){fobaz=dmod(Q49[0][FOOBAR]+Q21*Q49[1][FOOBAR],
-D2PI);fred=cos(fobaz);Q7=sin(fobaz);FOOBAZ+=Q50[0][FOOBAR]*
-fred+Q50[1][FOOBAR]*Q7;Q6+=Q50[2][FOOBAR]*fred+Q50[3][FOOBAR
-]*Q7;if(FOOBAR<10){q5+=(Q50[1][FOOBAR]*fred-Q50[0][FOOBAR]*
-Q7)*Q50[4][FOOBAR];quux+=(Q50[3][FOOBAR]*fred-Q50[2][FOOBAR]
-*Q7)*Q50[4][FOOBAR];}}Q8=Q38[0];dog=Q8+Q8;CAT=Q8*Q8;EMPTY=
-1.0-CAT;q9=BAR_FRED[0];Q10=q9+q9;FISH=dog*((1.0-CAT/8.0)*sin
-(q9)+5.0*Q8*sin(Q10)/8.0+13.0*CAT*sin(q9+Q10)/24.0);Q11=
-BAR_FRED[0]+FISH;q12=sin(Q11);GASP=cos(Q11);FULL=EMPTY/(1.0+
-Q8*GASP);Q13=dog*q42*((1.0+CAT*1.5)*GASP+Q8*(1.25-q12*q12/
-2.0));Q14=q42*Q8*q12/sqrt(EMPTY);fast=1.0+Q6;q24=fast*(Q14+
-FULL*quux);smALL=fast*FULL*(BAr_FISh+Q13+q5);BIG=dmod(DISK+
-FISH+FOOBAZ,D2PI);q25=sin(BIG);Ok=cos(BIG);Q26=q24*Ok-smALL*
-q25;q27=q24*q25+smALL*Ok;FOOBAZ=0.0;q5=0.0;Q15=0.0;BAD=0.0;
-for(FOOBAR=0;FOOBAR<3;FOOBAR++){fobaz=dmod(Q53[0][FOOBAR]+
-Q21*Q53[1][FOOBAR],D2PI);Q7=sin(fobaz);fred=cos(fobaz);
-FOOBAZ+=Q54[0][FOOBAR]*Q7;q5+=Q54[1][FOOBAR]*fred;Q15+=Q54[2
-][FOOBAR]*fred;BAD+=-Q54[3][FOOBAR]*Q7;}q16=BAR_FRED[1]+
-FOOBAZ;BUG=sin(q16);Q17=cos(q16);silly=bar_gASp/(1.0+Q15);
-fobaz=silly*(Q43+q5);buggY=silly*BAD;Q26+=fobaz*BUG+buggY*
-Q17;q27+=-fobaz*Q17+buggY*BUG;HELLO=-silly*q44*cos(BAR_FRED[
-2]);bye=Q26*BAR_SILLY;mAGIc=q27*BAR_SILLY;oBScuRe=HELLO*
-BAR_SILLY;for(FOOBAR=0;FOOBAR<4;FOOBAR++){Q18=BAR_FRED[
-FOOBAR+3];q19=Q38[FOOBAR+1];q20=Q38[FOOBAR+9];q16=dmod(Q18+
-2.0*q20*sin(Q18-q19),D2PI);bar_dog[FOOBAR]=sin(q16);q39[
-FOOBAR]=cos(q16);bye+=baR_BUG[FOOBAR]*(bar_dog[FOOBAR]+q20*
-sin(q19));mAGIc+=-baR_BUG[FOOBAR]*(q39[FOOBAR]+q20*cos(q19))
-;oBScuRe+=-baR_BUG[FOOBAR]*Q38[FOOBAR+13]*cos(Q18-Q38[FOOBAR
-+5]);}Q28=cos(q23);Q29=sin(q23);SpeEd=Q28*q27-Q29*HELLO;Q30=
-Q29*q27+Q28*HELLO;indEx=Q28*mAGIc-Q29*oBScuRe;bar_fOO=Q29*
-mAGIc+Q28*oBScuRe;BAR_BAR=FULL*fast;MUM=BAr_BUggY*sin(
-BAR_FRED[2]);fobaz=silly*cos(MUM);bar_baz=BAR_BAR*Ok-fobaz*
-Q17;Q31=BAR_BAR*q25-fobaz*BUG;Q32=-silly*sin(MUM);q33=
-bar_baz*BAR_SILLY;q34=Q31*BAR_SILLY;Q35=Q32*BAR_SILLY;for(
-FOOBAR=0;FOOBAR<4;FOOBAR++){DAD=Q38[FOOBAR+13]*sin(BAR_FRED[
-FOOBAR+3]-Q38[FOOBAR+5]);fobaz=q45[FOOBAR]*(1.0-Q38[FOOBAR+9
-]*cos(BAR_FRED[FOOBAR+3]-Q38[FOOBAR+1]));buggY=fobaz*cos(DAD
-);q33-=buggY*q39[FOOBAR];q34-=buggY*bar_dog[FOOBAR];Q35-=
-fobaz*sin(DAD);}Q36=Q28*Q31-Q29*Q32;bar_fobar=Q29*Q31+Q28*
-Q32;q37=Q28*q34-Q29*Q35;bar_foobar=Q29*q34+Q28*Q35;BAR_FOBAZ
-=palSlaEpj(q0);bar_foobaz=DS2R*(0.035+(0.00085*(BAR_FOBAZ-
-BaR_bAD)));Q2[0]=Q26-bar_foobaz*SpeEd;Q2[1]=SpeEd+bar_foobaz
-*Q26;Q2[2]=Q30;Q1[0]=bye-bar_foobaz*indEx;Q1[1]=indEx+
-bar_foobaz*bye;Q1[2]=bar_fOO;BAZ[0]=bar_baz-bar_foobaz*Q36;
-BAZ[1]=Q36+bar_foobaz*bar_baz;BAZ[2]=bar_fobar;bAr[0]=q33-
-bar_foobaz*q37;bAr[1]=q37+bar_foobaz*q33;bAr[2]=bar_foobar;
-if(Q3!=0){palSlaPrec(BAR_FOBAZ,FOo,q40);for(Q4=0;Q4<3;Q4++){q41
-=0.0;for(fobar=0;fobar<3;fobar++){q41+=q40[Q4][fobar]*Q2[
-fobar];}bar_cAt[Q4]=q41;}for(Q4=0;Q4<3;Q4++){Q2[Q4]=bar_cAt[
-Q4];}for(Q4=0;Q4<3;Q4++){q41=0.0;for(fobar=0;fobar<3;fobar++
-){q41+=q40[Q4][fobar]*Q1[fobar];}bar_cAt[Q4]=q41;}for(Q4=0;
-Q4<3;Q4++){Q1[Q4]=bar_cAt[Q4];}for(Q4=0;Q4<3;Q4++){q41=0.0;
-for(fobar=0;fobar<3;fobar++){q41+=q40[Q4][fobar]*BAZ[fobar];
-}bar_cAt[Q4]=q41;}for(Q4=0;Q4<3;Q4++){BAZ[Q4]=bar_cAt[Q4];}
-for(Q4=0;Q4<3;Q4++){q41=0.0;for(fobar=0;fobar<3;fobar++){q41
-+=q40[Q4][fobar]*bAr[fobar];}bar_cAt[Q4]=q41;}for(Q4=0;Q4<3;
-Q4++){bAr[Q4]=bar_cAt[Q4];}}}
-
-void palSlaFk425(double FoO,double BAR,double Q0,double Q1,
-double Baz,double q2,double*FobAr,double*Q3,double*q4,double
-*q5,double*FOOBAR,double*FObaz){double foobaz,QUux,q6,FrEd,
-doG,q7,Q8,Q9,CAT,Q10,fiSH,q11,gasp,q12,q13,BAd,Q14,q15,BuG,
-Q16,silly,q17,buggy,Q18;int q19,MUm;double dAD[3],q20[3];
-double disk[6],q21[6];static double empty=100.0*60.0*60.0*
-360.0/D2PI;double Q22=1.0e-30;double FULL=21.095;static
-double q23[3]={-1.62557e-6,-0.31919e-6,-0.13843e-6};static
-double FAST[3]={1.245e-3,-1.580e-3,-0.659e-3};static double
-SMALL[6][6]={{0.9999256782,-0.0111820611,-0.0048579477,
-0.00000242395018,-0.00000002710663,-0.00000001177656},{
-0.0111820610,0.9999374784,-0.0000271765,0.00000002710663,
-0.00000242397878,-0.00000000006587},{0.0048579479,-
-0.0000271474,0.9999881997,0.00000001177656,-0.00000000006582
-,0.00000242410173},{-0.000551,-0.238565,0.435739,0.99994704,
--0.01118251,-0.00485767},{0.238514,-0.002667,-0.008541,
-0.01118251,0.99995883,-0.00002718},{-0.435623,0.012254,
-0.002117,0.00485767,-0.00002714,1.00000956}};foobaz=FoO;QUux
-=BAR;q6=Q0*empty;FrEd=Q1*empty;doG=Baz;q7=q2;Q8=sin(foobaz);
-Q9=cos(foobaz);CAT=sin(QUux);Q10=cos(QUux);dAD[0]=Q9*Q10;dAD
-[1]=Q8*Q10;dAD[2]=CAT;fiSH=FULL*q7*doG;q20[0]=(-Q8*Q10*q6)-(
-Q9*CAT*FrEd)+(fiSH*dAD[0]);q20[1]=(Q9*Q10*q6)-(Q8*CAT*FrEd)+
-(fiSH*dAD[1]);q20[2]=(Q10*FrEd)+(fiSH*dAD[2]);fiSH=(dAD[0]*
-q23[0])+(dAD[1]*q23[1])+(dAD[2]*q23[2]);q11=(dAD[0]*FAST[0])
-+(dAD[1]*FAST[1])+(dAD[2]*FAST[2]);for(q19=0;q19<3;q19++){
-disk[q19]=dAD[q19]-q23[q19]+fiSH*dAD[q19];disk[q19+3]=q20[
-q19]-FAST[q19]+q11*dAD[q19];}for(q19=0;q19<6;q19++){fiSH=0.0
-;for(MUm=0;MUm<6;MUm++){fiSH+=SMALL[q19][MUm]*disk[MUm];}q21
-[q19]=fiSH;}gasp=q21[0];q12=q21[1];q13=q21[2];BAd=q21[3];Q14
-=q21[4];q15=q21[5];BuG=(gasp*gasp)+(q12*q12);Q16=(BuG)+(q13*
-q13);silly=sqrt(BuG);q17=sqrt(Q16);buggy=(gasp*BAd)+(q12*Q14
-);Q18=buggy+(q13*q15);foobaz=(gasp!=0.0||q12!=0.0)?atan2(q12
-,gasp):0.0;if(foobaz<0.0)foobaz+=D2PI;QUux=atan2(q13,silly);
-if(silly>Q22){q6=((gasp*Q14)-(q12*BAd))/BuG;FrEd=((q15*BuG)-
-(q13*buggy))/(Q16*silly);}if(doG>Q22){q7=Q18/(doG*q17*FULL);
-doG=doG/q17;}*FobAr=foobaz;*Q3=QUux;*q4=q6/empty;*q5=FrEd/
-empty;*FObaz=q7;*FOOBAR=doG;}
-
-void palSlaFk45z(double Q0,double FOO,double q1,double*q2,
-double*Q3){double q4;int q5,bar;double Q6[3],baz[3],Q7[3],Q8
-[6];static double fobar=100.0*60.0*60.0*360.0/D2PI;static
-double foobar[3]={-1.62557e-6,-0.31919e-6,-0.13843e-6};
-static double FOBAZ[3]={1.245e-3,-1.580e-3,-0.659e-3};static
- double Q9[6][3]={{0.9999256782,-0.0111820611,-0.0048579477}
-,{0.0111820610,0.9999374784,-0.0000271765},{0.0048579479,-
-0.0000271474,0.9999881997},{-0.000551,-0.238565,0.435739},{
-0.238514,-0.002667,-0.008541},{-0.435623,0.012254,0.002117}}
-;palSlaDcs2c(Q0,FOO,Q6);q4=(q1-1950.0)/fobar;for(q5=0;q5<3;q5++
-){baz[q5]=foobar[q5]+q4*FOBAZ[q5];}q4=Q6[0]*baz[0]+Q6[1]*baz
-[1]+Q6[2]*baz[2];for(q5=0;q5<3;q5++){Q7[q5]=Q6[q5]-baz[q5]+
-q4*Q6[q5];}for(q5=0;q5<6;q5++){q4=0.0;for(bar=0;bar<3;bar++)
-{q4+=Q9[q5][bar]*Q7[bar];}Q8[q5]=q4;}q4=(palSlaEpj(palSlaEpb2d(q1)
-)-2000.0)/fobar;for(q5=0;q5<3;q5++){Q8[q5]+=q4*Q8[q5+3];}
-palSlaDcc2s(Q8,&q4,Q3);*q2=palSlaDranrm(q4);}
-
-void palSlaFk524(double Q0,double foo,double q1,double BAR,
-double BAZ,double Q2,double*q3,double*Q4,double*fobar,double
-*q5,double*Q6,double*foobar){double fOBAZ,q7,foobaz,q8,QUUX,
-Q9;double q10,Q11,Q12,fred,q13,Q14,q15,q16;double q17[6],Q18
-[6];double DOG,Q19,caT;double q20,fish,GASP,q21;int BAD,BUG;
-static double Q22=100.0*60.0*60.0*360.0/D2PI;static double
-Q23=1.0e-30;static double Q24=21.095;static double silLY[6]=
-{-1.62557e-6,-0.31919e-6,-0.13843e-6,1.245e-3,-1.580e-3,-
-0.659e-3};static double buggy[6][6]={{0.9999256795,
-0.0111814828,0.0048590039,-0.00000242389840,-
-0.00000002710544,-0.00000001177742},{-0.0111814828,
-0.9999374849,-0.0000271771,0.00000002710544,-
-0.00000242392702,0.00000000006585},{-0.0048590040,-
-0.0000271557,0.9999881946,0.00000001177742,0.00000000006585,
--0.00000242404995},{-0.000551,0.238509,-0.435614,0.99990432,
-0.01118145,0.00485852},{-0.238560,-0.002667,0.012254,-
-0.01118145,0.99991613,-0.00002717},{0.435730,-0.008541,
-0.002117,-0.00485852,-0.00002716,0.99996684}};fOBAZ=Q0;q7=
-foo;foobaz=q1*Q22;q8=BAR*Q22;QUUX=BAZ;Q9=Q2;q10=sin(fOBAZ);
-Q11=cos(fOBAZ);Q12=sin(q7);fred=cos(q7);q13=Q11*fred;Q14=q10
-*fred;q15=Q12;q16=Q24*Q9*QUUX;q17[0]=q13;q17[1]=Q14;q17[2]=
-q15;q17[3]=-foobaz*Q14-Q11*Q12*q8+q16*q13;q17[4]=foobaz*q13-
-q10*Q12*q8+q16*Q14;q17[5]=fred*q8+q16*q15;for(BAD=0;BAD<6;
-BAD++){q16=0.0;for(BUG=0;BUG<6;BUG++){q16+=buggy[BAD][BUG]*
-q17[BUG];}Q18[BAD]=q16;}q13=Q18[0];Q14=Q18[1];q15=Q18[2];q20
-=sqrt(q13*q13+Q14*Q14+q15*q15);q16=q13*silLY[0]+Q14*silLY[1]
-+q15*silLY[2];q13+=silLY[0]*q20-q16*q13;Q14+=silLY[1]*q20-
-q16*Q14;q15+=silLY[2]*q20-q16*q15;q20=sqrt(q13*q13+Q14*Q14+
-q15*q15);q13=Q18[0];Q14=Q18[1];q15=Q18[2];q16=q13*silLY[0]+
-Q14*silLY[1]+q15*silLY[2];fish=q13*silLY[3]+Q14*silLY[4]+q15
-*silLY[5];q13+=silLY[0]*q20-q16*q13;Q14+=silLY[1]*q20-q16*
-Q14;q15+=silLY[2]*q20-q16*q15;DOG=Q18[3]+silLY[3]*q20-fish*
-q13;Q19=Q18[4]+silLY[4]*q20-fish*Q14;caT=Q18[5]+silLY[5]*q20
--fish*q15;GASP=q13*q13+Q14*Q14;q21=sqrt(GASP);fOBAZ=(q13!=
-0.0||Q14!=0.0)?atan2(Q14,q13):0.0;if(fOBAZ<0.0)fOBAZ+=D2PI;
-q7=atan2(q15,q21);if(q21>Q23){foobaz=(q13*Q19-Q14*DOG)/GASP;
-q8=(caT*GASP-q15*(q13*DOG+Q14*Q19))/((GASP+q15*q15)*q21);}if
-(QUUX>Q23){Q9=(q13*DOG+Q14*Q19+q15*caT)/(QUUX*Q24*q20);QUUX=
-QUUX/q20;}*q3=fOBAZ;*Q4=q7;*fobar=foobaz/Q22;*q5=q8/Q22;*
-foobar=Q9;*Q6=QUUX;}
-
-void palSlaFk54z(double foo,double baR,double Baz,double*fobar,
-double*fOOBAr,double*Q0,double*FOBAZ){static double FOOBAZ=
-0.0;double Q1,QuuX,Q2,FRED;palSlaFk524(foo,baR,FOOBAZ,FOOBAZ,
-FOOBAZ,FOOBAZ,&Q1,&QuuX,Q0,FOBAZ,&Q2,&FRED);palSlaPm(Q1,QuuX,*
-Q0,*FOBAZ,FOOBAZ,FOOBAZ,1950.0,Baz,fobar,fOOBAr);}
-
-void palSlaFk5hz(double foo,double Q0,double q1,double*BAR,
-double*q2)
-#define BAZ 0.484813681109535994e-5
-{static double FOBAR[3]={-19.9e-3*BAZ,-9.1e-3*BAZ,22.9e-3*
-BAZ},FOobaR[3]={-0.30e-3*BAZ,0.60e-3*BAZ,0.70e-3*BAZ};double
- q3[3],fobaz[3][3],FOOBAZ,q4[3],QUUX[3][3],FRED[3],dog[3],Q5
-;int Cat;palSlaDcs2c(foo,Q0,q3);palSlaDav2m(FOBAR,fobaz);FOOBAZ=
-2000.0-q1;for(Cat=0;Cat<3;Cat++){q4[Cat]=FOobaR[Cat]*FOOBAZ;
-}palSlaDav2m(q4,QUUX);palSlaDimxv(QUUX,q3,FRED);palSlaDmxv(fobaz,FRED
-,dog);palSlaDcc2s(dog,&Q5,q2);*BAR=palSlaDranrm(Q5);}
-#undef BAZ
-
-void palSlaGaleq(double q0,double q1,double*foO,double*bAR){
-double Q2[3],baz[3];static double Q3[3][3]={{-0.054875539726
-,-0.873437108010,-0.483834985808},{0.494109453312,-
-0.444829589425,0.746982251810},{-0.867666135858,-
-0.198076386122,0.455983795705}};palSlaDcs2c(q0,q1,Q2);palSlaDimxv(
-Q3,Q2,baz);palSlaDcc2s(baz,foO,bAR);*foO=palSlaDranrm(*foO);*bAR=
-palSlaDrange(*bAR);}
-
-void palSlaGalsup(double fOo,double bar,double*baz,double*Q0){
-double FobaR[3],Q1[3];static double Q2[3][3]={{-
-0.735742574804,0.677261296414,0.0},{-0.074553778365,-
-0.080991471307,0.993922590400},{0.673145302109,
-0.731271165817,0.110081262225}};palSlaDcs2c(fOo,bar,FobaR);
-palSlaDmxv(Q2,FobaR,Q1);palSlaDcc2s(Q1,baz,Q0);*baz=palSlaDranrm(*baz
-);*Q0=palSlaDrange(*Q0);}
-
-void palSlaGeoc(double Q0,double Q1,double*FOO,double*Q2){
-double q3,q4,q5,q6;static double q7=6378140.0;static double
-bar=1.0/298.257;double q8=(1.0-bar)*(1.0-bar);static double
-BAZ=1.49597870e11;q3=sin(Q0);q4=cos(Q0);q5=1.0/sqrt(q4*q4+q8
-*q3*q3);q6=q8*q5;*FOO=(q7*q5+Q1)*q4/BAZ;*Q2=(q7*q6+Q1)*q3/
-BAZ;}
-
-double palSlaGmst(double Q0){double FOo;FOo=(Q0-51544.5)/
-36525.0;return palSlaDranrm(dmod(Q0,1.0)*D2PI+(24110.54841+(
-8640184.812866+(0.093104-6.2e-6*FOo)*FOo)*FOo)*DS2R);}
-
-void palSlaHfk5z(double q0,double q1,double FoO,double*BAR,
-double*q2,double*Q3,double*baZ)
-#define Q4 0.484813681109535994e-5
-{static double FOBAR[3]={-19.9e-3*Q4,-9.1e-3*Q4,22.9e-3*Q4},
-fOOBAR[3]={-0.30e-3*Q4,0.60e-3*Q4,0.70e-3*Q4};double q5[3],
-FoBAZ[3][3],Q6[3],q7,FOOBAZ[3],Q8[3][3],qUUx[3][3],Q9[6],q10
-[3],Q11,Q12,q13;int freD;palSlaDcs2c(q0,q1,q5);palSlaDav2m(FOBAR,
-FoBAZ);palSlaDmxv(FoBAZ,fOOBAR,Q6);q7=FoO-2000.0;for(freD=0;
-freD<3;freD++){FOOBAZ[freD]=fOOBAR[freD]*q7;}palSlaDav2m(FOOBAZ
-,Q8);palSlaDmxm(FoBAZ,Q8,qUUx);palSlaDimxv(qUUx,q5,Q9);palSlaDvxv(Q6,
-q5,q10);palSlaDimxv(qUUx,q10,Q9+3);palSlaDc62s(Q9,&Q11,q2,&Q12,Q3,
-baZ,&q13);*BAR=palSlaDranrm(Q11);}
-#undef Q4
-
-void palSlaMappa(double q0,double q1,double foo[21])
-#define Q2 499.004782
-#define Q3 1.974126e-8
-{int Q4;double BAR[3],q5[3],Q6[3],baz,Q7[3],q8;foo[0]=palSlaEpj
-(q1)-q0;palSlaEvp(q1,q0,BAR,&foo[1],q5,Q6);palSlaDvn(Q6,&foo[4],&
-baz);foo[7]=Q3/baz;for(Q4=0;Q4<3;Q4++){foo[Q4+8]=BAR[Q4]*Q2;
-}palSlaDvn(&foo[8],Q7,&q8);foo[11]=sqrt(1.0-q8*q8);palSlaPrenut(q0
-,q1,(double(*)[3])&foo[12]);}
-#undef Q2
-#undef Q3
-
-void palSlaMapqkz(double FOO,double Q0,double bar[21],double*q1
-,double*BAZ){int fObaR;double Q2,FOobAr,Q3[3],Q4[3],Q5[3],q6
-,fobaz,FOOBAZ,q7[3],QuUX,q8,frED[3],dog[3];Q2=bar[7];FOobAr=
-bar[11];for(fObaR=0;fObaR<3;fObaR++){Q3[fObaR]=bar[fObaR+4];
-Q4[fObaR]=bar[fObaR+8];}palSlaDcs2c(FOO,Q0,Q5);q6=palSlaDvdv(Q5,Q3
-);fobaz=q6+1.0;FOOBAZ=Q2/gmax(fobaz,1e-5);for(fObaR=0;fObaR<
-3;fObaR++){q7[fObaR]=Q5[fObaR]+FOOBAZ*(Q3[fObaR]-q6*Q5[fObaR
-]);}QuUX=palSlaDvdv(q7,Q4);q8=QuUX+1.0;FOOBAZ=1.0+QuUX/(FOobAr+
-1.0);for(fObaR=0;fObaR<3;fObaR++){frED[fObaR]=((FOobAr*q7[
-fObaR])+(FOOBAZ*Q4[fObaR]))/q8;}palSlaDmxv((double(*)[3])&bar[
-12],frED,dog);palSlaDcc2s(dog,q1,BAZ);*q1=palSlaDranrm(*q1);}
-
-void palSlaNut(double FoO,double bar[3][3]){double q0,Q1,baz;
-palSlaNutc(FoO,&q0,&Q1,&baz);palSlaDeuler("\170\172\170",baz,-q0,-
-(baz+Q1),bar);}
-
-void palSlaNutc(double Q0,double*foo,double*q1,double*Q2)
-#define q3 1296000.0
-#define Q4 51544.5
-#define q5 36525.0
-{static int q6[][9]={{0,0,0,0,-1,0,0,0,0},{0,0,2,-2,2,0,0,0,
-0},{0,0,2,0,2,0,0,0,0},{0,0,0,0,-2,0,0,0,0},{0,1,0,0,0,0,0,0
-,0},{0,1,2,-2,2,0,0,0,0},{1,0,0,0,0,0,0,0,0},{0,0,2,0,1,0,0,
-0,0},{1,0,2,0,2,0,0,0,0},{0,-1,2,-2,2,0,0,0,0},{0,0,2,-2,1,0
-,0,0,0},{-1,0,2,0,2,0,0,0,0},{-1,0,0,2,0,0,0,0,0},{1,0,0,0,1
-,0,0,0,0},{1,0,0,0,-1,0,0,0,0},{-1,0,2,2,2,0,0,0,0},{1,0,2,0
-,1,0,0,0,0},{-2,0,2,0,1,0,0,0,0},{0,0,0,2,0,0,0,0,0},{0,0,2,
-2,2,0,0,0,0},{2,0,0,-2,0,0,0,0,0},{2,0,2,0,2,0,0,0,0},{1,0,2
-,-2,2,0,0,0,0},{-1,0,2,0,1,0,0,0,0},{2,0,0,0,0,0,0,0,0},{0,0
-,2,0,0,0,0,0,0},{0,1,0,0,1,0,0,0,0},{-1,0,0,2,1,0,0,0,0},{0,
-2,2,-2,2,0,0,0,0},{0,0,2,-2,0,0,0,0,0},{-1,0,0,2,-1,0,0,0,0}
-,{0,1,0,0,-1,0,0,0,0},{0,2,0,0,0,0,0,0,0},{-1,0,2,2,1,0,0,0,
-0},{1,0,2,2,2,0,0,0,0},{0,1,2,0,2,0,0,0,0},{-2,0,2,0,0,0,0,0
-,0},{0,0,2,2,1,0,0,0,0},{0,-1,2,0,2,0,0,0,0},{0,0,0,2,1,0,0,
-0,0},{1,0,2,-2,1,0,0,0,0},{2,0,0,-2,-1,0,0,0,0},{2,0,2,-2,2,
-0,0,0,0},{2,0,2,0,1,0,0,0,0},{0,0,0,2,-1,0,0,0,0},{0,-1,2,-2
-,1,0,0,0,0},{-1,-1,0,2,0,0,0,0,0},{2,0,0,-2,1,0,0,0,0},{1,0,
-0,2,0,0,0,0,0},{0,1,2,-2,1,0,0,0,0},{1,-1,0,0,0,0,0,0,0},{-2
-,0,2,0,2,0,0,0,0},{0,-1,0,2,0,0,0,0,0},{3,0,2,0,2,0,0,0,0},{
-0,0,0,1,0,0,0,0,0},{1,-1,2,0,2,0,0,0,0},{1,0,0,-1,0,0,0,0,0}
-,{-1,-1,2,2,2,0,0,0,0},{-1,0,2,0,0,0,0,0,0},{2,0,0,0,-1,0,0,
-0,0},{0,-1,2,2,2,0,0,0,0},{1,1,2,0,2,0,0,0,0},{2,0,0,0,1,0,0
-,0,0},{1,1,0,0,0,0,0,0,0},{1,0,-2,2,-1,0,0,0,0},{1,0,2,0,0,0
-,0,0,0},{-1,1,0,1,0,0,0,0,0},{1,0,0,0,2,0,0,0,0},{-1,0,1,0,1
-,0,0,0,0},{0,0,2,1,2,0,0,0,0},{-1,1,0,1,1,0,0,0,0},{-1,0,2,4
-,2,0,0,0,0},{0,-2,2,-2,1,0,0,0,0},{1,0,2,2,1,0,0,0,0},{1,0,0
-,0,-2,0,0,0,0},{-2,0,2,2,2,0,0,0,0},{1,1,2,-2,2,0,0,0,0},{-2
-,0,2,4,2,0,0,0,0},{-1,0,4,0,2,0,0,0,0},{2,0,2,-2,1,0,0,0,0},
-{1,0,0,-1,-1,0,0,0,0},{2,0,2,2,2,0,0,0,0},{1,0,0,2,1,0,0,0,0
-},{3,0,0,0,0,0,0,0,0},{0,0,2,-2,-1,0,0,0,0},{3,0,2,-2,2,0,0,
-0,0},{0,0,4,-2,2,0,0,0,0},{-1,0,0,4,0,0,0,0,0},{0,1,2,0,1,0,
-0,0,0},{0,0,2,-2,3,0,0,0,0},{-2,0,0,4,0,0,0,0,0},{-1,-1,0,2,
-1,0,0,0,0},{-2,0,2,0,-1,0,0,0,0},{0,0,2,0,-1,0,0,0,0},{0,-1,
-2,0,1,0,0,0,0},{0,1,0,0,2,0,0,0,0},{0,0,2,-1,2,0,0,0,0},{2,1
-,0,-2,0,0,0,0,0},{0,0,2,4,2,0,0,0,0},{-1,-1,0,2,-1,0,0,0,0},
-{-1,1,0,2,0,0,0,0,0},{1,-1,0,0,1,0,0,0,0},{0,-1,2,-2,0,0,0,0
-,0},{0,1,0,0,-2,0,0,0,0},{1,-1,2,2,2,0,0,0,0},{1,0,0,2,-1,0,
-0,0,0},{-1,1,2,2,2,0,0,0,0},{3,0,2,0,1,0,0,0,0},{0,1,2,2,2,0
-,0,0,0},{1,0,2,-2,0,0,0,0,0},{-1,0,-2,4,-1,0,0,0,0},{-1,-1,2
-,2,1,0,0,0,0},{0,-1,2,2,1,0,0,0,0},{2,-1,2,0,2,0,0,0,0},{0,0
-,0,2,2,0,0,0,0},{1,-1,2,0,1,0,0,0,0},{-1,1,2,0,2,0,0,0,0},{0
-,1,0,2,0,0,0,0,0},{0,1,2,-2,0,0,0,0,0},{0,3,2,-2,2,0,0,0,0},
-{0,0,0,1,1,0,0,0,0},{-1,0,2,2,0,0,0,0,0},{2,1,2,0,2,0,0,0,0}
-,{1,1,0,0,1,0,0,0,0},{2,0,0,2,0,0,0,0,0},{1,1,2,0,1,0,0,0,0}
-,{-1,0,0,2,2,0,0,0,0},{1,0,-2,2,0,0,0,0,0},{0,-1,0,2,-1,0,0,
-0,0},{-1,0,1,0,2,0,0,0,0},{0,1,0,1,0,0,0,0,0},{1,0,-2,2,-2,0
-,0,0,0},{0,0,0,1,-1,0,0,0,0},{1,-1,0,0,-1,0,0,0,0},{0,0,0,4,
-0,0,0,0,0},{1,-1,0,2,0,0,0,0,0},{1,0,2,1,2,0,0,0,0},{1,0,2,-
-1,2,0,0,0,0},{-1,0,0,2,-2,0,0,0,0},{0,0,2,1,1,0,0,0,0},{-1,0
-,2,0,-1,0,0,0,0},{-1,0,2,4,1,0,0,0,0},{0,0,2,2,0,0,0,0,0},{1
-,1,2,-2,1,0,0,0,0},{0,0,1,0,1,0,0,0,0},{-1,0,2,-1,1,0,0,0,0}
-,{-2,0,2,2,1,0,0,0,0},{2,-1,0,0,0,0,0,0,0},{4,0,2,0,2,0,0,0,
-0},{2,1,2,-2,2,0,0,0,0},{0,1,2,1,2,0,0,0,0},{1,0,4,-2,2,0,0,
-0,0},{1,1,0,0,-1,0,0,0,0},{-2,0,2,4,1,0,0,0,0},{2,0,2,0,0,0,
-0,0,0},{-1,0,1,0,0,0,0,0,0},{1,0,0,1,0,0,0,0,0},{0,1,0,2,1,0
-,0,0,0},{-1,0,4,0,1,0,0,0,0},{-1,0,0,4,1,0,0,0,0},{2,0,2,2,1
-,0,0,0,0},{2,1,0,0,0,0,0,0,0},{0,0,5,-5,5,-3,0,0,0},{0,0,0,0
-,0,0,0,2,0},{0,0,1,-1,1,0,0,-1,0},{0,0,-1,1,-1,1,0,0,0},{0,0
-,-1,1,0,0,2,0,0},{0,0,3,-3,3,0,0,-1,0},{0,0,-8,8,-7,5,0,0,0}
-,{0,0,-1,1,-1,0,2,0,0},{0,0,-2,2,-2,2,0,0,0},{0,0,-6,6,-6,4,
-0,0,0},{0,0,-2,2,-2,0,8,-3,0},{0,0,6,-6,6,0,-8,3,0},{0,0,4,-
-4,4,-2,0,0,0},{0,0,-3,3,-3,2,0,0,0},{0,0,4,-4,3,0,-8,3,0},{0
-,0,-4,4,-5,0,8,-3,0},{0,0,0,0,0,2,0,0,0},{0,0,-4,4,-4,3,0,0,
-0},{0,1,-1,1,-1,0,0,1,0},{0,0,0,0,0,0,0,1,0},{0,0,1,-1,1,1,0
-,0,0},{0,0,2,-2,2,0,-2,0,0},{0,-1,-7,7,-7,5,0,0,0},{-2,0,2,0
-,2,0,0,-2,0},{-2,0,2,0,1,0,0,-3,0},{0,0,2,-2,2,0,0,-2,0},{0,
-0,1,-1,1,0,0,1,0},{0,0,0,0,0,0,0,0,2},{0,0,0,0,0,0,0,0,1},{2
-,0,-2,0,-2,0,0,3,0},{0,0,1,-1,1,0,0,-2,0},{0,0,-7,7,-7,5,0,0
-,0}};static double bar[][4]={{3341.5,17206241.8,3.1,17409.5}
-,{-1716.8,-1317185.3,1.4,-156.8},{285.7,-227667.0,0.3,-23.5}
-,{-68.6,-207448.0,0.0,-21.4},{950.3,147607.9,-2.3,-355.0},{-
-66.7,-51689.1,0.2,122.6},{-108.6,71117.6,0.0,7.0},{35.6,-
-38740.2,0.1,-36.2},{85.4,-30127.6,0.0,-3.1},{9.0,21583.0,0.1
-,-50.3},{22.1,12822.8,0.0,13.3},{3.4,12350.8,0.0,1.3},{-21.1
-,15699.4,0.0,1.6},{4.2,6313.8,0.0,6.2},{-22.8,5796.9,0.0,6.1
-},{15.7,-5961.1,0.0,-0.6},{13.1,-5159.1,0.0,-4.6},{1.8,
-4592.7,0.0,4.5},{-17.5,6336.0,0.0,0.7},{16.3,-3851.1,0.0,-
-0.4},{-2.8,4771.7,0.0,0.5},{13.8,-3099.3,0.0,-0.3},{0.2,
-2860.3,0.0,0.3},{1.4,2045.3,0.0,2.0},{-8.6,2922.6,0.0,0.3},{
--7.7,2587.9,0.0,0.2},{8.8,-1408.1,0.0,3.7},{1.4,1517.5,0.0,
-1.5},{-1.9,-1579.7,0.0,7.7},{1.3,-2178.6,0.0,-0.2},{-4.8,
-1286.8,0.0,1.3},{6.3,1267.2,0.0,-4.0},{-1.0,1669.3,0.0,-8.3}
-,{2.4,-1020.0,0.0,-0.9},{4.5,-766.9,0.0,0.0},{-1.1,756.5,0.0
-,-1.7},{-1.4,-1097.3,0.0,-0.5},{2.6,-663.0,0.0,-0.6},{0.8,-
-714.1,0.0,1.6},{0.4,-629.9,0.0,-0.6},{0.3,580.4,0.0,0.6},{-
-1.6,577.3,0.0,0.5},{-0.9,644.4,0.0,0.0},{2.2,-534.0,0.0,-0.5
-},{-2.5,493.3,0.0,0.5},{-0.1,-477.3,0.0,-2.4},{-0.9,735.0,
-0.0,-1.7},{0.7,406.2,0.0,0.4},{-2.8,656.9,0.0,0.0},{0.6,
-358.0,0.0,2.0},{-0.7,472.5,0.0,-1.1},{-0.1,-300.5,0.0,0.0},{
--1.2,435.1,0.0,-1.0},{1.8,-289.4,0.0,0.0},{0.6,-422.6,0.0,
-0.0},{0.8,-287.6,0.0,0.6},{-38.6,-392.3,0.0,0.0},{0.7,-281.8
-,0.0,0.6},{0.6,-405.7,0.0,0.0},{-1.2,229.0,0.0,0.2},{1.1,-
-264.3,0.0,0.5},{-0.7,247.9,0.0,-0.5},{-0.2,218.0,0.0,0.2},{
-0.6,-339.0,0.0,0.8},{-0.7,198.7,0.0,0.2},{-1.5,334.0,0.0,0.0
-},{0.1,334.0,0.0,0.0},{-0.1,-198.1,0.0,0.0},{-106.6,0.0,0.0,
-0.0},{-0.5,165.8,0.0,0.0},{0.0,134.8,0.0,0.0},{0.9,-151.6,
-0.0,0.0},{0.0,-129.7,0.0,0.0},{0.8,-132.8,0.0,-0.1},{0.5,-
-140.7,0.0,0.0},{-0.1,138.4,0.0,0.0},{0.0,129.0,0.0,-0.3},{
-0.5,-121.2,0.0,0.0},{-0.3,114.5,0.0,0.0},{-0.1,101.8,0.0,0.0
-},{-3.6,-101.9,0.0,0.0},{0.8,-109.4,0.0,0.0},{0.2,-97.0,0.0,
-0.0},{-0.7,157.3,0.0,0.0},{0.2,-83.3,0.0,0.0},{-0.3,93.3,0.0
-,0.0},{-0.1,92.1,0.0,0.0},{-0.5,133.6,0.0,0.0},{-0.1,81.5,
-0.0,0.0},{0.0,123.9,0.0,0.0},{-0.3,128.1,0.0,0.0},{0.1,74.1,
-0.0,-0.3},{-0.2,-70.3,0.0,0.0},{-0.4,66.6,0.0,0.0},{0.1,-
-66.7,0.0,0.0},{-0.7,69.3,0.0,-0.3},{0.0,-70.4,0.0,0.0},{-0.1
-,101.5,0.0,0.0},{0.5,-69.1,0.0,0.0},{-0.2,58.5,0.0,0.2},{0.1
-,-94.9,0.0,0.2},{0.0,52.9,0.0,-0.2},{0.1,86.7,0.0,-0.2},{-
-0.1,-59.2,0.0,0.2},{0.3,-58.8,0.0,0.1},{-0.3,49.0,0.0,0.0},{
--0.2,56.9,0.0,-0.1},{0.3,-50.2,0.0,0.0},{-0.2,53.4,0.0,-0.1}
-,{0.1,-76.5,0.0,0.0},{-0.2,45.3,0.0,0.0},{0.1,-46.8,0.0,0.0}
-,{0.2,-44.6,0.0,0.0},{0.2,-48.7,0.0,0.0},{0.1,-46.8,0.0,0.0}
-,{0.1,-42.0,0.0,0.0},{0.0,46.4,0.0,-0.1},{0.2,-67.3,0.0,0.1}
-,{0.0,-65.8,0.0,0.2},{-0.1,-43.9,0.0,0.3},{0.0,-38.9,0.0,0.0
-},{-0.3,63.9,0.0,0.0},{-0.2,41.2,0.0,0.0},{0.0,-36.1,0.0,0.2
-},{-0.3,58.5,0.0,0.0},{-0.1,36.1,0.0,0.0},{0.0,-39.7,0.0,0.0
-},{0.1,-57.7,0.0,0.0},{-0.2,33.4,0.0,0.0},{36.4,0.0,0.0,0.0}
-,{-0.1,55.7,0.0,-0.1},{0.1,-35.4,0.0,0.0},{0.1,-31.0,0.0,0.0
-},{-0.1,30.1,0.0,0.0},{-0.3,49.2,0.0,0.0},{-0.2,49.1,0.0,0.0
-},{-0.1,33.6,0.0,0.0},{0.1,-33.5,0.0,0.0},{0.1,-31.0,0.0,0.0
-},{-0.1,28.0,0.0,0.0},{0.1,-25.2,0.0,0.0},{0.1,-26.2,0.0,0.0
-},{-0.2,41.5,0.0,0.0},{0.0,24.5,0.0,0.1},{-16.2,0.0,0.0,0.0}
-,{0.0,-22.3,0.0,0.0},{0.0,23.1,0.0,0.0},{-0.1,37.5,0.0,0.0},
-{0.2,-25.7,0.0,0.0},{0.0,25.2,0.0,0.0},{0.1,-24.5,0.0,0.0},{
--0.1,24.3,0.0,0.0},{0.1,-20.7,0.0,0.0},{0.1,-20.8,0.0,0.0},{
--0.2,33.4,0.0,0.0},{32.9,0.0,0.0,0.0},{0.1,-32.6,0.0,0.0},{
-0.0,19.9,0.0,0.0},{-0.1,19.6,0.0,0.0},{0.0,-18.7,0.0,0.0},{
-0.1,-19.0,0.0,0.0},{0.1,-28.6,0.0,0.0},{4.0,178.8,-11.8,0.3}
-,{39.8,-107.3,-5.6,-1.0},{9.9,164.0,-4.1,0.1},{-4.8,-135.3,-
-3.4,-0.1},{50.5,75.0,1.4,-1.2},{-1.1,-53.5,1.3,0.0},{-45.0,-
-2.4,-0.4,6.6},{-11.5,-61.0,-0.9,0.4},{4.4,-68.4,-3.4,0.0},{
-7.7,-47.1,-4.7,-1.0},{-42.9,-12.6,-1.2,4.2},{-42.8,12.7,-1.2
-,-4.2},{-7.6,-44.1,2.1,-0.5},{-64.1,1.7,0.2,4.5},{36.4,-10.4
-,1.0,3.5},{35.6,10.2,1.0,-3.5},{-1.7,39.5,2.0,0.0},{50.9,-
-8.2,-0.8,-5.0},{0.0,52.3,1.2,0.0},{-42.9,-17.8,0.4,0.0},{2.6
-,34.3,0.8,0.0},{-0.8,-48.6,2.4,-0.1},{-4.9,30.5,3.7,0.7},{
-0.0,-43.6,2.1,0.0},{0.0,-25.4,1.2,0.0},{2.0,40.9,-2.0,0.0},{
--2.1,26.1,0.6,0.0},{22.6,-3.2,-0.5,-0.5},{-7.6,24.9,-0.4,-
-0.2},{-6.2,34.9,1.7,0.3},{2.0,17.4,-0.4,0.1},{-3.9,20.5,2.4,
-0.6}};static double BAz[][4]={{9205365.8,-1506.2,885.7,-0.2}
-,{573095.9,-570.2,-305.0,-0.3},{97845.5,147.8,-48.8,-0.2},{-
-89753.6,28.0,46.9,0.0},{7406.7,-327.1,-18.2,0.8},{22442.3,-
-22.3,-67.6,0.0},{-683.6,46.8,0.0,0.0},{20070.7,36.0,1.6,0.0}
-,{12893.8,39.5,-6.2,0.0},{-9593.2,14.4,30.2,-0.1},{-6899.5,
-4.8,-0.6,0.0},{-5332.5,-0.1,2.7,0.0},{-125.2,10.5,0.0,0.0},{
--3323.4,-0.9,-0.3,0.0},{3142.3,8.9,0.3,0.0},{2552.5,7.3,-1.2
-,0.0},{2634.4,8.8,0.2,0.0},{-2424.4,1.6,-0.4,0.0},{-123.3,
-3.9,0.0,0.0},{1642.4,7.3,-0.8,0.0},{47.9,3.2,0.0,0.0},{
-1321.2,6.2,-0.6,0.0},{-1234.1,-0.3,0.6,0.0},{-1076.5,-0.3,
-0.0,0.0},{-61.6,1.8,0.0,0.0},{-55.4,1.6,0.0,0.0},{856.9,-4.9
-,-2.1,0.0},{-800.7,-0.1,0.0,0.0},{685.1,-0.6,-3.8,0.0},{-
-16.9,-1.5,0.0,0.0},{695.7,1.8,0.0,0.0},{642.2,-2.6,-1.6,0.0}
-,{13.3,1.1,-0.1,0.0},{521.9,1.6,0.0,0.0},{325.8,2.0,-0.1,0.0
-},{-325.1,-0.5,0.9,0.0},{10.1,0.3,0.0,0.0},{334.5,1.6,0.0,
-0.0},{307.1,0.4,-0.9,0.0},{327.2,0.5,0.0,0.0},{-304.6,-0.1,
-0.0,0.0},{304.0,0.6,0.0,0.0},{-276.8,-0.5,0.1,0.0},{268.9,
-1.3,0.0,0.0},{271.8,1.1,0.0,0.0},{271.5,-0.4,-0.8,0.0},{-5.2
-,0.5,0.0,0.0},{-220.5,0.1,0.0,0.0},{-20.1,0.3,0.0,0.0},{-
-191.0,0.1,0.5,0.0},{-4.1,0.3,0.0,0.0},{130.6,-0.1,0.0,0.0},{
-3.0,0.3,0.0,0.0},{122.9,0.8,0.0,0.0},{3.7,-0.3,0.0,0.0},{
-123.1,0.4,-0.3,0.0},{-52.7,15.3,0.0,0.0},{120.7,0.3,-0.3,0.0
-},{4.0,-0.3,0.0,0.0},{126.5,0.5,0.0,0.0},{112.7,0.5,-0.3,0.0
-},{-106.1,-0.3,0.3,0.0},{-112.9,-0.2,0.0,0.0},{3.6,-0.2,0.0,
-0.0},{107.4,0.3,0.0,0.0},{-10.9,0.2,0.0,0.0},{-0.9,0.0,0.0,
-0.0},{85.4,0.0,0.0,0.0},{0.0,-88.8,0.0,0.0},{-71.0,-0.2,0.0,
-0.0},{-70.3,0.0,0.0,0.0},{64.5,0.4,0.0,0.0},{69.8,0.0,0.0,
-0.0},{66.1,0.4,0.0,0.0},{-61.0,-0.2,0.0,0.0},{-59.5,-0.1,0.0
-,0.0},{-55.6,0.0,0.2,0.0},{51.7,0.2,0.0,0.0},{-49.0,-0.1,0.0
-,0.0},{-52.7,-0.1,0.0,0.0},{-49.6,1.4,0.0,0.0},{46.3,0.4,0.0
-,0.0},{49.6,0.1,0.0,0.0},{-5.1,0.1,0.0,0.0},{-44.0,-0.1,0.0,
-0.0},{-39.9,-0.1,0.0,0.0},{-39.5,-0.1,0.0,0.0},{-3.9,0.1,0.0
-,0.0},{-42.1,-0.1,0.0,0.0},{-17.2,0.1,0.0,0.0},{-2.3,0.1,0.0
-,0.0},{-39.2,0.0,0.0,0.0},{-38.4,0.1,0.0,0.0},{36.8,0.2,0.0,
-0.0},{34.6,0.1,0.0,0.0},{-32.7,0.3,0.0,0.0},{30.4,0.0,0.0,
-0.0},{0.4,0.1,0.0,0.0},{29.3,0.2,0.0,0.0},{31.6,0.1,0.0,0.0}
-,{0.8,-0.1,0.0,0.0},{-27.9,0.0,0.0,0.0},{2.9,0.0,0.0,0.0},{-
-25.3,0.0,0.0,0.0},{25.0,0.1,0.0,0.0},{27.5,0.1,0.0,0.0},{-
-24.4,-0.1,0.0,0.0},{24.9,0.2,0.0,0.0},{-22.8,-0.1,0.0,0.0},{
-0.9,-0.1,0.0,0.0},{24.4,0.1,0.0,0.0},{23.9,0.1,0.0,0.0},{
-22.5,0.1,0.0,0.0},{20.8,0.1,0.0,0.0},{20.1,0.0,0.0,0.0},{
-21.5,0.1,0.0,0.0},{-20.0,0.0,0.0,0.0},{1.4,0.0,0.0,0.0},{-
-0.2,-0.1,0.0,0.0},{19.0,0.0,-0.1,0.0},{20.5,0.0,0.0,0.0},{-
-2.0,0.0,0.0,0.0},{-17.6,-0.1,0.0,0.0},{19.0,0.0,0.0,0.0},{-
-2.4,0.0,0.0,0.0},{-18.4,-0.1,0.0,0.0},{17.1,0.0,0.0,0.0},{
-0.4,0.0,0.0,0.0},{18.4,0.1,0.0,0.0},{0.0,17.4,0.0,0.0},{-0.6
-,0.0,0.0,0.0},{-15.4,0.0,0.0,0.0},{-16.8,-0.1,0.0,0.0},{16.3
-,0.0,0.0,0.0},{-2.0,0.0,0.0,0.0},{-1.5,0.0,0.0,0.0},{-14.3,-
-0.1,0.0,0.0},{14.4,0.0,0.0,0.0},{-13.4,0.0,0.0,0.0},{-14.3,-
-0.1,0.0,0.0},{-13.7,0.0,0.0,0.0},{13.1,0.1,0.0,0.0},{-1.7,
-0.0,0.0,0.0},{-12.8,0.0,0.0,0.0},{0.0,-14.4,0.0,0.0},{12.4,
-0.0,0.0,0.0},{-12.0,0.0,0.0,0.0},{-0.8,0.0,0.0,0.0},{10.9,
-0.1,0.0,0.0},{-10.8,0.0,0.0,0.0},{10.5,0.0,0.0,0.0},{-10.4,
-0.0,0.0,0.0},{-11.2,0.0,0.0,0.0},{10.5,0.1,0.0,0.0},{-1.4,
-0.0,0.0,0.0},{0.0,0.1,0.0,0.0},{0.7,0.0,0.0,0.0},{-10.3,0.0,
-0.0,0.0},{-10.0,0.0,0.0,0.0},{9.6,0.0,0.0,0.0},{9.4,0.1,0.0,
-0.0},{0.6,0.0,0.0,0.0},{-87.7,4.4,-0.4,-6.3},{46.3,22.4,0.5,
--2.4},{15.6,-3.4,0.1,0.4},{5.2,5.8,0.2,-0.1},{-30.1,26.9,0.7
-,0.0},{23.2,-0.5,0.0,0.6},{1.0,23.2,3.4,0.0},{-12.2,-4.3,0.0
-,0.0},{-2.1,-3.7,-0.2,0.1},{-18.6,-3.8,-0.4,1.8},{5.5,-18.7,
--1.8,-0.5},{-5.5,-18.7,1.8,-0.5},{18.4,-3.6,0.3,0.9},{-0.6,
-1.3,0.0,0.0},{-5.6,-19.5,1.9,0.0},{5.5,-19.1,-1.9,0.0},{-
-17.3,-0.8,0.0,0.9},{-3.2,-8.3,-0.8,0.3},{-0.1,0.0,0.0,0.0},{
--5.4,7.8,-0.3,0.0},{-14.8,1.4,0.0,0.3},{-3.8,0.4,0.0,-0.2},{
-12.6,3.2,0.5,-1.5},{0.1,0.0,0.0,0.0},{-13.6,2.4,-0.1,0.0},{
-0.9,1.2,0.0,0.0},{-11.9,-0.5,0.0,0.3},{0.4,12.0,0.3,-0.2},{
-8.3,6.1,-0.1,0.1},{0.0,0.0,0.0,0.0},{0.4,-10.8,0.3,0.0},{9.6
-,2.2,0.3,-1.2}};static int FObaR=sizeof(q6)/sizeof(int)/9;
-int foObAR;double Q7,Q8,q9,FOBAZ,q10,q11,Q12,q13,q14,Q15,
-foobaz,quux,Q16,Q17,q18;Q7=(Q0-Q4)/q5;Q8=134.96340251*DD2R+
-fmod(Q7*(1717915923.2178+Q7*(31.8792+Q7*(0.051635+Q7*(-
-0.00024470)))),q3)*DAS2R;q9=357.52910918*DD2R+fmod(Q7*(
-129596581.0481+Q7*(-0.5532+Q7*(0.000136+Q7*(-0.00001149)))),
-q3)*DAS2R;FOBAZ=93.27209062*DD2R+fmod(Q7*(1739527262.8478+Q7
-*(-12.7512+Q7*(-0.001037+Q7*(0.00000417)))),q3)*DAS2R;q10=
-297.85019547*DD2R+fmod(Q7*(1602961601.2090+Q7*(-6.3706+Q7*(
-0.006539+Q7*(-0.00003169)))),q3)*DAS2R;q11=125.04455501*DD2R
-+fmod(Q7*(-6962890.5431+Q7*(7.4722+Q7*(0.007702+Q7*(-
-0.00005939)))),q3)*DAS2R;Q12=181.97980085*DD2R+fmod(
-210664136.433548*Q7,q3)*DAS2R;q13=355.43299958*DD2R+fmod(
-68905077.493988*Q7,q3)*DAS2R;q14=34.35151874*DD2R+fmod(
-10925660.377991*Q7,q3)*DAS2R;Q15=50.07744430*DD2R+fmod(
-4399609.855732*Q7,q3)*DAS2R;Q17=-153.1*sin(q9)-1.9*sin(2.0*
-q9);q18=0.0;for(foObAR=FObaR-1;foObAR>=0;foObAR--){foobaz=((
-double)q6[foObAR][0])*Q8+((double)q6[foObAR][1])*q9+((double
-)q6[foObAR][2])*FOBAZ+((double)q6[foObAR][3])*q10+((double)
-q6[foObAR][4])*q11+((double)q6[foObAR][5])*Q12+((double)q6[
-foObAR][6])*q13+((double)q6[foObAR][7])*q14+((double)q6[
-foObAR][8])*Q15;quux=cos(foobaz);Q16=sin(foobaz);Q17+=(bar[
-foObAR][0]+bar[foObAR][2]*Q7)*quux+(bar[foObAR][1]+bar[
-foObAR][3]*Q7)*Q16;q18+=(BAz[foObAR][0]+BAz[foObAR][2]*Q7)*
-quux+(BAz[foObAR][1]+BAz[foObAR][3]*Q7)*Q16;}*foo=(Q17*1e-6-
-0.042888-0.29856*Q7)*DAS2R;*q1=(q18*1e-6-0.005171-0.02408*Q7
-)*DAS2R;*Q2=(84381.412+(-46.80927+(-0.000152+(0.0019989+(-
-0.00000051+(-0.000000025)*Q7)*Q7)*Q7)*Q7)*Q7)*DAS2R;}
-#undef q3
-#undef Q4
-#undef q5
-
-void palSlaPm(double Q0,double foo,double Q1,double BAR,double
-BAZ,double Q2,double Q3,double q4,double*fobar,double*q5){
-static double q6=(365.25*86400.0/149597870.0)*DAS2R;int q7;
-double FOOBAR,FOBAZ[3],foobaz,QUuX[3];palSlaDcs2c(Q0,foo,QUuX);
-FOOBAR=q6*Q2*BAZ;FOBAZ[0]=-Q1*QUuX[1]-BAR*cos(Q0)*sin(foo)+
-FOOBAR*QUuX[0];FOBAZ[1]=Q1*QUuX[0]-BAR*sin(Q0)*sin(foo)+
-FOOBAR*QUuX[1];FOBAZ[2]=BAR*cos(foo)+FOOBAR*QUuX[2];foobaz=
-q4-Q3;for(q7=0;q7<3;q7++)QUuX[q7]=QUuX[q7]+(foobaz*FOBAZ[q7]
-);palSlaDcc2s(QUuX,fobar,q5);*fobar=palSlaDranrm(*fobar);}
-
-void palSlaPrebn(double foo,double q0,double q1[3][3]){double
-BAr,q2,Baz,Q3,fobar,FOOBAR,q4;BAr=(foo-1850.0)/100.0;q2=(q0-
-foo)/100.0;Baz=q2*DAS2R;Q3=2303.5548+(1.39720+0.000059*BAr)*
-BAr;fobar=(Q3+(0.30242-0.000269*BAr+0.017996*q2)*q2)*Baz;
-FOOBAR=(Q3+(1.09478+0.000387*BAr+0.018324*q2)*q2)*Baz;q4=(
-2005.1125+(-0.85294-0.000365*BAr)*BAr+(-0.42647-0.000365*BAr
--0.041802*q2)*q2)*Baz;palSlaDeuler("\132\131\132",-fobar,q4,-
-FOOBAR,q1);}
-
-void palSlaPrec(double q0,double q1,double q2[3][3]){double Q3,
-Q4,Q5,FOO,BAR,Q6,BAZ;Q3=(q0-2000.0)/100.0;Q4=(q1-q0)/100.0;
-Q5=Q4*DAS2R;FOO=2306.2181+((1.39656-(0.000139*Q3))*Q3);BAR=(
-FOO+((0.30188-0.000344*Q3)+0.017998*Q4)*Q4)*Q5;Q6=(FOO+((
-1.09468+0.000066*Q3)+0.018203*Q4)*Q4)*Q5;BAZ=((2004.3109+(-
-0.85330-0.000217*Q3)*Q3)+((-0.42665-0.000217*Q3)-0.041833*Q4
-)*Q4)*Q5;palSlaDeuler("\132\131\132",-BAR,BAZ,-Q6,q2);}
-
-void palSlaPrenut(double FOO,double Q0,double q1[3][3]){double
-BAr[3][3],q2[3][3];palSlaPrec(FOO,palSlaEpj(Q0),BAr);palSlaNut(Q0,q2)
-;palSlaDmxm(q2,BAr,q1);}
-
-void palSlaRefco(double foo,double Q0,double q1,double BAr,
-double q2,double baz,double q3,double Q4,double*FOBAR,double
-*q5){double FOOBAR,Q6;static double Q7=0.7853981633974483;
-static double q8=1.325817663668033;palSlaRefro(Q7,foo,Q0,q1,BAr
-,q2,baz,q3,Q4,&FOOBAR);palSlaRefro(q8,foo,Q0,q1,BAr,q2,baz,q3,
-Q4,&Q6);*FOBAR=(64.0*FOOBAR-Q6)/60.0;*q5=(Q6-4.0*FOOBAR)/
-60.0;}
-
-static void q0(double,double,double,double,double,double,
-double,double,double,double,double,double,double*,double*,
-double*);static void FOO(double,double,double,double,double,
-double*,double*);void palSlaRefro(double q1,double BAR,double
-Q2,double Q3,double q4,double q5,double q6,double q7,double
-baz,double*FOBAR)
-#define foobar 16384
-{static double fobaz=1.623156204;static double Q8=8314.32;
-static double FOObAz=28.9644;static double q9=18.0152;static
- double quux=6378120.0;static double q10=18.36;static double
- q11=11000.0;static double FREd=80000.0;double dog;double
-Q12;double q13;double q14;double Q15;double Q16,caT,q17,FISH
-,GASP,bad;double Q18;double q19;double Q20;double bug;int
-SILLY,Q21,Q22,buggy,mum,dad;double q23,q24,q25,DISK,EMPty,
-q26,FuLl,q27,FAST,SMALL,big,OK,HeLLo,bYE,q28,MaGIC,oBscuRe,
-speed,iNdEX,bAR_FOO,Bar_BAr,Q29,Q30,q31,q32,bar_baz,Q33,q34,
-bar_fOBAR,Q35,Q36,BAR_FOOBAR,Q37,q38,bAr_FOBaZ,q39,Q40,q41,
-baR_fOoBaz,q42,BaR_qUux,Q43,BAR_FRED,BaR_DoG,Q44,BAr_CAt,
-bar_fish,Q45,q46,Q47,Q48;
-#define q49(Q50,q51) ((q51)/(Q50+q51));
-Q48=0.0;
-q23=palSlaDrange(q1);q24=fabs(q23);q24=gmin(q24,fobaz);q25=gmax
-(BAR,-1000.0);q25=gmin(q25,FREd);Q12=gmax(Q2,100.0);Q12=gmin
-(Q12,500.0);DISK=gmax(Q3,0.0);DISK=gmin(DISK,10000.0);EMPty=
-gmax(q4,0.0);EMPty=gmin(EMPty,1.0);q26=gmax(q5,0.1);q13=fabs
-(q7);q13=gmax(q13,0.001);q13=gmin(q13,0.01);q28=fabs(baz);
-q28=gmax(q28,1e-12);FuLl=gmin(q28,0.1)/2.0;dad=(q26<=100.0);
-q27=q26*q26;FAST=9.784*(1.0-0.0026*cos(2.0*q6)-2.8e-7*q25);
-SMALL=(dad)?((287.604+1.6288/q27+0.0136/(q27*q27))*273.15/
-1013.25)*1e-6:77.6890e-6;bug=FAST*FOObAz/Q8;big=bug/q13;q14=
-big-2.0;Q15=q10-2.0;OK=Q12-273.15;HeLLo=pow(10.0,(0.7859+
-0.03477*OK)/(1.0+0.00412*OK))*(1.0+DISK*(4.5e-6+6e-10*OK*OK)
-);bYE=(DISK>0.0)?EMPty*HeLLo/(1.0-(1.0-EMPty)*HeLLo/DISK):
-0.0;q28=bYE*(1.0-q9/FOObAz)*big/(q10-big);Q16=SMALL*(DISK+
-q28)/Q12;caT=(SMALL*q28+(dad?11.2684e-6:6.3938e-6)*bYE)/Q12;
-q17=(big-1.0)*q13*Q16/Q12;FISH=(q10-1.0)*q13*caT/Q12;GASP=
-dad?0.0:375463e-6*bYE/Q12;bad=GASP*Q15*q13/(Q12*Q12);dog=
-quux+q25;q0(dog,Q12,q13,q14,Q15,Q16,caT,q17,FISH,GASP,bad,
-dog,&MaGIC,&oBscuRe,&speed);iNdEX=oBscuRe*dog*sin(q24);
-bAR_FOO=q49(oBscuRe,speed);Q18=quux+gmax(q11,q25);q0(dog,Q12
-,q13,q14,Q15,Q16,caT,q17,FISH,GASP,bad,Q18,&q19,&Q20,&
-Bar_BAr);Q29=asin(iNdEX/(Q18*Q20));Q30=q49(Q20,Bar_BAr);FOO(
-Q18,q19,Q20,bug,Q18,&q31,&q32);bar_baz=asin(iNdEX/(Q18*q31))
-;Q33=q49(q31,q32);q34=quux+FREd;FOO(Q18,q19,Q20,bug,q34,&
-bar_fOBAR,&Q35);Q36=asin(iNdEX/(q34*bar_fOBAR));BAR_FOOBAR=
-q49(bar_fOBAR,Q35);for(Q21=1;Q21<=2;Q21++){Q37=1.0;SILLY=8;
-if(Q21==1){q38=q24;bAr_FOBaZ=Q29-q38;q39=bAR_FOO;Q40=Q30;}
-else{q38=bar_baz;bAr_FOBaZ=Q36-q38;q39=Q33;Q40=BAR_FOOBAR;}
-q41=0.0;baR_fOoBaz=0.0;Q22=1;for(;;){q42=bAr_FOBaZ/(double)
-SILLY;BaR_qUux=(Q21==1)?dog:Q18;for(buggy=1;buggy<SILLY;
-buggy+=Q22){Q43=sin(q38+q42*(double)buggy);if(Q43>1e-20){q28
-=iNdEX/Q43;BAR_FRED=BaR_qUux;mum=0;do{if(Q21==1){q0(dog,Q12,
-q13,q14,Q15,Q16,caT,q17,FISH,GASP,bad,BAR_FRED,&Q44,&BAr_CAt
-,&bar_fish);}else{FOO(Q18,q19,Q20,bug,BAR_FRED,&BAr_CAt,&
-bar_fish);}BaR_DoG=(BAR_FRED*BAr_CAt-q28)/(BAr_CAt+bar_fish)
-;BAR_FRED-=BaR_DoG;}while(fabs(BaR_DoG)>1.0&&mum++<=4);
-BaR_qUux=BAR_FRED;}if(Q21==1){q0(dog,Q12,q13,q14,Q15,Q16,caT
-,q17,FISH,GASP,bad,BaR_qUux,&Q45,&BAr_CAt,&bar_fish);}else{
-FOO(Q18,q19,Q20,bug,BaR_qUux,&BAr_CAt,&bar_fish);}q46=q49(
-BAr_CAt,bar_fish);if(Q22==1&&buggy%2==0){baR_fOoBaz+=q46;}
-else{q41+=q46;}}Q47=q42*(q39+4.0*q41+2.0*baR_fOoBaz+Q40)/3.0
-;if(Q21==1)Q48=Q47;if(fabs(Q47-Q37)<=FuLl||SILLY>=foobar)
-break;Q37=Q47;SILLY+=SILLY;baR_fOoBaz+=q41;q41=0.0;Q22=2;}}*
-FOBAR=Q48+Q47;if(q23<0.0)*FOBAR=-(*FOBAR);}static void q0(
-double dog,double Q12,double q13,double q14,double Q15,
-double Q16,double caT,double q17,double FISH,double GASP,
-double bad,double BaR_qUux,double*Q45,double*BAr_CAt,double*
-bar_fish){double q28,Q52,Q53,BAR_GASp;q28=Q12-q13*(BaR_qUux-
-dog);q28=gmin(q28,320.0);q28=gmax(q28,100.0);Q52=q28/Q12;Q53
-=pow(Q52,q14);BAR_GASp=pow(Q52,Q15);*Q45=q28;*BAr_CAt=1.0+(
-Q16*Q53-(caT-GASP/q28)*BAR_GASp)*Q52;*bar_fish=BaR_qUux*(-
-q17*Q53+(FISH-bad/Q52)*BAR_GASp);}static void FOO(double Q18
-,double q19,double Q20,double bug,double BaR_qUux,double*
-BAr_CAt,double*bar_fish){double BAR_BAD,q28;BAR_BAD=bug/q19;
-q28=(Q20-1.0)*exp(-BAR_BAD*(BaR_qUux-Q18));*BAr_CAt=1.0+q28;
-*bar_fish=-BaR_qUux*BAR_BAD*q28;}
-#undef foobar
-#undef q49
-
-float palSlaRverot(float Q0,float q1,float foo,float q2)
-#define q3 0.4655
-{return(float)(q3*cos((double)Q0)*sin((double)(q2-q1))*cos((
-double)foo));}
-#undef q3
-
-float palSlaRvgalc(float Q0,float FOo){static float q1[3]={-
-108.70408f,97.86251f,-164.33610f};float BAR[3];palSlaCs2c(Q0,
-FOo,BAR);return palSlaVdv(q1,BAR);}
-
-float palSlaRvlg(float FOO,float BAR){static float baz[3]={-
-148.23284f,133.44888f,-224.09467f};float Q0[3];palSlaCs2c(FOO,
-BAR,Q0);return palSlaVdv(baz,Q0);}
-
-float palSlaRvlsrd(float foo,float Q0){static float BAr[3]={
-0.63823f,14.58542f,-7.80116f};float q1[3];palSlaCs2c(foo,Q0,q1)
-;return palSlaVdv(BAr,q1);}
-
-float palSlaRvlsrk(float q0,float Q1){static float foo[3]={-
-0.29000f,17.31726f,-10.00141f};float q2[3];palSlaCs2c(q0,Q1,q2)
-;return palSlaVdv(foo,q2);}
-
-void palSlaSubet(double Q0,double FOO,double q1,double*BAR,
-double*q2){double Q3[3],Q4[3],Baz;int q5;palSlaEtrms(q1,Q3);
-palSlaDcs2c(Q0,FOO,Q4);Baz=1.0+palSlaDvdv(Q4,Q3);for(q5=0;q5<3;q5
-++){Q4[q5]=Baz*Q4[q5]-Q3[q5];}palSlaDcc2s(Q4,BAR,q2);*BAR=
-palSlaDranrm(*BAR);}
-
-void palSlaSupgal(double foo,double baR,double*BAZ,double*q0){
-double Q1[3],FOBAR[3];static double Q2[3][3]={{-
-0.735742574804,0.677261296414,0.0},{-0.074553778365,-
-0.080991471307,0.993922590400},{0.673145302109,
-0.731271165817,0.110081262225}};palSlaDcs2c(foo,baR,Q1);
-palSlaDimxv(Q2,Q1,FOBAR);palSlaDcc2s(FOBAR,BAZ,q0);*BAZ=palSlaDranrm(
-*BAZ);*q0=palSlaDrange(*q0);}
-
-float palSlaVdv(float FOO[3],float BAR[3]){return FOO[0]*BAR[0]
-+FOO[1]*BAR[1]+FOO[2]*BAR[2];}
-
-
-/* Not quite like slaDh2e since it converts from topocentric (az,el) to
- apparent (ha,dec). This includes a correction for diurnal aberration.
- The magnitude of the diurnal aberration vector should be supplied in
- parameter "diurab". The extra code is taken from the Fortran routine
- SLA_OAPQK. */
-
-void palSlaDh2e(double az,double el,double phi,double diurab,double *ha,double *dec){
- double sa,ca,se,ce,sp,cp,x,y,z,r,xmhda,ymhda,zmhda,f;
-
- sa=sin(az);
- ca=cos(az);
- se=sin(el);
- ce=cos(el);
- sp=sin(phi);
- cp=cos(phi);
-
-/* Cartesian (az,el) to Cartesian (ha,dec) - note, +ha, not -ha. */
- xmhda=-ca*ce*sp+se*cp;
- ymhda=-sa*ce;
- zmhda=ca*ce*cp+se*sp;
-
-/* Correct this vector for diurnal aberration. Since the above
- expressions produce +ha rather than -ha, we do not negate "diurab"
- before using it. Compare this to SLA_AOPQK. */
- f = (1-diurab*ymhda);
- x = f*xmhda;
- y = f*(ymhda+diurab);
- z = f*zmhda;
-
-/* Cartesian (ha,dec) to spherical (ha,dec). */
- r=sqrt(x*x+y*y);
- if (r==0.0) {
- *ha=0.0;
- } else {
- *ha=atan2(y,x);
- }
- *dec=atan2(z,r);
-}
-
-
-/* Not quite like slaDe2h since it converts from apparent (ha,dec) to
- topocentric (az,el). This includes a correction for diurnal
- aberration. The magnitude of the diurnal aberration vector should be
- supplied in parameter "diurab". The extra code is taken from the
- Fortran routine SLA_AOPQK. */
-
-void palSlaDe2h( double ha, double dec, double phi, double diurab,
- double *az, double *el){
- double sh,ch,sd,cd,sp,cp,x,y,z,r,a,xhd,yhd,zhd,xhdt,yhdt,zhdt,f;
-
- sh=sin(ha);
- ch=cos(ha);
- sd=sin(dec);
- cd=cos(dec);
- sp=sin(phi);
- cp=cos(phi);
-
-/* Components of cartesian (-ha,dec) vector. */
- xhd = ch*cd;
- yhd = -sh*cd;
- zhd = sd;
-
-/* Modify the above vector to apply diurnal aberration. */
- f = (1.0-diurab*yhd);
- xhdt = f*xhd;
- yhdt = f*(yhd+diurab);
- zhdt = f*zhd;
-
-/* Convert to cartesian (az,el). */
- x=-xhdt*sp+zhdt*cp;
- y=yhdt;
- z=xhdt*cp+zhdt*sp;
-
-/* Convert to spherical (az,el). */
- r=sqrt(x*x+y*y);
- if( r == 0.0 ) {
- a=0.0;
- } else {
- a=atan2(y,x);
- }
-
- if(a<0.0) a=a+D2PI;
-
- *az=a;
- *el=atan2(z,r);
-}
-
-
-
-double palSlaGmsta( double Dt, double uQ){ static double
-s2r=7.272205216643039903848712E-5; double r,d1,d2,t; if(Dt<uQ) { d1=Dt;
-d2=uQ; } else { d1=uQ; d2=Dt; } t=(d1+(d2-51544.5))/36525.0;
-r=palSlaDranrm(s2r*(24110.54841+ (8640184.812866+ (0.093104
--6.2E-6*t)*t)*t +86400.0*(fmod(d1,1.0)+fmod(d2,1.0)))); return r; }
-
-void palSlaPvobs(double p,double h,double stl,double pv[6]){double
-r,z,s,c,v;double sr=7.292115855306589E-5;palSlaGeoc(p,h,&r,&z);
-s=sin(stl);c=cos(stl);v=sr*r;pv[0]=r*c;pv[1]=r*s;pv[2]=z;
-pv[3]=-v*s;pv[4]=v*c;pv[5]=0.0;}
-
-
-
+/* Include configuration results in order to get any definition for the
+ EXTERNAL_PAL macro. This macro is set if the --with-external_pal
+ option was set when AST was configured. */
+#if HAVE_CONFIG_H
+#include <config.h>
+#endif
+
+/* If an external PAL library is being used, we leave this file empty. */
+#ifndef EXTERNAL_PAL
+
+/* Rename all PAL functions so that references to "palXxx" in the files
+ included below get translated to "astPalXxx". */
+#include "pal2ast.h"
+
+/* Rename all SOFA functions so that references to "iauXxx" in the files
+ included below get translated to "astIauXxx". */
+#include "sofa2ast.h"
+
+/* Include code from all PAL source files */
+#include "pal/palAddet.c"
+#include "pal/palAmpqk.c"
+#include "pal/palCaldj.c"
+#include "pal/palDat.c"
+#include "pal/palDe2h.c"
+#include "pal/palDeuler.c"
+#include "pal/palDh2e.c"
+#include "pal/palDjcal.c"
+#include "pal/palDmat.c"
+#include "pal/palDs2tp.c"
+#include "pal/palDtp2s.c"
+#include "pal/palDtps2c.c"
+#include "pal/palDtt.c"
+#include "pal/palEcmat.c"
+#include "pal/palEqgal.c"
+#include "pal/palEtrms.c"
+#include "pal/palEvp.c"
+#include "pal/palFk45z.c"
+#include "pal/palFk524.c"
+#include "pal/palFk54z.c"
+#include "pal/palGaleq.c"
+#include "pal/palGalsup.c"
+#include "pal/palMappa.c"
+#include "pal/palMapqkz.c"
+#include "pal/palOne2One.c"
+#include "pal/palPrebn.c"
+#include "pal/palPrec.c"
+#include "pal/palPrenut.c"
+#include "pal/palPvobs.c"
+#include "pal/palRvgalc.c"
+#include "pal/palRvlg.c"
+#include "pal/palRvlsrd.c"
+#include "pal/palRvlsrk.c"
+#include "pal/palSubet.c"
+#include "pal/palSupgal.c"
+
+/* Include code from all SOFA source files */
+#include "sofa/a2af.c"
+#include "sofa/a2tf.c"
+#include "sofa/af2a.c"
+#include "sofa/anp.c"
+#include "sofa/anpm.c"
+#include "sofa/bi00.c"
+#include "sofa/bp00.c"
+#include "sofa/bp06.c"
+#include "sofa/bpn2xy.c"
+#include "sofa/c2i00a.c"
+#include "sofa/c2i00b.c"
+#include "sofa/c2i06a.c"
+#include "sofa/c2ibpn.c"
+#include "sofa/c2ixy.c"
+#include "sofa/c2ixys.c"
+#include "sofa/c2s.c"
+#include "sofa/c2t00a.c"
+#include "sofa/c2t00b.c"
+#include "sofa/c2t06a.c"
+#include "sofa/c2tcio.c"
+#include "sofa/c2teqx.c"
+#include "sofa/c2tpe.c"
+#include "sofa/c2txy.c"
+#include "sofa/cal2jd.c"
+#include "sofa/cp.c"
+#include "sofa/cpv.c"
+#include "sofa/cr.c"
+#include "sofa/d2dtf.c"
+#include "sofa/d2tf.c"
+#include "sofa/dat.c"
+#include "sofa/dtdb.c"
+#include "sofa/dtf2d.c"
+#include "sofa/ee00.c"
+#include "sofa/ee00a.c"
+#include "sofa/ee00b.c"
+#include "sofa/ee06a.c"
+#include "sofa/eect00.c"
+#include "sofa/eform.c"
+#include "sofa/eo06a.c"
+#include "sofa/eors.c"
+#include "sofa/epb.c"
+#include "sofa/epb2jd.c"
+#include "sofa/epj.c"
+#include "sofa/epj2jd.c"
+#include "sofa/epv00.c"
+#include "sofa/eqeq94.c"
+#include "sofa/era00.c"
+#include "sofa/fad03.c"
+#include "sofa/fae03.c"
+#include "sofa/faf03.c"
+#include "sofa/faju03.c"
+#include "sofa/fal03.c"
+#include "sofa/falp03.c"
+#include "sofa/fama03.c"
+#include "sofa/fame03.c"
+#include "sofa/fane03.c"
+#include "sofa/faom03.c"
+#include "sofa/fapa03.c"
+#include "sofa/fasa03.c"
+#include "sofa/faur03.c"
+#include "sofa/fave03.c"
+#include "sofa/fk52h.c"
+#include "sofa/fk5hip.c"
+#include "sofa/fk5hz.c"
+#include "sofa/fw2m.c"
+#include "sofa/fw2xy.c"
+#include "sofa/gc2gd.c"
+#include "sofa/gc2gde.c"
+#include "sofa/gd2gc.c"
+#include "sofa/gd2gce.c"
+#include "sofa/gmst00.c"
+#include "sofa/gmst06.c"
+#include "sofa/gmst82.c"
+#include "sofa/gst00a.c"
+#include "sofa/gst00b.c"
+#include "sofa/gst06.c"
+#include "sofa/gst06a.c"
+#include "sofa/gst94.c"
+#include "sofa/h2fk5.c"
+#include "sofa/hfk5z.c"
+#include "sofa/ir.c"
+#include "sofa/jd2cal.c"
+#include "sofa/jdcalf.c"
+#include "sofa/num00a.c"
+#include "sofa/num00b.c"
+#include "sofa/num06a.c"
+#include "sofa/numat.c"
+#include "sofa/nut00a.c"
+#include "sofa/nut00b.c"
+#include "sofa/nut06a.c"
+#include "sofa/nut80.c"
+#include "sofa/nutm80.c"
+#include "sofa/obl06.c"
+#include "sofa/obl80.c"
+#include "sofa/p06e.c"
+#include "sofa/p2pv.c"
+#include "sofa/p2s.c"
+#include "sofa/pap.c"
+#include "sofa/pas.c"
+#include "sofa/pb06.c"
+#include "sofa/pdp.c"
+#include "sofa/pfw06.c"
+#include "sofa/plan94.c"
+#include "sofa/pm.c"
+#include "sofa/pmat00.c"
+#include "sofa/pmat06.c"
+#include "sofa/pmat76.c"
+#include "sofa/pmp.c"
+#include "sofa/pn.c"
+#include "sofa/pn00.c"
+#include "sofa/pn00a.c"
+#include "sofa/pn00b.c"
+#include "sofa/pn06.c"
+#include "sofa/pn06a.c"
+#include "sofa/pnm00a.c"
+#include "sofa/pnm00b.c"
+#include "sofa/pnm06a.c"
+#include "sofa/pnm80.c"
+#include "sofa/pom00.c"
+#include "sofa/ppp.c"
+#include "sofa/ppsp.c"
+#include "sofa/pr00.c"
+#include "sofa/prec76.c"
+#include "sofa/pv2p.c"
+#include "sofa/pv2s.c"
+#include "sofa/pvdpv.c"
+#include "sofa/pvm.c"
+#include "sofa/pvmpv.c"
+#include "sofa/pvppv.c"
+#include "sofa/pvstar.c"
+#include "sofa/pvu.c"
+#include "sofa/pvup.c"
+#include "sofa/pvxpv.c"
+#include "sofa/pxp.c"
+#include "sofa/rm2v.c"
+#include "sofa/rv2m.c"
+#include "sofa/rx.c"
+#include "sofa/rxp.c"
+#include "sofa/rxpv.c"
+#include "sofa/rxr.c"
+#include "sofa/ry.c"
+#include "sofa/rz.c"
+#include "sofa/s00.c"
+#include "sofa/s00a.c"
+#include "sofa/s00b.c"
+#include "sofa/s06.c"
+#include "sofa/s06a.c"
+#include "sofa/s2c.c"
+#include "sofa/s2p.c"
+#include "sofa/s2pv.c"
+#include "sofa/s2xpv.c"
+#include "sofa/sepp.c"
+#include "sofa/seps.c"
+#include "sofa/sp00.c"
+#include "sofa/starpm.c"
+#include "sofa/starpv.c"
+#include "sofa/sxp.c"
+#include "sofa/sxpv.c"
+#include "sofa/taitt.c"
+#include "sofa/taiut1.c"
+#include "sofa/taiutc.c"
+#include "sofa/tcbtdb.c"
+#include "sofa/tcgtt.c"
+#include "sofa/tdbtcb.c"
+#include "sofa/tdbtt.c"
+#include "sofa/tf2a.c"
+#include "sofa/tf2d.c"
+#include "sofa/tr.c"
+#include "sofa/trxp.c"
+#include "sofa/trxpv.c"
+#include "sofa/tttai.c"
+#include "sofa/tttcg.c"
+#include "sofa/tttdb.c"
+#include "sofa/ttut1.c"
+#include "sofa/ut1tai.c"
+#include "sofa/ut1tt.c"
+#include "sofa/ut1utc.c"
+#include "sofa/utctai.c"
+#include "sofa/utcut1.c"
+#include "sofa/xy06.c"
+#include "sofa/xys00a.c"
+#include "sofa/xys00b.c"
+#include "sofa/xys06a.c"
+#include "sofa/zp.c"
+#include "sofa/zpv.c"
+#include "sofa/zr.c"
+
+#endif
+
+#endif
diff --git a/pal.h b/pal.h
index 820427a..da3477b 100644
--- a/pal.h
+++ b/pal.h
@@ -1,507 +1,556 @@
#ifndef PALHDEF
#define PALHDEF
+
/*
-** Author:
-** Patrick Wallace (ptw at tpsoft.demon.co.uk)
-**
-** License:
-** This program is free software; you can redistribute it and/or modify
-** it under the terms of the GNU General Public License as published by
-** the Free Software Foundation; either version 2 of the License, or
-** (at your option) any later version.
-**
-** This program is distributed in the hope that it will be useful,
-** but WITHOUT ANY WARRANTY; without even the implied warranty of
-** MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
-** GNU General Public License for more details.
-**
-** You should have received a copy of the GNU General Public License
-** along with this program; if not, write to the Free Software
-** Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
-** USA.
-**
-** Last revision: 10 December 2002
-**
+*+
+* Name:
+* pal.h
+
+* Purpose:
+* Function prototypes for PAL routines.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Include file
+
+* Description:
+* Function prototypes for PAL routines.
+
+* Authors:
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* DSBJ: David S Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-08 (TIMJ):
+* Initial version. Define all SLA prototypes in PAL form even
+* though none are implemented.
+* 16-FEB-2012 (DSB):
+* If the PAL and SOFA libraries distributed within AST are being
+* used, rename the public symbols defined by both to avoid clashes
+* with any external PAL or SOFA library.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
*/
+/* Include configuration results in order to get any definition for the
+ EXTERNAL_PAL macro. This macro is set if the --with-external_pal
+ option was set when AST was configured. */
+#if HAVE_CONFIG_H
+#include <config.h>
+#endif
+
+/* If we not using external PAL and SOFA libraries, rename all PAL
+ functions so that references to "palXxx" below get translated to
+ "astPalXxx". */
+#ifndef EXTERNAL_PAL
+#include "pal2ast.h"
+#endif
+
#ifdef __cplusplus
extern "C" {
#endif
#include <math.h>
-void palSlaAddet ( double rm, double dm, double eq, double *rc, double *dc );
+/* Prototypes for all PAL functions. */
+
+void palAddet ( double rm, double dm, double eq, double *rc, double *dc );
-void palSlaAfin ( char *string, int *iptr, float *a, int *j );
+void palAfin ( const char *string, int *iptr, float *a, int *j );
-double palSlaAirmas ( double zd );
+double palAirmas ( double zd );
-void palSlaAltaz ( double ha, double dec, double phi,
+void palAltaz ( double ha, double dec, double phi,
double *az, double *azd, double *azdd,
double *el, double *eld, double *eldd,
double *pa, double *pad, double *padd );
-void palSlaAmp ( double ra, double da, double date, double eq,
+void palAmp ( double ra, double da, double date, double eq,
double *rm, double *dm );
-void palSlaAmpqk ( double ra, double da, double amprms[21],
+void palAmpqk ( double ra, double da, double amprms[21],
double *rm, double *dm );
-void palSlaAop ( double rap, double dap, double date, double dut,
+void palAop ( double rap, double dap, double date, double dut,
double elongm, double phim, double hm, double xp,
double yp, double tdk, double pmb, double rh,
double wl, double tlr,
double *aob, double *zob, double *hob,
double *dob, double *rob );
-void palSlaAoppa ( double date, double dut, double elongm, double phim,
+void palAoppa ( double date, double dut, double elongm, double phim,
double hm, double xp, double yp, double tdk, double pmb,
double rh, double wl, double tlr, double aoprms[14] );
-void palSlaAoppat ( double date, double aoprms[14] );
+void palAoppat ( double date, double aoprms[14] );
-void palSlaAopqk ( double rap, double dap, double aoprms[14],
+void palAopqk ( double rap, double dap, double aoprms[14],
double *aob, double *zob, double *hob,
double *dob, double *rob );
-void palSlaAtmdsp ( double tdk, double pmb, double rh, double wl1,
+void palAtmdsp ( double tdk, double pmb, double rh, double wl1,
double a1, double b1, double wl2, double *a2, double *b2 );
-void palSlaAv2m ( float axvec[3], float rmat[3][3] );
+void palAv2m ( float axvec[3], float rmat[3][3] );
-float palSlaBear ( float a1, float b1, float a2, float b2 );
+float palBear ( float a1, float b1, float a2, float b2 );
-void palSlaCaf2r ( int ideg, int iamin, float asec, float *rad, int *j );
+void palCaf2r ( int ideg, int iamin, float asec, float *rad, int *j );
-void palSlaCaldj ( int iy, int im, int id, double *djm, int *j );
+void palCaldj ( int iy, int im, int id, double *djm, int *j );
-void palSlaCalyd ( int iy, int im, int id, int *ny, int *nd, int *j );
+void palCalyd ( int iy, int im, int id, int *ny, int *nd, int *j );
-void palSlaCc2s ( float v[3], float *a, float *b );
+void palCc2s ( float v[3], float *a, float *b );
-void palSlaCc62s ( float v[6], float *a, float *b, float *r,
+void palCc62s ( float v[6], float *a, float *b, float *r,
float *ad, float *bd, float *rd );
-void palSlaCd2tf ( int ndp, float days, char *sign, int ihmsf[4] );
+void palCd2tf ( int ndp, float days, char *sign, int ihmsf[4] );
-void palSlaCldj ( int iy, int im, int id, double *djm, int *j );
+void palCldj ( int iy, int im, int id, double *djm, int *j );
-void palSlaClyd ( int iy, int im, int id, int *ny, int *nd, int *jstat );
+void palClyd ( int iy, int im, int id, int *ny, int *nd, int *jstat );
-void palSlaCombn ( int nsel, int ncand, int list[], int *j );
+void palCombn ( int nsel, int ncand, int list[], int *j );
-void palSlaCr2af ( int ndp, float angle, char *sign, int idmsf[4] );
+void palCr2af ( int ndp, float angle, char *sign, int idmsf[4] );
-void palSlaCr2tf ( int ndp, float angle, char *sign, int ihmsf[4] );
+void palCr2tf ( int ndp, float angle, char *sign, int ihmsf[4] );
-void palSlaCs2c ( float a, float b, float v[3] );
+void palCs2c ( float a, float b, float v[3] );
-void palSlaCs2c6 ( float a, float b, float r, float ad,
+void palCs2c6 ( float a, float b, float r, float ad,
float bd, float rd, float v[6] );
-void palSlaCtf2d ( int ihour, int imin, float sec, float *days, int *j );
+void palCtf2d ( int ihour, int imin, float sec, float *days, int *j );
-void palSlaCtf2r ( int ihour, int imin, float sec, float *rad, int *j );
+void palCtf2r ( int ihour, int imin, float sec, float *rad, int *j );
-void palSlaDaf2r ( int ideg, int iamin, double asec, double *rad, int *j );
+void palDaf2r ( int ideg, int iamin, double asec, double *rad, int *j );
-void palSlaDafin ( char *string, int *iptr, double *a, int *j );
+void palDafin ( const char *string, int *iptr, double *a, int *j );
-double palSlaDat ( double dju );
+double palDat ( double dju );
-void palSlaDav2m ( double axvec[3], double rmat[3][3] );
+void palDav2m ( double axvec[3], double rmat[3][3] );
-double palSlaDbear ( double a1, double b1, double a2, double b2 );
+double palDbear ( double a1, double b1, double a2, double b2 );
-void palSlaDbjin ( char *string, int *nstrt,
+void palDbjin ( const char *string, int *nstrt,
double *dreslt, int *jf1, int *jf2 );
-void palSlaDc62s ( double v[6], double *a, double *b, double *r,
+void palDc62s ( double v[6], double *a, double *b, double *r,
double *ad, double *bd, double *rd );
-void palSlaDcc2s ( double v[3], double *a, double *b );
+void palDcc2s ( double v[3], double *a, double *b );
-void palSlaDcmpf ( double coeffs[6], double *xz, double *yz, double *xs,
+void palDcmpf ( double coeffs[6], double *xz, double *yz, double *xs,
double *ys, double *perp, double *orient );
-void palSlaDcs2c ( double a, double b, double v[3] );
+void palDcs2c ( double a, double b, double v[3] );
-void palSlaDd2tf ( int ndp, double days, char *sign, int ihmsf[4] );
+void palDd2tf ( int ndp, double days, char *sign, int ihmsf[4] );
-void palSlaDe2h ( double ha, double dec, double phi, double diurab,
+void palDe2h ( double ha, double dec, double phi,
double *az, double *el );
-void palSlaDeuler ( char *order, double phi, double theta, double psi,
+void palDeuler ( const char *order, double phi, double theta, double psi,
double rmat[3][3] );
-void palSlaDfltin ( char *string, int *nstrt, double *dreslt, int *jflag );
+void palDfltin ( const char *string, int *nstrt, double *dreslt, int *jflag );
-void palSlaDh2e( double az, double el, double phi, double diurab, double *ha,
- double *dec);
+void palDh2e ( double az, double el, double phi, double *ha, double *dec);
-void palSlaDimxv ( double dm[3][3], double va[3], double vb[3] );
+void palDimxv ( double dm[3][3], double va[3], double vb[3] );
-void palSlaDjcal ( int ndp, double djm, int iymdf[4], int *j );
+void palDjcal ( int ndp, double djm, int iymdf[4], int *j );
-void palSlaDjcl ( double djm, int *iy, int *im, int *id, double *fd, int *j );
+void palDjcl ( double djm, int *iy, int *im, int *id, double *fd, int *j );
-void palSlaDm2av ( double rmat[3][3], double axvec[3] );
+void palDm2av ( double rmat[3][3], double axvec[3] );
-void palSlaDmat ( int n, double *a, double *y, double *d, int *jf, int *iw );
+void palDmat ( int n, double *a, double *y, double *d, int *jf, int *iw );
-void palSlaDmoon ( double date, double pv[6] );
+void palDmoon ( double date, double pv[6] );
-void palSlaDmxm ( double a[3][3], double b[3][3], double c[3][3] );
+void palDmxm ( double a[3][3], double b[3][3], double c[3][3] );
-void palSlaDmxv ( double dm[3][3], double va[3], double vb[3] );
+void palDmxv ( double dm[3][3], double va[3], double vb[3] );
-double palSlaDpav ( double v1[3], double v2[3] );
+double palDpav ( double v1[3], double v2[3] );
-void palSlaDr2af ( int ndp, double angle, char *sign, int idmsf[4] );
+void palDr2af ( int ndp, double angle, char *sign, int idmsf[4] );
-void palSlaDr2tf ( int ndp, double angle, char *sign, int ihmsf[4] );
+void palDr2tf ( int ndp, double angle, char *sign, int ihmsf[4] );
-double palSlaDrange ( double angle );
+double palDrange ( double angle );
-double palSlaDranrm ( double angle );
+double palDranrm ( double angle );
-void palSlaDs2c6 ( double a, double b, double r, double ad, double bd,
+void palDs2c6 ( double a, double b, double r, double ad, double bd,
double rd, double v[6] );
-void palSlaDs2tp ( double ra, double dec, double raz, double decz,
+void palDs2tp ( double ra, double dec, double raz, double decz,
double *xi, double *eta, int *j );
-double palSlaDsep ( double a1, double b1, double a2, double b2 );
+double palDsep ( double a1, double b1, double a2, double b2 );
-double palSlaDsepv ( double v1[3], double v2[3] );
+double palDsepv ( double v1[3], double v2[3] );
-double palSlaDt ( double epoch );
+double palDt ( double epoch );
-void palSlaDtf2d ( int ihour, int imin, double sec, double *days, int *j );
+void palDtf2d ( int ihour, int imin, double sec, double *days, int *j );
-void palSlaDtf2r ( int ihour, int imin, double sec, double *rad, int *j );
+void palDtf2r ( int ihour, int imin, double sec, double *rad, int *j );
-void palSlaDtp2s ( double xi, double eta, double raz, double decz,
+void palDtp2s ( double xi, double eta, double raz, double decz,
double *ra, double *dec );
-void palSlaDtp2v ( double xi, double eta, double v0[3], double v[3] );
+void palDtp2v ( double xi, double eta, double v0[3], double v[3] );
-void palSlaDtps2c ( double xi, double eta, double ra, double dec,
+void palDtps2c ( double xi, double eta, double ra, double dec,
double *raz1, double *decz1,
double *raz2, double *decz2, int *n );
-void palSlaDtpv2c ( double xi, double eta, double v[3],
+void palDtpv2c ( double xi, double eta, double v[3],
double v01[3], double v02[3], int *n );
-double palSlaDtt ( double dju );
+double palDtt ( double dju );
-void palSlaDv2tp ( double v[3], double v0[3], double *xi, double *eta, int *j );
+void palDv2tp ( double v[3], double v0[3], double *xi, double *eta, int *j );
-double palSlaDvdv ( double va[3], double vb[3] );
+double palDvdv ( double va[3], double vb[3] );
-void palSlaDvn ( double v[3], double uv[3], double *vm );
+void palDvn ( double v[3], double uv[3], double *vm );
-void palSlaDvxv ( double va[3], double vb[3], double vc[3] );
+void palDvxv ( double va[3], double vb[3], double vc[3] );
-void palSlaE2h ( float ha, float dec, float phi, float *az, float *el );
+void palE2h ( float ha, float dec, float phi, float *az, float *el );
-void palSlaEarth ( int iy, int id, float fd, float posvel[6] );
+void palEarth ( int iy, int id, float fd, float posvel[6] );
-void palSlaEcleq ( double dl, double db, double date, double *dr, double *dd );
+void palEcleq ( double dl, double db, double date, double *dr, double *dd );
-void palSlaEcmat ( double date, double rmat[3][3] );
+void palEcmat ( double date, double rmat[3][3] );
-void palSlaEcor ( float rm, float dm, int iy, int id, float fd,
+void palEcor ( float rm, float dm, int iy, int id, float fd,
float *rv, float *tl );
-void palSlaEg50 ( double dr, double dd, double *dl, double *db );
+void palEg50 ( double dr, double dd, double *dl, double *db );
-void palSlaEl2ue ( double date, int jform, double epoch, double orbinc,
+void palEl2ue ( double date, int jform, double epoch, double orbinc,
double anode, double perih, double aorq, double e,
double aorl, double dm, double u[], int *jstat );
-double palSlaEpb ( double date );
+double palEpb ( double date );
-double palSlaEpb2d ( double epb );
+double palEpb2d ( double epb );
-double palSlaEpco ( char k0, char k, double e );
+double palEpco ( char k0, char k, double e );
-double palSlaEpj ( double date );
+double palEpj ( double date );
-double palSlaEpj2d ( double epj );
+double palEpj2d ( double epj );
-void palSlaEqecl ( double dr, double dd, double date, double *dl, double *db );
+void palEqecl ( double dr, double dd, double date, double *dl, double *db );
-double palSlaEqeqx ( double date );
+double palEqeqx ( double date );
-void palSlaEqgal ( double dr, double dd, double *dl, double *db );
+void palEqgal ( double dr, double dd, double *dl, double *db );
-void palSlaEtrms ( double ep, double ev[3] );
+void palEtrms ( double ep, double ev[3] );
-void palSlaEuler ( char *order, float phi, float theta, float psi,
+void palEuler ( const char *order, float phi, float theta, float psi,
float rmat[3][3] );
-void palSlaEvp ( double date, double deqx,
+void palEvp ( double date, double deqx,
double dvb[3], double dpb[3],
double dvh[3], double dph[3] );
-void palSlaFitxy ( int itype, int np, double xye[][2], double xym[][2],
+void palFitxy ( int itype, int np, double xye[][2], double xym[][2],
double coeffs[6], int *j );
-void palSlaFk425 ( double r1950, double d1950, double dr1950,
+void palFk425 ( double r1950, double d1950, double dr1950,
double dd1950, double p1950, double v1950,
double *r2000, double *d2000, double *dr2000,
double *dd2000, double *p2000, double *v2000 );
-void palSlaFk45z ( double r1950, double d1950, double bepoch,
+void palFk45z ( double r1950, double d1950, double bepoch,
double *r2000, double *d2000 );
-void palSlaFk524 ( double r2000, double d2000, double dr2000,
+void palFk524 ( double r2000, double d2000, double dr2000,
double dd2000, double p2000, double v2000,
double *r1950, double *d1950, double *dr1950,
double *dd1950, double *p1950, double *v1950 );
-void palSlaFk52h ( double r5, double d5, double dr5, double dd5,
+void palFk52h ( double r5, double d5, double dr5, double dd5,
double *dr, double *dh, double *drh, double *ddh );
-void palSlaFk54z ( double r2000, double d2000, double bepoch,
+void palFk54z ( double r2000, double d2000, double bepoch,
double *r1950, double *d1950,
double *dr1950, double *dd1950 );
-void palSlaFk5hz ( double r5, double d5, double epoch,
+void palFk5hz ( double r5, double d5, double epoch,
double *rh, double *dh );
-void palSlaFlotin ( char *string, int *nstrt, float *reslt, int *jflag );
+void palFlotin ( const char *string, int *nstrt, float *reslt, int *jflag );
-void palSlaGaleq ( double dl, double db, double *dr, double *dd );
+void palGaleq ( double dl, double db, double *dr, double *dd );
-void palSlaGalsup ( double dl, double db, double *dsl, double *dsb );
+void palGalsup ( double dl, double db, double *dsl, double *dsb );
-void palSlaGe50 ( double dl, double db, double *dr, double *dd );
+void palGe50 ( double dl, double db, double *dr, double *dd );
-void palSlaGeoc ( double p, double h, double *r, double *z );
+void palGeoc ( double p, double h, double *r, double *z );
-double palSlaGmst ( double ut1 );
+double palGmst ( double ut1 );
-double palSlaGmsta ( double date, double ut1 );
+double palGmsta ( double date, double ut1 );
-void palSlaH2e ( float az, float el, float phi, float *ha, float *dec );
+void palH2e ( float az, float el, float phi, float *ha, float *dec );
-void palSlaH2fk5 ( double dr, double dh, double drh, double ddh,
+void palH2fk5 ( double dr, double dh, double drh, double ddh,
double *r5, double *d5, double *dr5, double *dd5 );
-void palSlaHfk5z ( double rh, double dh, double epoch,
+void palHfk5z ( double rh, double dh, double epoch,
double *r5, double *d5, double *dr5, double *dd5 );
-void palSlaImxv ( float rm[3][3], float va[3], float vb[3] );
+void palImxv ( float rm[3][3], float va[3], float vb[3] );
-void palSlaInt2in ( char *string, int *nstrt, int *ireslt, int *jflag );
+void palInt2in ( const char *string, int *nstrt, int *ireslt, int *jflag );
-void palSlaIntin ( char *string, int *nstrt, long *ireslt, int *jflag );
+void palIntin ( const char *string, int *nstrt, long *ireslt, int *jflag );
-void palSlaInvf ( double fwds[6], double bkwds[6], int *j );
+void palInvf ( double fwds[6], double bkwds[6], int *j );
-void palSlaKbj ( int jb, double e, char *k, int *j );
+void palKbj ( int jb, double e, char *k, int *j );
-void palSlaM2av ( float rmat[3][3], float axvec[3] );
+void palM2av ( float rmat[3][3], float axvec[3] );
-void palSlaMap ( double rm, double dm, double pr, double pd,
+void palMap ( double rm, double dm, double pr, double pd,
double px, double rv, double eq, double date,
double *ra, double *da );
-void palSlaMappa ( double eq, double date, double amprms[21] );
+void palMappa ( double eq, double date, double amprms[21] );
-void palSlaMapqk ( double rm, double dm, double pr, double pd,
+void palMapqk ( double rm, double dm, double pr, double pd,
double px, double rv, double amprms[21],
double *ra, double *da );
-void palSlaMapqkz ( double rm, double dm, double amprms[21],
+void palMapqkz ( double rm, double dm, double amprms[21],
double *ra, double *da );
-void palSlaMoon ( int iy, int id, float fd, float posvel[6] );
+void palMoon ( int iy, int id, float fd, float posvel[6] );
-void palSlaMxm ( float a[3][3], float b[3][3], float c[3][3] );
+void palMxm ( float a[3][3], float b[3][3], float c[3][3] );
-void palSlaMxv ( float rm[3][3], float va[3], float vb[3] );
+void palMxv ( float rm[3][3], float va[3], float vb[3] );
-void palSlaNut ( double date, double rmatn[3][3] );
+void palNut ( double date, double rmatn[3][3] );
-void palSlaNutc ( double date, double *dpsi, double *deps, double *eps0 );
+void palNutc ( double date, double *dpsi, double *deps, double *eps0 );
-void palSlaNutc80 ( double date, double *dpsi, double *deps, double *eps0 );
+void palNutc80 ( double date, double *dpsi, double *deps, double *eps0 );
-void palSlaOap ( char *type, double ob1, double ob2, double date,
+void palOap ( const char *type, double ob1, double ob2, double date,
double dut, double elongm, double phim, double hm,
double xp, double yp, double tdk, double pmb,
double rh, double wl, double tlr,
double *rap, double *dap );
-void palSlaOapqk ( char *type, double ob1, double ob2, double aoprms[14],
+void palOapqk ( const char *type, double ob1, double ob2, double aoprms[14],
double *rap, double *dap );
-void palSlaObs ( int n, char *c, char *name, double *w, double *p, double *h );
+void palObs ( int n, char *c, char *name, double *w, double *p, double *h );
-double palSlaPa ( double ha, double dec, double phi );
+double palPa ( double ha, double dec, double phi );
-double palSlaPav ( float v1[3], float v2[3] );
+double palPav ( float v1[3], float v2[3] );
-void palSlaPcd ( double disco, double *x, double *y );
+void palPcd ( double disco, double *x, double *y );
-void palSlaPda2h ( double p, double d, double a,
+void palPda2h ( double p, double d, double a,
double *h1, int *j1, double *h2, int *j2 );
-void palSlaPdq2h ( double p, double d, double q,
+void palPdq2h ( double p, double d, double q,
double *h1, int *j1, double *h2, int *j2 );
-void palSlaPermut ( int n, int istate[], int iorder[], int *j );
+void palPermut ( int n, int istate[], int iorder[], int *j );
-void palSlaPertel (int jform, double date0, double date1,
+void palPertel (int jform, double date0, double date1,
double epoch0, double orbi0, double anode0,
double perih0, double aorq0, double e0, double am0,
double *epoch1, double *orbi1, double *anode1,
double *perih1, double *aorq1, double *e1, double *am1,
int *jstat );
-void palSlaPertue ( double date, double u[], int *jstat );
+void palPertue ( double date, double u[], int *jstat );
-void palSlaPlanel ( double date, int jform, double epoch, double orbinc,
+void palPlanel ( double date, int jform, double epoch, double orbinc,
double anode, double perih, double aorq, double e,
double aorl, double dm, double pv[6], int *jstat );
-void palSlaPlanet ( double date, int np, double pv[6], int *j );
+void palPlanet ( double date, int np, double pv[6], int *j );
-void palSlaPlante ( double date, double elong, double phi, int jform,
+void palPlante ( double date, double elong, double phi, int jform,
double epoch, double orbinc, double anode, double perih,
double aorq, double e, double aorl, double dm,
double *ra, double *dec, double *r, int *jstat );
-void palSlaPlantu ( double date, double elong, double phi, double u[],
+void palPlantu ( double date, double elong, double phi, double u[],
double *ra, double *dec, double *r, int *jstat );
-void palSlaPm ( double r0, double d0, double pr, double pd,
+void palPm ( double r0, double d0, double pr, double pd,
double px, double rv, double ep0, double ep1,
double *r1, double *d1 );
-void palSlaPolmo ( double elongm, double phim, double xp, double yp,
+void palPolmo ( double elongm, double phim, double xp, double yp,
double *elong, double *phi, double *daz );
-void palSlaPrebn ( double bep0, double bep1, double rmatp[3][3] );
+void palPrebn ( double bep0, double bep1, double rmatp[3][3] );
-void palSlaPrec ( double ep0, double ep1, double rmatp[3][3] );
+void palPrec ( double ep0, double ep1, double rmatp[3][3] );
-void palSlaPrecl ( double ep0, double ep1, double rmatp[3][3] );
+void palPrecl ( double ep0, double ep1, double rmatp[3][3] );
-void palSlaPreces ( char sys[3], double ep0, double ep1,
+void palPreces ( const char sys[3], double ep0, double ep1,
double *ra, double *dc );
-void palSlaPrenut ( double epoch, double date, double rmatpn[3][3] );
+void palPrenut ( double epoch, double date, double rmatpn[3][3] );
-void palSlaPv2el ( double pv[], double date, double pmass, int jformr,
+void palPv2el ( double pv[], double date, double pmass, int jformr,
int *jform, double *epoch, double *orbinc,
double *anode, double *perih, double *aorq, double *e,
double *aorl, double *dm, int *jstat );
-void palSlaPv2ue ( double pv[], double date, double pmass,
+void palPv2ue ( double pv[], double date, double pmass,
double u[], int *jstat );
-void palSlaPvobs ( double p, double h, double stl, double pv[6] );
+void palPvobs ( double p, double h, double stl, double pv[6] );
-void palSlaPxy ( int np, double xye[][2], double xym[][2],
+void palPxy ( int np, double xye[][2], double xym[][2],
double coeffs[6],
double xyp[][2], double *xrms, double *yrms, double *rrms );
-float palSlaRange ( float angle );
+float palRange ( float angle );
-float palSlaRanorm ( float angle );
+float palRanorm ( float angle );
-double palSlaRcc ( double tdb, double ut1, double wl, double u, double v );
+double palRcc ( double tdb, double ut1, double wl, double u, double v );
-void palSlaRdplan ( double date, int np, double elong, double phi,
+void palRdplan ( double date, int np, double elong, double phi,
double *ra, double *dec, double *diam );
-void palSlaRefco ( double hm, double tdk, double pmb, double rh,
+void palRefco ( double hm, double tdk, double pmb, double rh,
double wl, double phi, double tlr, double eps,
double *refa, double *refb );
-void palSlaRefcoq ( double tdk, double pmb, double rh, double wl,
+void palRefcoq ( double tdk, double pmb, double rh, double wl,
double *refa, double *refb );
-void palSlaRefro ( double zobs, double hm, double tdk, double pmb,
+void palRefro ( double zobs, double hm, double tdk, double pmb,
double rh, double wl, double phi, double tlr, double eps,
double *ref );
-void palSlaRefv ( double vu[3], double refa, double refb, double vr[3] );
+void palRefv ( double vu[3], double refa, double refb, double vr[3] );
-void palSlaRefz ( double zu, double refa, double refb, double *zr );
+void palRefz ( double zu, double refa, double refb, double *zr );
-float palSlaRverot ( float phi, float ra, float da, float st );
+float palRverot ( float phi, float ra, float da, float st );
-float palSlaRvgalc ( float r2000, float d2000 );
+double palRvgalc ( double r2000, double d2000 );
-float palSlaRvlg ( float r2000, float d2000 );
+double palRvlg ( double r2000, double d2000 );
-float palSlaRvlsrd ( float r2000, float d2000 );
+double palRvlsrd ( double r2000, double d2000 );
-float palSlaRvlsrk ( float r2000, float d2000 );
+double palRvlsrk ( double r2000, double d2000 );
-void palSlaS2tp ( float ra, float dec, float raz, float decz,
+void palS2tp ( float ra, float dec, float raz, float decz,
float *xi, float *eta, int *j );
-float palSlaSep ( float a1, float b1, float a2, float b2 );
+float palSep ( float a1, float b1, float a2, float b2 );
-float palSlaSepv ( float v1[3], float v2[3] );
+float palSepv ( float v1[3], float v2[3] );
-void palSlaSmat ( int n, float *a, float *y, float *d, int *jf, int *iw );
+void palSmat ( int n, float *a, float *y, float *d, int *jf, int *iw );
-void palSlaSubet ( double rc, double dc, double eq,
+void palSubet ( double rc, double dc, double eq,
double *rm, double *dm );
-void palSlaSupgal ( double dsl, double dsb, double *dl, double *db );
+void palSupgal ( double dsl, double dsb, double *dl, double *db );
-void palSlaSvd ( int m, int n, int mp, int np,
+void palSvd ( int m, int n, int mp, int np,
double *a, double *w, double *v, double *work,
int *jstat );
-void palSlaSvdcov ( int n, int np, int nc,
+void palSvdcov ( int n, int np, int nc,
double *w, double *v, double *work, double *cvm );
-void palSlaSvdsol ( int m, int n, int mp, int np,
+void palSvdsol ( int m, int n, int mp, int np,
double *b, double *u, double *w, double *v,
double *work, double *x );
-void palSlaTp2s ( float xi, float eta, float raz, float decz,
+void palTp2s ( float xi, float eta, float raz, float decz,
float *ra, float *dec );
-void palSlaTp2v ( float xi, float eta, float v0[3], float v[3] );
+void palTp2v ( float xi, float eta, float v0[3], float v[3] );
-void palSlaTps2c ( float xi, float eta, float ra, float dec,
+void palTps2c ( float xi, float eta, float ra, float dec,
float *raz1, float *decz1,
float *raz2, float *decz2, int *n );
-void palSlaTpv2c ( float xi, float eta, float v[3],
+void palTpv2c ( float xi, float eta, float v[3],
float v01[3], float v02[3], int *n );
-void palSlaUe2el ( double u[], int jformr,
+void palUe2el ( double u[], int jformr,
int *jform, double *epoch, double *orbinc,
double *anode, double *perih, double *aorq, double *e,
double *aorl, double *dm, int *jstat );
-void palSlaUe2pv ( double date, double u[], double pv[], int *jstat );
+void palUe2pv ( double date, double u[], double pv[], int *jstat );
-void palSlaUnpcd ( double disco, double *x, double *y );
+void palUnpcd ( double disco, double *x, double *y );
-void palSlaV2tp ( float v[3], float v0[3], float *xi, float *eta, int *j );
+void palV2tp ( float v[3], float v0[3], float *xi, float *eta, int *j );
-float palSlaVdv ( float va[3], float vb[3] );
+float palVdv ( float va[3], float vb[3] );
-void palSlaVn ( float v[3], float uv[3], float *vm );
+void palVn ( float v[3], float uv[3], float *vm );
-void palSlaVxv ( float va[3], float vb[3], float vc[3] );
+void palVxv ( float va[3], float vb[3], float vc[3] );
-void palSlaXy2xy ( double x1, double y1, double coeffs[6],
+void palXy2xy ( double x1, double y1, double coeffs[6],
double *x2, double *y2 );
-double palSlaZd ( double ha, double dec, double phi );
+double palZd ( double ha, double dec, double phi );
#ifdef __cplusplus
}
diff --git a/pal/pal.h b/pal/pal.h
new file mode 100644
index 0000000..482694f
--- /dev/null
+++ b/pal/pal.h
@@ -0,0 +1,541 @@
+#ifndef PALHDEF
+#define PALHDEF
+
+/*
+*+
+* Name:
+* pal.h
+
+* Purpose:
+* Function prototypes for PAL routines.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Include file
+
+* Description:
+* Function prototypes for PAL routines.
+
+* Authors:
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* Notes:
+*
+
+* History:
+* 2012-02-08 (TIMJ):
+* Initial version. Define all SLA prototypes in PAL form even
+* though none are implemented.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#ifdef __cplusplus
+extern "C" {
+#endif
+
+#include <math.h>
+
+void palAddet ( double rm, double dm, double eq, double *rc, double *dc );
+
+void palAfin ( const char *string, int *iptr, float *a, int *j );
+
+double palAirmas ( double zd );
+
+void palAltaz ( double ha, double dec, double phi,
+ double *az, double *azd, double *azdd,
+ double *el, double *eld, double *eldd,
+ double *pa, double *pad, double *padd );
+
+void palAmp ( double ra, double da, double date, double eq,
+ double *rm, double *dm );
+
+void palAmpqk ( double ra, double da, double amprms[21],
+ double *rm, double *dm );
+
+void palAop ( double rap, double dap, double date, double dut,
+ double elongm, double phim, double hm, double xp,
+ double yp, double tdk, double pmb, double rh,
+ double wl, double tlr,
+ double *aob, double *zob, double *hob,
+ double *dob, double *rob );
+
+void palAoppa ( double date, double dut, double elongm, double phim,
+ double hm, double xp, double yp, double tdk, double pmb,
+ double rh, double wl, double tlr, double aoprms[14] );
+
+void palAoppat ( double date, double aoprms[14] );
+
+void palAopqk ( double rap, double dap, double aoprms[14],
+ double *aob, double *zob, double *hob,
+ double *dob, double *rob );
+
+void palAtmdsp ( double tdk, double pmb, double rh, double wl1,
+ double a1, double b1, double wl2, double *a2, double *b2 );
+
+void palAv2m ( float axvec[3], float rmat[3][3] );
+
+float palBear ( float a1, float b1, float a2, float b2 );
+
+void palCaf2r ( int ideg, int iamin, float asec, float *rad, int *j );
+
+void palCaldj ( int iy, int im, int id, double *djm, int *j );
+
+void palCalyd ( int iy, int im, int id, int *ny, int *nd, int *j );
+
+void palCc2s ( float v[3], float *a, float *b );
+
+void palCc62s ( float v[6], float *a, float *b, float *r,
+ float *ad, float *bd, float *rd );
+
+void palCd2tf ( int ndp, float days, char *sign, int ihmsf[4] );
+
+void palCldj ( int iy, int im, int id, double *djm, int *j );
+
+void palClyd ( int iy, int im, int id, int *ny, int *nd, int *jstat );
+
+void palCombn ( int nsel, int ncand, int list[], int *j );
+
+void palCr2af ( int ndp, float angle, char *sign, int idmsf[4] );
+
+void palCr2tf ( int ndp, float angle, char *sign, int ihmsf[4] );
+
+void palCs2c ( float a, float b, float v[3] );
+
+void palCs2c6 ( float a, float b, float r, float ad,
+ float bd, float rd, float v[6] );
+
+void palCtf2d ( int ihour, int imin, float sec, float *days, int *j );
+
+void palCtf2r ( int ihour, int imin, float sec, float *rad, int *j );
+
+void palDaf2r ( int ideg, int iamin, double asec, double *rad, int *j );
+
+void palDafin ( const char *string, int *iptr, double *a, int *j );
+
+double palDat ( double dju );
+
+void palDav2m ( double axvec[3], double rmat[3][3] );
+
+double palDbear ( double a1, double b1, double a2, double b2 );
+
+void palDbjin ( const char *string, int *nstrt,
+ double *dreslt, int *jf1, int *jf2 );
+
+void palDc62s ( double v[6], double *a, double *b, double *r,
+ double *ad, double *bd, double *rd );
+
+void palDcc2s ( double v[3], double *a, double *b );
+
+void palDcmpf ( double coeffs[6], double *xz, double *yz, double *xs,
+ double *ys, double *perp, double *orient );
+
+void palDcs2c ( double a, double b, double v[3] );
+
+void palDd2tf ( int ndp, double days, char *sign, int ihmsf[4] );
+
+void palDe2h ( double ha, double dec, double phi,
+ double *az, double *el );
+
+void palDeuler ( const char *order, double phi, double theta, double psi,
+ double rmat[3][3] );
+
+void palDfltin ( const char *string, int *nstrt, double *dreslt, int *jflag );
+
+void palDh2e ( double az, double el, double phi, double *ha, double *dec);
+
+void palDimxv ( double dm[3][3], double va[3], double vb[3] );
+
+void palDjcal ( int ndp, double djm, int iymdf[4], int *j );
+
+void palDjcl ( double djm, int *iy, int *im, int *id, double *fd, int *j );
+
+void palDm2av ( double rmat[3][3], double axvec[3] );
+
+void palDmat ( int n, double *a, double *y, double *d, int *jf, int *iw );
+
+void palDmoon ( double date, double pv[6] );
+
+void palDmxm ( double a[3][3], double b[3][3], double c[3][3] );
+
+void palDmxv ( double dm[3][3], double va[3], double vb[3] );
+
+double palDpav ( double v1[3], double v2[3] );
+
+void palDr2af ( int ndp, double angle, char *sign, int idmsf[4] );
+
+void palDr2tf ( int ndp, double angle, char *sign, int ihmsf[4] );
+
+double palDrange ( double angle );
+
+double palDranrm ( double angle );
+
+void palDs2c6 ( double a, double b, double r, double ad, double bd,
+ double rd, double v[6] );
+
+void palDs2tp ( double ra, double dec, double raz, double decz,
+ double *xi, double *eta, int *j );
+
+double palDsep ( double a1, double b1, double a2, double b2 );
+
+double palDsepv ( double v1[3], double v2[3] );
+
+double palDt ( double epoch );
+
+void palDtf2d ( int ihour, int imin, double sec, double *days, int *j );
+
+void palDtf2r ( int ihour, int imin, double sec, double *rad, int *j );
+
+void palDtp2s ( double xi, double eta, double raz, double decz,
+ double *ra, double *dec );
+
+void palDtp2v ( double xi, double eta, double v0[3], double v[3] );
+
+void palDtps2c ( double xi, double eta, double ra, double dec,
+ double *raz1, double *decz1,
+ double *raz2, double *decz2, int *n );
+
+void palDtpv2c ( double xi, double eta, double v[3],
+ double v01[3], double v02[3], int *n );
+
+double palDtt ( double dju );
+
+void palDv2tp ( double v[3], double v0[3], double *xi, double *eta, int *j );
+
+double palDvdv ( double va[3], double vb[3] );
+
+void palDvn ( double v[3], double uv[3], double *vm );
+
+void palDvxv ( double va[3], double vb[3], double vc[3] );
+
+void palE2h ( float ha, float dec, float phi, float *az, float *el );
+
+void palEarth ( int iy, int id, float fd, float posvel[6] );
+
+void palEcleq ( double dl, double db, double date, double *dr, double *dd );
+
+void palEcmat ( double date, double rmat[3][3] );
+
+void palEcor ( float rm, float dm, int iy, int id, float fd,
+ float *rv, float *tl );
+
+void palEg50 ( double dr, double dd, double *dl, double *db );
+
+void palEl2ue ( double date, int jform, double epoch, double orbinc,
+ double anode, double perih, double aorq, double e,
+ double aorl, double dm, double u[], int *jstat );
+
+double palEpb ( double date );
+
+double palEpb2d ( double epb );
+
+double palEpco ( char k0, char k, double e );
+
+double palEpj ( double date );
+
+double palEpj2d ( double epj );
+
+void palEqecl ( double dr, double dd, double date, double *dl, double *db );
+
+double palEqeqx ( double date );
+
+void palEqgal ( double dr, double dd, double *dl, double *db );
+
+void palEtrms ( double ep, double ev[3] );
+
+void palEuler ( const char *order, float phi, float theta, float psi,
+ float rmat[3][3] );
+
+void palEvp ( double date, double deqx,
+ double dvb[3], double dpb[3],
+ double dvh[3], double dph[3] );
+
+void palFitxy ( int itype, int np, double xye[][2], double xym[][2],
+ double coeffs[6], int *j );
+
+void palFk425 ( double r1950, double d1950, double dr1950,
+ double dd1950, double p1950, double v1950,
+ double *r2000, double *d2000, double *dr2000,
+ double *dd2000, double *p2000, double *v2000 );
+
+void palFk45z ( double r1950, double d1950, double bepoch,
+ double *r2000, double *d2000 );
+
+void palFk524 ( double r2000, double d2000, double dr2000,
+ double dd2000, double p2000, double v2000,
+ double *r1950, double *d1950, double *dr1950,
+ double *dd1950, double *p1950, double *v1950 );
+
+void palFk52h ( double r5, double d5, double dr5, double dd5,
+ double *dr, double *dh, double *drh, double *ddh );
+
+void palFk54z ( double r2000, double d2000, double bepoch,
+ double *r1950, double *d1950,
+ double *dr1950, double *dd1950 );
+
+void palFk5hz ( double r5, double d5, double epoch,
+ double *rh, double *dh );
+
+void palFlotin ( const char *string, int *nstrt, float *reslt, int *jflag );
+
+void palGaleq ( double dl, double db, double *dr, double *dd );
+
+void palGalsup ( double dl, double db, double *dsl, double *dsb );
+
+void palGe50 ( double dl, double db, double *dr, double *dd );
+
+void palGeoc ( double p, double h, double *r, double *z );
+
+double palGmst ( double ut1 );
+
+double palGmsta ( double date, double ut1 );
+
+void palH2e ( float az, float el, float phi, float *ha, float *dec );
+
+void palH2fk5 ( double dr, double dh, double drh, double ddh,
+ double *r5, double *d5, double *dr5, double *dd5 );
+
+void palHfk5z ( double rh, double dh, double epoch,
+ double *r5, double *d5, double *dr5, double *dd5 );
+
+void palImxv ( float rm[3][3], float va[3], float vb[3] );
+
+void palInt2in ( const char *string, int *nstrt, int *ireslt, int *jflag );
+
+void palIntin ( const char *string, int *nstrt, long *ireslt, int *jflag );
+
+void palInvf ( double fwds[6], double bkwds[6], int *j );
+
+void palKbj ( int jb, double e, char *k, int *j );
+
+void palM2av ( float rmat[3][3], float axvec[3] );
+
+void palMap ( double rm, double dm, double pr, double pd,
+ double px, double rv, double eq, double date,
+ double *ra, double *da );
+
+void palMappa ( double eq, double date, double amprms[21] );
+
+void palMapqk ( double rm, double dm, double pr, double pd,
+ double px, double rv, double amprms[21],
+ double *ra, double *da );
+
+void palMapqkz ( double rm, double dm, double amprms[21],
+ double *ra, double *da );
+
+void palMoon ( int iy, int id, float fd, float posvel[6] );
+
+void palMxm ( float a[3][3], float b[3][3], float c[3][3] );
+
+void palMxv ( float rm[3][3], float va[3], float vb[3] );
+
+void palNut ( double date, double rmatn[3][3] );
+
+void palNutc ( double date, double *dpsi, double *deps, double *eps0 );
+
+void palNutc80 ( double date, double *dpsi, double *deps, double *eps0 );
+
+void palOap ( const char *type, double ob1, double ob2, double date,
+ double dut, double elongm, double phim, double hm,
+ double xp, double yp, double tdk, double pmb,
+ double rh, double wl, double tlr,
+ double *rap, double *dap );
+
+void palOapqk ( const char *type, double ob1, double ob2, double aoprms[14],
+ double *rap, double *dap );
+
+void palObs ( int n, char *c, char *name, double *w, double *p, double *h );
+
+double palPa ( double ha, double dec, double phi );
+
+double palPav ( float v1[3], float v2[3] );
+
+void palPcd ( double disco, double *x, double *y );
+
+void palPda2h ( double p, double d, double a,
+ double *h1, int *j1, double *h2, int *j2 );
+
+void palPdq2h ( double p, double d, double q,
+ double *h1, int *j1, double *h2, int *j2 );
+
+void palPermut ( int n, int istate[], int iorder[], int *j );
+
+void palPertel (int jform, double date0, double date1,
+ double epoch0, double orbi0, double anode0,
+ double perih0, double aorq0, double e0, double am0,
+ double *epoch1, double *orbi1, double *anode1,
+ double *perih1, double *aorq1, double *e1, double *am1,
+ int *jstat );
+
+void palPertue ( double date, double u[], int *jstat );
+
+void palPlanel ( double date, int jform, double epoch, double orbinc,
+ double anode, double perih, double aorq, double e,
+ double aorl, double dm, double pv[6], int *jstat );
+
+void palPlanet ( double date, int np, double pv[6], int *j );
+
+void palPlante ( double date, double elong, double phi, int jform,
+ double epoch, double orbinc, double anode, double perih,
+ double aorq, double e, double aorl, double dm,
+ double *ra, double *dec, double *r, int *jstat );
+
+void palPlantu ( double date, double elong, double phi, double u[],
+ double *ra, double *dec, double *r, int *jstat );
+
+void palPm ( double r0, double d0, double pr, double pd,
+ double px, double rv, double ep0, double ep1,
+ double *r1, double *d1 );
+
+void palPolmo ( double elongm, double phim, double xp, double yp,
+ double *elong, double *phi, double *daz );
+
+void palPrebn ( double bep0, double bep1, double rmatp[3][3] );
+
+void palPrec ( double ep0, double ep1, double rmatp[3][3] );
+
+void palPrecl ( double ep0, double ep1, double rmatp[3][3] );
+
+void palPreces ( const char sys[3], double ep0, double ep1,
+ double *ra, double *dc );
+
+void palPrenut ( double epoch, double date, double rmatpn[3][3] );
+
+void palPv2el ( double pv[], double date, double pmass, int jformr,
+ int *jform, double *epoch, double *orbinc,
+ double *anode, double *perih, double *aorq, double *e,
+ double *aorl, double *dm, int *jstat );
+
+void palPv2ue ( double pv[], double date, double pmass,
+ double u[], int *jstat );
+
+void palPvobs ( double p, double h, double stl, double pv[6] );
+
+void palPxy ( int np, double xye[][2], double xym[][2],
+ double coeffs[6],
+ double xyp[][2], double *xrms, double *yrms, double *rrms );
+
+float palRange ( float angle );
+
+float palRanorm ( float angle );
+
+double palRcc ( double tdb, double ut1, double wl, double u, double v );
+
+void palRdplan ( double date, int np, double elong, double phi,
+ double *ra, double *dec, double *diam );
+
+void palRefco ( double hm, double tdk, double pmb, double rh,
+ double wl, double phi, double tlr, double eps,
+ double *refa, double *refb );
+
+void palRefcoq ( double tdk, double pmb, double rh, double wl,
+ double *refa, double *refb );
+
+void palRefro ( double zobs, double hm, double tdk, double pmb,
+ double rh, double wl, double phi, double tlr, double eps,
+ double *ref );
+
+void palRefv ( double vu[3], double refa, double refb, double vr[3] );
+
+void palRefz ( double zu, double refa, double refb, double *zr );
+
+float palRverot ( float phi, float ra, float da, float st );
+
+double palRvgalc ( double r2000, double d2000 );
+
+double palRvlg ( double r2000, double d2000 );
+
+double palRvlsrd ( double r2000, double d2000 );
+
+double palRvlsrk ( double r2000, double d2000 );
+
+void palS2tp ( float ra, float dec, float raz, float decz,
+ float *xi, float *eta, int *j );
+
+float palSep ( float a1, float b1, float a2, float b2 );
+
+float palSepv ( float v1[3], float v2[3] );
+
+void palSmat ( int n, float *a, float *y, float *d, int *jf, int *iw );
+
+void palSubet ( double rc, double dc, double eq,
+ double *rm, double *dm );
+
+void palSupgal ( double dsl, double dsb, double *dl, double *db );
+
+void palSvd ( int m, int n, int mp, int np,
+ double *a, double *w, double *v, double *work,
+ int *jstat );
+
+void palSvdcov ( int n, int np, int nc,
+ double *w, double *v, double *work, double *cvm );
+
+void palSvdsol ( int m, int n, int mp, int np,
+ double *b, double *u, double *w, double *v,
+ double *work, double *x );
+
+void palTp2s ( float xi, float eta, float raz, float decz,
+ float *ra, float *dec );
+
+void palTp2v ( float xi, float eta, float v0[3], float v[3] );
+
+void palTps2c ( float xi, float eta, float ra, float dec,
+ float *raz1, float *decz1,
+ float *raz2, float *decz2, int *n );
+
+void palTpv2c ( float xi, float eta, float v[3],
+ float v01[3], float v02[3], int *n );
+
+void palUe2el ( double u[], int jformr,
+ int *jform, double *epoch, double *orbinc,
+ double *anode, double *perih, double *aorq, double *e,
+ double *aorl, double *dm, int *jstat );
+
+void palUe2pv ( double date, double u[], double pv[], int *jstat );
+
+void palUnpcd ( double disco, double *x, double *y );
+
+void palV2tp ( float v[3], float v0[3], float *xi, float *eta, int *j );
+
+float palVdv ( float va[3], float vb[3] );
+
+void palVn ( float v[3], float uv[3], float *vm );
+
+void palVxv ( float va[3], float vb[3], float vc[3] );
+
+void palXy2xy ( double x1, double y1, double coeffs[6],
+ double *x2, double *y2 );
+
+double palZd ( double ha, double dec, double phi );
+
+#ifdef __cplusplus
+}
+#endif
+
+#endif
diff --git a/pal/palAddet.c b/pal/palAddet.c
new file mode 100644
index 0000000..54c26c1
--- /dev/null
+++ b/pal/palAddet.c
@@ -0,0 +1,109 @@
+/*
+*+
+* Name:
+* palAddet
+
+* Purpose:
+* Add the E-terms to a pre IAU 1976 mean place
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palAddet ( double rm, double dm, double eq,
+* double *rc, double *dc );
+
+* Arguments:
+* rm = double (Given)
+* RA without E-terms (radians)
+* dm = double (Given)
+* Dec without E-terms (radians)
+* eq = double (Given)
+* Besselian epoch of mean equator and equinox
+* rc = double * (Returned)
+* RA with E-terms included (radians)
+* dc = double * (Returned)
+* Dec with E-terms included (radians)
+
+* Description:
+* Add the E-terms (elliptic component of annual aberration)
+* to a pre IAU 1976 mean place to conform to the old
+* catalogue convention.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* Notes:
+* Most star positions from pre-1984 optical catalogues (or
+* derived from astrometry using such stars) embody the
+* E-terms. If it is necessary to convert a formal mean
+* place (for example a pulsar timing position) to one
+* consistent with such a star catalogue, then the RA,Dec
+* should be adjusted using this routine.
+
+* See Also:
+* Explanatory Supplement to the Astronomical Ephemeris,
+* section 2D, page 48.
+
+* History:
+* 2012-02-12(TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+void palAddet ( double rm, double dm, double eq, double *rc, double *dc ) {
+ double a[3]; /* The E-terms */
+ double v[3];
+ int i;
+
+ /* Note the preference for IAU routines */
+
+ /* Retrieve the E-terms */
+ palEtrms( eq, a );
+
+ /* Spherical to Cartesian */
+ iauS2c( rm, dm, v );
+
+ /* Include the E-terms */
+ for (i=0; i<3; i++) {
+ v[i] += a[i];
+ }
+
+ /* Cartesian to spherical */
+ iauC2s( v, rc, dc );
+
+ /* Bring RA into conventional range */
+ *rc = iauAnp( *rc );
+
+}
diff --git a/pal/palAmpqk.c b/pal/palAmpqk.c
new file mode 100644
index 0000000..49f2e23
--- /dev/null
+++ b/pal/palAmpqk.c
@@ -0,0 +1,126 @@
+/*
+*+
+* Name:
+* palAmpqk
+
+* Purpose:
+* Convert star RA,Dec from geocentric apparent to mean place.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palAmpqk ( double ra, double da, double amprms[21],
+* double *rm, double *dm )
+
+* Arguments:
+* ra = double (Given)
+* Apparent RA (radians).
+* da = double (Given)
+* Apparent Dec (radians).
+* amprms = double[21] (Given)
+* Star-independent mean-to-apparent parameters (see palMappa):
+* (0) time interval for proper motion (Julian years)
+* (1-3) barycentric position of the Earth (AU)
+* (4-6) not used
+* (7) not used
+* (8-10) abv: barycentric Earth velocity in units of c
+* (11) sqrt(1-v*v) where v=modulus(abv)
+* (12-20) precession/nutation (3,3) matrix
+* rm = double (Returned)
+* Mean RA (radians).
+* dm = double (Returned)
+* Mean Dec (radians).
+
+* Description:
+* Convert star RA,Dec from geocentric apparent to mean place. The "mean"
+* coordinate system is in fact close to ICRS. Use of this function
+* is appropriate when efficiency is important and where many star
+* positions are all to be transformed for one epoch and equinox. The
+* star-independent parameters can be obtained by calling the palMappa
+* function.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-13 (PTW):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+void palAmpqk ( double ra, double da, double amprms[21], double *rm,
+ double *dm ){
+
+/* Local Variables: */
+ double ab1; /* sqrt(1-v*v) where v=modulus of Earth vel */
+ double abv[3]; /* Earth velocity wrt SSB (c, FK5) */
+ double p1[3], p2[3], p3[3]; /* work vectors */
+ double ab1p1, p1dv, p1dvp1, w;
+ int i, j;
+
+/* Unpack some of the parameters */
+ ab1 = amprms[11];
+ for( i = 0; i < 3; i++ ) {
+ abv[i] = amprms[i + 8];
+ }
+
+/* Apparent RA,Dec to Cartesian */
+ iauS2c( ra, da, p3 );
+
+/* Precession and nutation */
+ iauTrxp( (double(*)[3]) &rms[12], p3, p2 );
+
+/* Aberration */
+ ab1p1 = ab1 + 1.0;
+ for( i = 0; i < 3; i++ ) {
+ p1[i] = p2[i];
+ }
+ for( j = 0; j < 2; j++ ) {
+ p1dv = iauPdp( p1, abv );
+ p1dvp1 = 1.0 + p1dv;
+ w = 1.0 + p1dv / ab1p1;
+ for( i = 0; i < 3; i++ ) {
+ p1[i] = ( p1dvp1 * p2[i] - w * abv[i] ) / ab1;
+ }
+ iauPn( p1, &w, p3 );
+ for( i = 0; i < 3; i++ ) {
+ p1[i] = p3[i];
+ }
+ }
+
+/* Mean RA,Dec */
+ iauC2s( p1, rm, dm );
+ *rm = iauAnp( *rm );
+}
diff --git a/pal/palCaldj.c b/pal/palCaldj.c
new file mode 100644
index 0000000..38ed424
--- /dev/null
+++ b/pal/palCaldj.c
@@ -0,0 +1,96 @@
+/*
+*+
+* Name:
+* palCaldj
+
+* Purpose:
+* Gregorian Calendar to Modified Julian Date
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palCaldj ( int iy, int im, int id, double *djm, int *j );
+
+* Arguments:
+* iy = int (Given)
+* Year in the Gregorian calendar
+* im = int (Given)
+* Month in the Gergorian calendar
+* id = int (Given)
+* Day in the Gregorian calendar
+* djm = double * (Returned)
+* Modified Julian Date (JD-2400000.5) for 0 hrs
+* j = status (Returned)
+* 0 = OK. See iauCal2jd for other values.
+
+* Description:
+* Modified Julian Date to Gregorian Calendar with special
+* behaviour for 2-digit years relating to 1950 to 2049.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-11 (TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Notes:
+* - Uses iauCal2jd
+* - Unlike iauCal2jd this routine treats the years 0-100 as
+* referring to the end of the 20th Century and beginning of
+* the 21st Century. If this behaviour is not acceptable
+* use the SOFA routine directly or palCldj.
+* Acceptable years are 00-49, interpreted as 2000-2049,
+* 50-99, " " 1950-1999,
+* all others, interpreted literally.
+* - Unlike SLA this routine will work with negative years.
+
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "palmac.h"
+#include "sofa.h"
+
+void palCaldj ( int iy, int im, int id, double *djm, int *j ) {
+ int adj = 0; /* Year adjustment */
+ double djm0;
+
+ if (iy >= 0 && iy <= 49) {
+ adj = 2000;
+ } else if (iy >= 50 && iy <= 99) {
+ adj = 1900;
+ }
+ iy += adj;
+
+ *j = iauCal2jd( iy, im, id, &djm0, djm );
+}
diff --git a/pal/palDat.c b/pal/palDat.c
new file mode 100644
index 0000000..43e9b53
--- /dev/null
+++ b/pal/palDat.c
@@ -0,0 +1,93 @@
+/*
+*+
+* Name:
+* palDtt
+
+* Purpose:
+* Return offset between UTC and TT
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* dat = palDat( double utc );
+
+* Arguments:
+* utc = double (Given)
+* UTC date as a modified JD (JD-2400000.5)
+
+* Returned Value:
+* dat = double
+* TAI-UTC in seconds
+
+* Description:
+* Increment to be applied to Coordinated Universal Time UTC to give
+* International Atomic Time (TAI).
+
+* Authors:
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* Notes:
+* - This routine converts the MJD argument to calendar date before calling
+* the SOFA iauDat function.
+* - This routine matches the slaDat interface which differs from the iauDat
+* interface. Consider coding directly to the SOFA interface.
+* - See iauDat for a description of error conditions when calling this function
+* with a time outside of the UTC range.
+* - The status argument from iauDat is ignored. This is reasonable since the
+* error codes are mainly related to incorrect calendar dates when calculating
+* the JD internally.
+
+* History:
+* 2012-02-08 (TIMJ):
+* Initial version
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "palmac.h"
+
+#include "sofa.h"
+
+double palDat ( double dju ) {
+ int iy;
+ int im;
+ int id;
+ int status;
+ double fd;
+ double deltat;
+
+ iauJd2cal( PAL__MJD0, dju,
+ &iy, &im, &id, &fd );
+
+ status = iauDat( iy, im, id, fd, &deltat );
+ return deltat;
+}
diff --git a/pal/palDe2h.c b/pal/palDe2h.c
new file mode 100644
index 0000000..ad157fc
--- /dev/null
+++ b/pal/palDe2h.c
@@ -0,0 +1,140 @@
+/*
+*+
+* Name:
+* palDe2h
+
+* Purpose:
+* Equatorial to horizon coordinates: HA,Dec to Az,E
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* palDe2h( double ha, double dec, double phi, double * az, double * el );
+
+* Arguments:
+* ha = double * (Given)
+* Hour angle (radians)
+* dec = double * (Given)
+* Declination (radians)
+* phi = double (Given)
+* Observatory latitude (radians)
+* az = double * (Returned)
+* Azimuth (radians)
+* el = double * (Returned)
+* Elevation (radians)
+
+* Description:
+
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* Notes:
+* - All the arguments are angles in radians.
+* - Azimuth is returned in the range 0-2pi; north is zero,
+* and east is +pi/2. Elevation is returned in the range
+* +/-pi/2.
+* - The latitude must be geodetic. In critical applications,
+* corrections for polar motion should be applied.
+* - In some applications it will be important to specify the
+* correct type of hour angle and declination in order to
+* produce the required type of azimuth and elevation. In
+* particular, it may be important to distinguish between
+* elevation as affected by refraction, which would
+* require the "observed" HA,Dec, and the elevation
+* in vacuo, which would require the "topocentric" HA,Dec.
+* If the effects of diurnal aberration can be neglected, the
+* "apparent" HA,Dec may be used instead of the topocentric
+* HA,Dec.
+* - No range checking of arguments is carried out.
+* - In applications which involve many such calculations, rather
+* than calling the present routine it will be more efficient to
+* use inline code, having previously computed fixed terms such
+* as sine and cosine of latitude, and (for tracking a star)
+* sine and cosine of declination.
+
+* History:
+* 2012-02-08 (TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "palmac.h"
+#include <math.h>
+
+void
+palDe2h ( double ha, double dec, double phi, double *az, double *el) {
+
+ double sh;
+ double ch;
+ double sd;
+ double cd;
+ double sp;
+ double cp;
+
+ double a;
+
+ double x;
+ double y;
+ double z;
+ double r;
+
+ /* Useful trig functions */
+ sh = sin(ha);
+ ch = cos(ha);
+ sd = sin(dec);
+ cd = cos(dec);
+ sp = sin(phi);
+ cp = cos(phi);
+
+ /* Az,El as x,y,z */
+ x = -ch * cd * sp + sd * cp;
+ y = -sh * cd;
+ z = ch * cd * cp + sd * sp;
+
+ /* To spherical */
+ r = sqrt(x * x + y * y);
+ if (r == 0.) {
+ a = 0.;
+ } else {
+ a = atan2(y, x);
+ }
+ if (a < 0.) {
+ a += PAL__D2PI;
+ }
+ *az = a;
+ *el = atan2(z, r);
+
+ return;
+}
diff --git a/pal/palDeuler.c b/pal/palDeuler.c
new file mode 100644
index 0000000..c504cf1
--- /dev/null
+++ b/pal/palDeuler.c
@@ -0,0 +1,139 @@
+/*
+*+
+* Name:
+* palDeuler
+
+* Purpose:
+* Form a rotation matrix from the Euler angles
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palDeuler ( const char *order, double phi, double theta, double psi,
+* double rmat[3][3] );
+
+* Arguments:
+* order = const char[] (Given)
+* Specifies about which axes the rotation occurs
+* phi = double (Given)
+* 1st rotation (radians)
+* theta = double (Given)
+* 2nd rotation (radians)
+* psi = double (Given)
+* 3rd rotation (radians)
+* rmat = double[3][3] (Given & Returned)
+* Rotation matrix
+
+* Description:
+* A rotation is positive when the reference frame rotates
+* anticlockwise as seen looking towards the origin from the
+* positive region of the specified axis.
+*
+* The characters of ORDER define which axes the three successive
+* rotations are about. A typical value is 'ZXZ', indicating that
+* RMAT is to become the direction cosine matrix corresponding to
+* rotations of the reference frame through PHI radians about the
+* old Z-axis, followed by THETA radians about the resulting X-axis,
+* then PSI radians about the resulting Z-axis.
+*
+* The axis names can be any of the following, in any order or
+* combination: X, Y, Z, uppercase or lowercase, 1, 2, 3. Normal
+* axis labelling/numbering conventions apply; the xyz (=123)
+* triad is right-handed. Thus, the 'ZXZ' example given above
+* could be written 'zxz' or '313' (or even 'ZxZ' or '3xZ'). ORDER
+* is terminated by length or by the first unrecognized character.
+*
+* Fewer than three rotations are acceptable, in which case the later
+* angle arguments are ignored. If all rotations are zero, the
+* identity matrix is produced.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-08 (TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+void
+palDeuler( const char *order, double phi, double theta, double psi,
+ double rmat[3][3] ) {
+ int i = 0;
+ double rotations[3];
+
+ /* Initialise rmat */
+ iauIr( rmat );
+
+ /* copy the rotations into an array */
+ rotations[0] = phi;
+ rotations[1] = theta;
+ rotations[2] = psi;
+
+ /* maximum three rotations */
+ while (i < 3 && order[i] != '\0') {
+
+ switch (order[i]) {
+ case 'X':
+ case 'x':
+ case '1':
+ iauRx( rotations[i], rmat );
+ break;
+
+ case 'Y':
+ case 'y':
+ case '2':
+ iauRy( rotations[i], rmat );
+ break;
+
+ case 'Z':
+ case 'z':
+ case '3':
+ iauRz( rotations[i], rmat );
+ break;
+
+ default:
+ /* break out the loop if we do not recognize something */
+ i = 3;
+
+ }
+
+ /* Go to the next position */
+ i++;
+ }
+
+ return;
+}
diff --git a/pal/palDh2e.c b/pal/palDh2e.c
new file mode 100644
index 0000000..6bda403
--- /dev/null
+++ b/pal/palDh2e.c
@@ -0,0 +1,131 @@
+/*
+*+
+* Name:
+* palDh2e
+
+* Purpose:
+* Horizon to equatorial coordinates: Az,El to HA,Dec
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* palDh2e( double az, double el, double phi, double * ha, double * dec );
+
+* Arguments:
+* az = double (Given)
+* Azimuth (radians)
+* el = double (Given)
+* Elevation (radians)
+* phi = double (Given)
+* Observatory latitude (radians)
+* ha = double * (Returned)
+* Hour angle (radians)
+* dec = double * (Returned)
+* Declination (radians)
+
+* Description:
+
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* Notes:
+* - All the arguments are angles in radians.
+* - The sign convention for azimuth is north zero, east +pi/2.
+* - HA is returned in the range +/-pi. Declination is returned
+* in the range +/-pi/2.
+* - The latitude is (in principle) geodetic. In critical
+* applications, corrections for polar motion should be applied.
+* - In some applications it will be important to specify the
+* correct type of elevation in order to produce the required
+* type of HA,Dec. In particular, it may be important to
+* distinguish between the elevation as affected by refraction,
+* which will yield the "observed" HA,Dec, and the elevation
+* in vacuo, which will yield the "topocentric" HA,Dec. If the
+* effects of diurnal aberration can be neglected, the
+* topocentric HA,Dec may be used as an approximation to the
+* "apparent" HA,Dec.
+* - No range checking of arguments is done.
+* - In applications which involve many such calculations, rather
+* than calling the present routine it will be more efficient to
+* use inline code, having previously computed fixed terms such
+* as sine and cosine of latitude.
+
+* History:
+* 2012-02-08 (TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include <math.h>
+
+void
+palDh2e ( double az, double el, double phi, double *ha, double *dec) {
+
+ double sa;
+ double ca;
+ double se;
+ double ce;
+ double sp;
+ double cp;
+
+ double x;
+ double y;
+ double z;
+ double r;
+
+ /* Useful trig functions */
+ sa = sin(az);
+ ca = cos(az);
+ se = sin(el);
+ ce = cos(el);
+ sp = sin(phi);
+ cp = cos(phi);
+
+ /* HA,Dec as x,y,z */
+ x = -ca * ce * sp + se * cp;
+ y = -sa * ce;
+ z = ca * ce * cp + se * sp;
+
+ /* To HA,Dec */
+ r = sqrt(x * x + y * y);
+ if (r == 0.) {
+ *ha = 0.;
+ } else {
+ *ha = atan2(y, x);
+ }
+ *dec = atan2(z, r);
+
+ return;
+}
diff --git a/pal/palDjcal.c b/pal/palDjcal.c
new file mode 100644
index 0000000..d7db3f1
--- /dev/null
+++ b/pal/palDjcal.c
@@ -0,0 +1,95 @@
+/*
+*+
+* Name:
+* palDjcal
+
+* Purpose:
+* Modified Julian Date to Gregorian Calendar
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palDjcal ( int ndp, double djm, int iymdf[4], int *j );
+
+* Arguments:
+* ndp = int (Given)
+* Number of decimal places of days in fraction.
+* djm = double (Given)
+* Modified Julian Date (JD-2400000.5)
+* iymdf[4] = int[] (Returned)
+* Year, month, day, fraction in Gregorian calendar.
+* j = status (Returned)
+* 0 = OK. See iauJd2cal for other values.
+
+* Description:
+* Modified Julian Date to Gregorian Calendar, expressed
+* in a form convenient for formatting messages (namely
+* rounded to a specified precision, and with the fields
+* stored in a single array)
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-10 (TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Notes:
+* - Uses iauJd2cal
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include <math.h>
+
+#include "pal.h"
+#include "palmac.h"
+#include "sofa.h"
+
+void palDjcal ( int ndp, double djm, int iymdf[4], int *j ) {
+ double frac = 0.0;
+ double nfd;
+
+ *j = iauJd2cal( PAL__MJD0, djm, &(iymdf[0]),
+ &(iymdf[1]), &(iymdf[2]),
+ &frac);
+
+ /* Convert ndp to a power of 10 */
+ nfd = pow( 10., (double)ndp );
+
+ /* Multiply the fraction */
+ frac *= nfd;
+
+ /* and now we want to round to the nearest integer */
+ iymdf[3] = (int)DNINT(frac);
+
+}
diff --git a/pal/palDmat.c b/pal/palDmat.c
new file mode 100644
index 0000000..eab2253
--- /dev/null
+++ b/pal/palDmat.c
@@ -0,0 +1,178 @@
+/*
+*+
+* Name:
+* palDmat
+
+* Purpose:
+* Matrix inversion & solution of simultaneous equations
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palDmat( int n, double *a, double *y, double *d, int *jf,
+* int *iw );
+
+* Arguments:
+* n = int (Given)
+* Number of simultaneous equations and number of unknowns.
+* a = double[] (Given & Returned)
+* A non-singular NxN matrix (implemented as a contiguous block
+* of memory). After calling this routine "a" contains the
+* inverse of the matrix.
+* y = double[] (Given & Returned)
+* The vector of N unknowns. On exit this vector contains the
+* N solutions.
+* d = double * (Returned)
+* The determinant.
+* jf = int * (Returned)
+* The singularity flag. If the matrix is non-singular, jf=0
+* is returned. If the matrix is singular, jf=-1 & d=0.0 are
+* returned. In the latter case, the contents of array "a" on
+* return are undefined.
+
+* Description:
+* Matrix inversion & solution of simultaneous equations
+* For the set of n simultaneous equations in n unknowns:
+* A.Y = X
+* this routine calculates the inverse of A, the determinant
+* of matrix A and the vector of N unknowns.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-11 (TIMJ):
+* Combination of a port of the Fortran and a comparison
+* with the obfuscated GPL C routine.
+* {enter_further_changes_here}
+
+* Notes:
+* - Implemented using Gaussian elimination with partial pivoting.
+* - Optimized for speed rather than accuracy with errors 1 to 4
+* times those of routines optimized for accuracy.
+
+* Copyright:
+* Copyright (C) 2001 Rutherford Appleton Laboratory.
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+
+void palDmat ( int n, double *a, double *y, double *d, int *jf, int *iw ) {
+
+ const double SFA = 1e-20;
+
+ int k;
+ double*aoff;
+
+ *jf=0;
+ *d=1.0;
+ for(k=0,aoff=a; k<n; k++, aoff+=n){
+ int imx;
+ double * aoff2 = aoff;
+ double amx=fabs(aoff[k]);
+ imx=k;
+ if(k!=n){
+ int i;
+ double *apos2;
+ for(i=k+1,apos2=aoff+n;i<n;i++,apos2+=n){
+ double t=fabs(apos2[k]);
+ if(t>amx){
+ amx=t;
+ imx=i;
+ aoff2=apos2;
+ }
+ }
+ }
+ if(amx<SFA){
+ *jf=-1;
+ } else {
+ if(imx!=k){
+ double t;
+ int j;
+ for(j=0;j<n;j++){
+ t=aoff[j];
+ aoff[j]=aoff2[j];
+ aoff2[j]=t;
+ }
+ t=y[k];
+ y[k]=y[imx];
+ y[imx]=t;*d=-*d;
+ }
+ iw[k]=imx;
+ *d*=aoff[k];
+ if(fabs(*d)<SFA){
+ *jf=-1;
+ } else {
+ double yk;
+ double * apos2;
+ int i, j;
+ aoff[k]=1.0/aoff[k];
+ for(j=0;j<n;j++){
+ if(j!=k){
+ aoff[j]*=aoff[k];
+ }
+ }
+ yk=y[k]*aoff[k];
+ y[k]=yk;
+ for(i=0,apos2=a;i<n;i++,apos2+=n){
+ if(i!=k){
+ for(j=0;j<n;j++){
+ if(j!=k){
+ apos2[j]-=apos2[k]*aoff[j];
+ }
+ }
+ y[i]-=apos2[k]*yk;
+ }
+ }
+ for(i=0,apos2=a;i<n;i++,apos2+=n){
+ if(i!=k){
+ apos2[k]*=-aoff[k];
+ }
+ }
+ }
+ }
+ }
+ if(*jf!=0){
+ *d=0.0;
+ } else {
+ for(k=n;k-->0;){
+ int ki=iw[k];
+ if(k!=ki){
+ int i;
+ double *apos = a;
+ for(i=0;i<n;i++,apos+=n){
+ double t=apos[k];
+ apos[k]=apos[ki];
+ apos[ki]=t;
+ }
+ }
+ }
+ }
+}
diff --git a/pal/palDs2tp.c b/pal/palDs2tp.c
new file mode 100644
index 0000000..fa0c4a1
--- /dev/null
+++ b/pal/palDs2tp.c
@@ -0,0 +1,125 @@
+/*
+*+
+* Name:
+* palDs2tp
+
+* Purpose:
+* Spherical to tangent plane projection
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* palDs2tp( double ra, double dec, double raz, double decz,
+* double *xi, double *eta, int *j );
+
+* Arguments:
+* ra = double (Given)
+* RA spherical coordinate of point to be projected (radians)
+* dec = double (Given)
+* Dec spherical coordinate of point to be projected (radians)
+* raz = double (Given)
+* RA spherical coordinate of tangent point (radians)
+* decz = double (Given)
+* Dec spherical coordinate of tangent point (radians)
+* xi = double * (Returned)
+* First rectangular coordinate on tangent plane (radians)
+* eta = double * (Returned)
+* Second rectangular coordinate on tangent plane (radians)
+* j = int * (Returned)
+* status: 0 = OK, star on tangent plane
+* 1 = error, star too far from axis
+* 2 = error, antistar on tangent plane
+* 3 = error, antistar too far from axis
+
+* Description:
+* Projection of spherical coordinates onto tangent plane:
+* "gnomonic" projection - "standard coordinates"
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-08 (TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include <math.h>
+
+void
+palDs2tp ( double ra, double dec, double raz, double decz,
+ double *xi, double *eta, int *j ) {
+
+ const double TINY = 1.0e-6;
+
+ double cdec;
+ double sdec;
+ double radif;
+ double cdecz;
+ double denom;
+ double sdecz;
+ double cradif;
+ double sradif;
+
+ /* Trig functions */
+ sdecz = sin(decz);
+ sdec = sin(dec);
+ cdecz = cos(decz);
+ cdec = cos(dec);
+ radif = ra - raz;
+ sradif = sin(radif);
+ cradif = cos(radif);
+
+ /* Reciprocal of star vector length to tangent plane */
+ denom = sdec * sdecz + cdec * cdecz * cradif;
+
+ /* Handle vectors too far from axis */
+ if (denom > TINY) {
+ *j = 0;
+ } else if (denom >= 0.) {
+ *j = 1;
+ denom = TINY;
+ } else if (denom > -TINY) {
+ *j = 2;
+ denom = -TINY;
+ } else {
+ *j = 3;
+ }
+
+ /* Compute tangent plane coordinates (even in dubious cases) */
+ *xi = cdec * sradif / denom;
+ *eta = (sdec * cdecz - cdec * sdecz * cradif) / denom;
+
+ return;
+}
diff --git a/pal/palDtp2s.c b/pal/palDtp2s.c
new file mode 100644
index 0000000..9a5d8de
--- /dev/null
+++ b/pal/palDtp2s.c
@@ -0,0 +1,93 @@
+/*
+*+
+* Name:
+* palDtp2s
+
+* Purpose:
+* Tangent plane to spherical coordinates
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* palDtp2s( double xi, double eta, double raz, double decz,
+* double *ra, double *dec);
+
+* Arguments:
+* xi = double (Given)
+* First rectangular coordinate on tangent plane (radians)
+* eta = double (Given)
+* Second rectangular coordinate on tangent plane (radians)
+* raz = double (Given)
+* RA spherical coordinate of tangent point (radians)
+* decz = double (Given)
+* Dec spherical coordinate of tangent point (radians)
+* ra = double * (Returned)
+* RA spherical coordinate of point to be projected (radians)
+* dec = double * (Returned)
+* Dec spherical coordinate of point to be projected (radians)
+
+* Description:
+* Transform tangent plane coordinates into spherical.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-08 (TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+#include <math.h>
+
+void
+palDtp2s ( double xi, double eta, double raz, double decz,
+ double *ra, double *dec ) {
+
+ double cdecz;
+ double denom;
+ double sdecz;
+ double d;
+
+ sdecz = sin(decz);
+ cdecz = cos(decz);
+ denom = cdecz - eta * sdecz;
+ d = atan2(xi, denom) + raz;
+ *ra = iauAnp(d);
+ *dec = atan2(sdecz + eta * cdecz, sqrt(xi * xi + denom * denom));
+
+ return;
+}
diff --git a/pal/palDtps2c.c b/pal/palDtps2c.c
new file mode 100644
index 0000000..d1a28b9
--- /dev/null
+++ b/pal/palDtps2c.c
@@ -0,0 +1,149 @@
+/*
+*+
+* Name:
+* palDtps2c
+
+* Purpose:
+* Determine RA,Dec of tangent point from coordinates
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* palDtps2c( double xi, double eta, double ra, double dec,
+* double * raz1, double decz1,
+* double * raz2, double decz2, int *n);
+
+* Arguments:
+* xi = double (Given)
+* First rectangular coordinate on tangent plane (radians)
+* eta = double (Given)
+* Second rectangular coordinate on tangent plane (radians)
+* ra = double (Given)
+* RA spherical coordinate of star (radians)
+* dec = double (Given)
+* Dec spherical coordinate of star (radians)
+* raz1 = double * (Returned)
+* RA spherical coordinate of tangent point, solution 1 (radians)
+* decz1 = double * (Returned)
+* Dec spherical coordinate of tangent point, solution 1 (radians)
+* raz2 = double * (Returned)
+* RA spherical coordinate of tangent point, solution 2 (radians)
+* decz2 = double * (Returned)
+* Dec spherical coordinate of tangent point, solution 2 (radians)
+* n = int * (Returned)
+* number of solutions: 0 = no solutions returned (note 2)
+* 1 = only the first solution is useful (note 3)
+* 2 = both solutions are useful (note 3)
+
+
+* Description:
+* From the tangent plane coordinates of a star of known RA,Dec,
+* determine the RA,Dec of the tangent point.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* Notes:
+* - The RAZ1 and RAZ2 values are returned in the range 0-2pi.
+* - Cases where there is no solution can only arise near the poles.
+* For example, it is clearly impossible for a star at the pole
+* itself to have a non-zero XI value, and hence it is
+* meaningless to ask where the tangent point would have to be
+* to bring about this combination of XI and DEC.
+* - Also near the poles, cases can arise where there are two useful
+* solutions. The argument N indicates whether the second of the
+* two solutions returned is useful. N=1 indicates only one useful
+* solution, the usual case; under these circumstances, the second
+* solution corresponds to the "over-the-pole" case, and this is
+* reflected in the values of RAZ2 and DECZ2 which are returned.
+* - The DECZ1 and DECZ2 values are returned in the range +/-pi, but
+* in the usual, non-pole-crossing, case, the range is +/-pi/2.
+* - This routine is the spherical equivalent of the routine sla_DTPV2C.
+
+* History:
+* 2012-02-08 (TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+#include <math.h>
+
+void
+palDtps2c( double xi, double eta, double ra, double dec,
+ double * raz1, double * decz1,
+ double * raz2, double * decz2, int *n) {
+
+ double x2;
+ double y2;
+ double sd;
+ double cd;
+ double sdf;
+ double r2;
+
+ x2 = xi * xi;
+ y2 = eta * eta;
+ sd = sin(dec);
+ cd = cos(dec);
+ sdf = sd * sqrt(x2 + 1. + y2);
+ r2 = cd * cd * (y2 + 1.) - sd * sd * x2;
+ if (r2 >= 0.) {
+ double r;
+ double s;
+ double c;
+
+ r = sqrt(r2);
+ s = sdf - eta * r;
+ c = sdf * eta + r;
+ if (xi == 0. && r == 0.) {
+ r = 1.;
+ }
+ *raz1 = iauAnp(ra - atan2(xi, r));
+ *decz1 = atan2(s, c);
+ r = -r;
+ s = sdf - eta * r;
+ c = sdf * eta + r;
+ *raz2 = iauAnp(ra - atan2(xi, r));
+ *decz2 = atan2(s, c);
+ if (fabs(sdf) < 1.) {
+ *n = 1;
+ } else {
+ *n = 2;
+ }
+ } else {
+ *n = 0;
+ }
+ return;
+}
diff --git a/pal/palDtt.c b/pal/palDtt.c
new file mode 100644
index 0000000..af52b94
--- /dev/null
+++ b/pal/palDtt.c
@@ -0,0 +1,74 @@
+/*
+*+
+* Name:
+* palDtt
+
+* Purpose:
+* Return offset between UTC and TT
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* dtt = palDtt( double utc );
+
+* Arguments:
+* utc = double (Given)
+* UTC date as a modified JD (JD-2400000.5)
+
+* Returned Value:
+* dtt = double
+* TT-UTC in seconds
+
+* Description:
+* Increment to be applied to Coordinated Universal Time UTC to give
+* Terrestrial Time TT (formerly Ephemeris Time ET)
+
+* Authors:
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* Notes:
+* - Consider a comprehensive upgrade to use the time transformations in SOFA's time
+* cookbook: http://www.iausofa.org/sofa_ts_c.pdf.
+* - See iauDat for a description of error conditions when calling this function
+* with a time outside of the UTC range. This behaviour differs from slaDtt.
+
+* History:
+* 2012-02-08 (TIMJ):
+* Initial version
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+
+double palDtt( double utc ) {
+ return 32.184 + palDat( utc );
+}
diff --git a/pal/palEcmat.c b/pal/palEcmat.c
new file mode 100644
index 0000000..0827c1d
--- /dev/null
+++ b/pal/palEcmat.c
@@ -0,0 +1,80 @@
+/*
+*+
+* Name:
+* palEcmat
+
+* Purpose:
+* Form the equatorial to ecliptic rotation matrix - IAU 2006
+* precession model.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* palEcmat( double date, double rmat[3][3] )
+
+* Arguments:
+* date = double (Given)
+* TT as Modified Julian Date (JD-2400000.5). The difference
+* between TT and TDB is of the order of a millisecond or two
+* (i.e. about 0.02 arc-seconds).
+* rmat = double[3][3] (Returned)
+* Rotation matrix
+
+* Description:
+* The equatorial to ecliptic rotation matrix is found and returned.
+* The matrix is in the sense V(ecl) = RMAT * V(equ); the
+* equator, equinox and ecliptic are mean of date.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* DSB: David Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-10 (DSB):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "palmac.h"
+#include "sofa.h"
+
+void palEcmat( double date, double rmat[3][3] ) {
+
+/* Mean obliquity (the angle between the ecliptic and mean equator of
+ date). */
+ double eps0 = iauObl06( PAL__MJD0, date );
+
+/* Matrix */
+ palDeuler( "X", eps0, 0.0, 0.0, rmat );
+
+}
diff --git a/pal/palEqgal.c b/pal/palEqgal.c
new file mode 100644
index 0000000..ed06d2e
--- /dev/null
+++ b/pal/palEqgal.c
@@ -0,0 +1,114 @@
+/*
+*+
+* Name:
+* palEqgal
+
+* Purpose:
+* Convert from J2000.0 equatorial coordinates to Galactic
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palEqgal ( double dr, double dd, double *dl, double *db );
+
+* Arguments:
+* dr = double (Given)
+* J2000.0 RA (radians)
+* dd = double (Given)
+* J2000.0 Dec (radians
+* dl = double * (Returned)
+* Galactic longitude (radians).
+* db = double * (Returned)
+* Galactic latitude (radians).
+
+* Description:
+* Transformation from J2000.0 equatorial coordinates
+* to IAU 1958 galactic coordinates.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* Notes:
+* The equatorial coordinates are J2000.0. Use the routine
+* palGe50 if conversion to B1950.0 'FK4' coordinates is
+* required.
+
+* See Also:
+* Blaauw et al, Mon.Not.R.Astron.Soc.,121,123 (1960)
+
+* History:
+* 2012-02-12(TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+void palEqgal ( double dr, double dd, double *dl, double *db ) {
+
+ double v1[3];
+ double v2[3];
+
+/*
+* L2,B2 system of galactic coordinates
+*
+* P = 192.25 RA of galactic north pole (mean B1950.0)
+* Q = 62.6 inclination of galactic to mean B1950.0 equator
+* R = 33 longitude of ascending node
+*
+* P,Q,R are degrees
+*
+* Equatorial to galactic rotation matrix (J2000.0), obtained by
+* applying the standard FK4 to FK5 transformation, for zero proper
+* motion in FK5, to the columns of the B1950 equatorial to
+* galactic rotation matrix:
+*/
+ double rmat[3][3] = {
+ { -0.054875539726,-0.873437108010,-0.483834985808 },
+ { +0.494109453312,-0.444829589425,+0.746982251810 },
+ { -0.867666135858,-0.198076386122,+0.455983795705 }
+ };
+
+ /* Spherical to Cartesian */
+ iauS2c( dr, dd, v1 );
+
+ /* Equatorial to Galactic */
+ iauRxp( rmat, v1, v2 );
+
+ /* Cartesian to spherical */
+ iauC2s( v2, dl, db );
+
+ /* Express in conventional ranges */
+ *dl = iauAnp( *dl );
+ *db = iauAnpm( *db );
+
+}
diff --git a/pal/palEtrms.c b/pal/palEtrms.c
new file mode 100644
index 0000000..a4d67ee
--- /dev/null
+++ b/pal/palEtrms.c
@@ -0,0 +1,103 @@
+/*
+*+
+* Name:
+* palEtrms
+
+* Purpose:
+* Compute the E-terms vector
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palEtrms ( double ep, double ev[3] );
+
+* Arguments:
+* ep = double (Given)
+* Besselian epoch
+* ev = double [3] (Returned)
+* E-terms as (dx,dy,dz)
+
+* Description:
+* Computes the E-terms (elliptic component of annual aberration)
+* vector.
+*
+* Note the use of the J2000 aberration constant (20.49552 arcsec).
+* This is a reflection of the fact that the E-terms embodied in
+* existing star catalogues were computed from a variety of
+* aberration constants. Rather than adopting one of the old
+* constants the latest value is used here.
+*
+* See also:
+* - Smith, C.A. et al., 1989. Astr.J. 97, 265.
+* - Yallop, B.D. et al., 1989. Astr.J. 97, 274.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-12 (TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "palmac.h"
+
+void palEtrms ( double ep, double ev[3] ) {
+
+ /* Use the J2000 aberration constant */
+ const double ABCONST = 20.49552;
+
+ double t, e, e0, p, ek, cp;
+
+ /* Julian centuries since B1950 */
+ t = (ep - 1950.) * .0100002135903;
+
+ /* Eccentricity */
+ e = .01673011 - (t * 1.26e-7 + 4.193e-5) * t;
+
+ /* Mean obliquity */
+ e0 = (84404.836 - ((t * .00181 + .00319) * t + 46.8495) * t) *
+ PAL__DAS2R;
+
+ /* Mean longitude of perihelion */
+ p = (((t * .012 + 1.65) * t + 6190.67) * t + 1015489.951) *
+ PAL__DAS2R;
+
+ /* E-terms */
+ ek = e * ABCONST * PAL__DAS2R;
+ cp = cos(p);
+ ev[0] = ek * sin(p);
+ ev[1] = -ek * cp * cos(e0);
+ ev[2] = -ek * cp * sin(e0);
+
+}
diff --git a/pal/palEvp.c b/pal/palEvp.c
new file mode 100644
index 0000000..6b0466e
--- /dev/null
+++ b/pal/palEvp.c
@@ -0,0 +1,107 @@
+/*
+*+
+* Name:
+* palEvp
+
+* Purpose:
+* Returns the barycentric and heliocentric velocity and position of the
+* Earth.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palEvp( double date, double deqx, double dvb[3], double dpb[3],
+* double dvh[3], double dph[3] )
+
+* Arguments:
+* date = double (Given)
+* TDB (loosely ET) as a Modified Julian Date (JD-2400000.5)
+* deqx = double (Given)
+* Julian epoch (e.g. 2000.0) of mean equator and equinox of the
+* vectors returned. If deqx <= 0.0, all vectors are referred to the
+* mean equator and equinox (FK5) of epoch date.
+* dvb = double[3] (Returned)
+* Barycentric velocity (AU/s, AU)
+* dpb = double[3] (Returned)
+* Barycentric position (AU/s, AU)
+* dvh = double[3] (Returned)
+* heliocentric velocity (AU/s, AU)
+* dph = double[3] (Returned)
+* Heliocentric position (AU/s, AU)
+
+* Description:
+* Returns the barycentric and heliocentric velocity and position of the
+* Earth at a given epoch, given with respect to a specified equinox.
+* For information about accuracy, see the function iauEpv00.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-13 (PTW):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+void palEvp( double date, double deqx, double dvb[3], double dpb[3],
+ double dvh[3], double dph[3] ){
+
+/* Local Variables; */
+ int i;
+ double pvh[2][3], pvb[2][3], d1, d2, r[3][3];
+
+/* BCRS PV-vectors. */
+ iauEpv00 ( 2400000.5, date, pvh, pvb );
+
+/* Was precession to another equinox requested? */
+ if ( deqx > 0.0 ) {
+
+/* Yes: compute precession matrix from J2000.0 to deqx. */
+ iauEpj2jd ( deqx, &d1, &d2 );
+ iauPmat06 ( d1, d2, r );
+
+/* Rotate the PV-vectors. */
+ iauRxpv ( r, pvh, pvh );
+ iauRxpv ( r, pvb, pvb );
+ }
+
+/* Return the required vectors. */
+ for ( i = 0; i < 3; i++ ) {
+ dvh[i] = pvh[1][i] / 86400.0;
+ dvb[i] = pvb[1][i] / 86400.0;
+ dph[i] = pvh[0][i];
+ dpb[i] = pvb[0][i];
+ }
+}
diff --git a/pal/palFk45z.c b/pal/palFk45z.c
new file mode 100644
index 0000000..fe2ac23
--- /dev/null
+++ b/pal/palFk45z.c
@@ -0,0 +1,184 @@
+/*
+*+
+* Name:
+* palFk45z
+
+* Purpose:
+* Convert B1950.0 FK4 star data to J2000.0 FK5 assuming zero
+* proper motion in the FK5 frame
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* palFk45z( double r1950, double d1950, double bepoch, double *r2000,
+* double *d2000 )
+
+* Arguments:
+* r1950 = double (Given)
+* B1950.0 FK4 RA at epoch (radians).
+* d1950 = double (Given)
+* B1950.0 FK4 Dec at epoch (radians).
+* bepoch = double (Given)
+* Besselian epoch (e.g. 1979.3)
+* r2000 = double (Returned)
+* J2000.0 FK5 RA (Radians).
+* d2000 = double (Returned)
+* J2000.0 FK5 Dec(Radians).
+
+* Description:
+* Convert B1950.0 FK4 star data to J2000.0 FK5 assuming zero
+* proper motion in the FK5 frame (double precision)
+*
+* This function converts stars from the Bessel-Newcomb, FK4
+* system to the IAU 1976, FK5, Fricke system, in such a
+* way that the FK5 proper motion is zero. Because such a star
+* has, in general, a non-zero proper motion in the FK4 system,
+* the routine requires the epoch at which the position in the
+* FK4 system was determined.
+*
+* The method is from Appendix 2 of Ref 1, but using the constants
+* of Ref 4.
+
+* Notes:
+* - The epoch BEPOCH is strictly speaking Besselian, but if a
+* Julian epoch is supplied the result will be affected only to
+* a negligible extent.
+*
+* - Conversion from Besselian epoch 1950.0 to Julian epoch 2000.0
+* only is provided for. Conversions involving other epochs will
+* require use of the appropriate precession, proper motion, and
+* E-terms routines before and/or after palFk45z is called.
+*
+* - In the FK4 catalogue the proper motions of stars within 10
+* degrees of the poles do not embody the differential E-term effect
+* and should, strictly speaking, be handled in a different manner
+* from stars outside these regions. However, given the general lack
+* of homogeneity of the star data available for routine astrometry,
+* the difficulties of handling positions that may have been
+* determined from astrometric fields spanning the polar and non-polar
+* regions, the likelihood that the differential E-terms effect was not
+* taken into account when allowing for proper motion in past
+* astrometry, and the undesirability of a discontinuity in the
+* algorithm, the decision has been made in this routine to include the
+* effect of differential E-terms on the proper motions for all stars,
+* whether polar or not. At epoch 2000, and measuring on the sky rather
+* than in terms of dRA, the errors resulting from this simplification
+* are less than 1 milliarcsecond in position and 1 milliarcsecond per
+* century in proper motion.
+*
+* References:
+* 1 - Aoki,S., et al, 1983. Astron.Astrophys., 128, 263.
+* 2 - Smith, C.A. et al, 1989. "The transformation of astrometric
+* catalog systems to the equinox J2000.0". Astron.J. 97, 265.
+* 3 - Yallop, B.D. et al, 1989. "Transformation of mean star places
+* from FK4 B1950.0 to FK5 J2000.0 using matrices in 6-space".
+* Astron.J. 97, 274.
+* 4 - Seidelmann, P.K. (ed), 1992. "Explanatory Supplement to
+* the Astronomical Almanac", ISBN 0-935702-68-7.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* DSB: David Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-10 (DSB):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "palmac.h"
+#include "sofa.h"
+
+void palFk45z( double r1950, double d1950, double bepoch, double *r2000,
+ double *d2000 ){
+
+/* Local Variables: */
+ double w;
+ int i;
+ int j;
+ double r0[3], a1[3], v1[3], v2[6]; /* Position and position+velocity vectors */
+
+
+/* CANONICAL CONSTANTS (see references) */
+
+/* Vector A. */
+ double a[3] = { -1.62557E-6, -0.31919E-6, -0.13843E-6 };
+
+/* Vectors Adot. */
+ double ad[3] = { 1.245E-3, -1.580E-3, -0.659E-3 };
+
+/* Matrix M (only half of which is needed here). */
+ double em[6][3] = { {0.9999256782, -0.0111820611, -0.0048579477},
+ {0.0111820610, 0.9999374784, -0.0000271765},
+ {0.0048579479, -0.0000271474, 0.9999881997},
+ {-0.000551, -0.238565, 0.435739},
+ {0.238514, -0.002667, -0.008541},
+ {-0.435623, 0.012254, 0.002117} };
+
+
+/* Spherical to Cartesian. */
+ iauS2c( r1950, d1950, r0 );
+
+/* Adjust vector A to give zero proper motion in FK5. */
+ w = ( bepoch - 1950.0 )/PAL__PMF;
+ for( i = 0; i < 3; i++ ) {
+ a1[ i ] = a[ i ] + w*ad[ i ];
+ }
+
+/* Remove e-terms. */
+ w = r0[ 0 ]*a1[ 0 ] + r0[ 1 ]*a1[ 1 ] + r0[ 2 ]*a1[ 2 ];
+ for( i = 0; i < 3; i++ ) {
+ v1[ i ] = r0[ i ] - a1[ i ] + w*r0[ i ];
+ }
+
+/* Convert position vector to Fricke system. */
+ for( i = 0; i < 6; i++ ) {
+ w = 0.0;
+ for( j = 0; j < 3; j++ ) {
+ w += em[ i ][ j ]*v1[ j ];
+ }
+ v2[ i ] = w;
+ }
+
+/* Allow for fictitious proper motion in FK4. */
+ w = ( palEpj( palEpb2d( bepoch ) ) - 2000.0 )/PAL__PMF;
+ for( i = 0; i < 3; i++ ) {
+ v2[ i ] += w*v2[ i + 3 ];
+ }
+
+/* Revert to spherical coordinates. */
+ iauC2s( v2, &w, d2000 );
+ *r2000 = iauAnp( w );
+}
+
+
diff --git a/pal/palFk524.c b/pal/palFk524.c
new file mode 100644
index 0000000..bcd5537
--- /dev/null
+++ b/pal/palFk524.c
@@ -0,0 +1,257 @@
+/*
+*+
+* Name:
+* palFk524
+
+* Purpose:
+* Convert J2000.0 FK5 star data to B1950.0 FK4.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* palFk524( double r2000, double d2000, double dr2000, double dd2000,
+* double p2000, double v2000, double *r1950, double *d1950,
+* double *dr1950, double *dd1950, double *p1950, double *v1950 )
+
+* Arguments:
+* r2000 = double (Given)
+* J2000.0 FK5 RA (radians).
+* d2000 = double (Given)
+* J2000.0 FK5 Dec (radians).
+* dr2000 = double (Given)
+* J2000.0 FK5 RA proper motion (rad/Jul.yr)
+* dd2000 = double (Given)
+* J2000.0 FK5 Dec proper motion (rad/Jul.yr)
+* p2000 = double (Given)
+* J2000.0 FK5 parallax (arcsec)
+* v2000 = double (Given)
+* J2000.0 FK5 radial velocity (km/s, +ve = moving away)
+* r2000 = double * (Returned)
+* B1950.0 FK4 RA (radians).
+* d2000 = double * (Returned)
+* B1950.0 FK4 Dec (radians).
+* dr2000 = double * (Returned)
+* B1950.0 FK4 RA proper motion (rad/Jul.yr)
+* dd2000 = double * (Returned)
+* B1950.0 FK4 Dec proper motion (rad/Jul.yr)
+* p2000 = double * (Returned)
+* B1950.0 FK4 parallax (arcsec)
+* v2000 = double * (Returned)q
+* B1950.0 FK4 radial velocity (km/s, +ve = moving away)
+
+* Description:
+* This function converts stars from the IAU 1976, FK5, Fricke
+* system, to the Bessel-Newcomb, FK4 system. The precepts
+* of Smith et al (Ref 1) are followed, using the implementation
+* by Yallop et al (Ref 2) of a matrix method due to Standish.
+* Kinoshita's development of Andoyer's post-Newcomb precession is
+* used. The numerical constants from Seidelmann et al (Ref 3) are
+* used canonically.
+
+* Notes:
+* - The proper motions in RA are dRA/dt rather than
+* cos(Dec)*dRA/dt, and are per year rather than per century.
+* - Note that conversion from Julian epoch 2000.0 to Besselian
+* epoch 1950.0 only is provided for. Conversions involving
+* other epochs will require use of the appropriate precession,
+* proper motion, and E-terms routines before and/or after
+* FK524 is called.
+* - In the FK4 catalogue the proper motions of stars within
+* 10 degrees of the poles do not embody the differential
+* E-term effect and should, strictly speaking, be handled
+* in a different manner from stars outside these regions.
+* However, given the general lack of homogeneity of the star
+* data available for routine astrometry, the difficulties of
+* handling positions that may have been determined from
+* astrometric fields spanning the polar and non-polar regions,
+* the likelihood that the differential E-terms effect was not
+* taken into account when allowing for proper motion in past
+* astrometry, and the undesirability of a discontinuity in
+* the algorithm, the decision has been made in this routine to
+* include the effect of differential E-terms on the proper
+* motions for all stars, whether polar or not. At epoch 2000,
+* and measuring on the sky rather than in terms of dRA, the
+* errors resulting from this simplification are less than
+* 1 milliarcsecond in position and 1 milliarcsecond per
+* century in proper motion.
+*
+* References:
+* 1 - Smith, C.A. et al, 1989. "The transformation of astrometric
+* catalog systems to the equinox J2000.0". Astron.J. 97, 265.
+* 2 - Yallop, B.D. et al, 1989. "Transformation of mean star places
+* from FK4 B1950.0 to FK5 J2000.0 using matrices in 6-space".
+* Astron.J. 97, 274.
+* 3 - Seidelmann, P.K. (ed), 1992. "Explanatory Supplement to
+* the Astronomical Almanac", ISBN 0-935702-68-7.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* DSB: David Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-13 (DSB):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "palmac.h"
+#include "math.h"
+
+void palFk524( double r2000, double d2000, double dr2000, double dd2000,
+ double p2000, double v2000, double *r1950, double *d1950,
+ double *dr1950, double *dd1950, double *p1950, double *v1950 ){
+
+/* Local Variables; */
+ double r, d, ur, ud, px, rv;
+ double sr, cr, sd, cd, x, y, z, w;
+ double v1[ 6 ], v2[ 6 ];
+ double xd, yd, zd;
+ double rxyz, wd, rxysq, rxy;
+ int i, j;
+
+/* Small number to avoid arithmetic problems. */
+ static const double tiny = 1.0-30;
+
+/* Canonical constants (see references). Constant vector and matrix. */
+ double a[ 6 ] = { -1.62557E-6, -0.31919E-6, -0.13843E-6,
+ +1.245E-3, -1.580E-3, -0.659E-3 };
+ double emi[ 6 ][ 6 ] = {
+ { 0.9999256795, 0.0111814828, 0.0048590039,
+ -0.00000242389840, -0.00000002710544, -0.00000001177742},
+ {-0.0111814828, 0.9999374849, -0.0000271771,
+ 0.00000002710544, -0.00000242392702, 0.00000000006585 },
+ {-0.0048590040, -0.0000271557, 0.9999881946,
+ 0.00000001177742, 0.00000000006585, -0.00000242404995 },
+ {-0.000551, 0.238509, -0.435614,
+ 0.99990432, 0.01118145, 0.00485852 },
+ {-0.238560, -0.002667, 0.012254,
+ -0.01118145, 0.99991613, -0.00002717},
+ { 0.435730, -0.008541, 0.002117,
+ -0.00485852, -0.00002716, 0.99996684 } };
+
+/* Pick up J2000 data (units radians and arcsec/JC). */
+ r = r2000;
+ d = d2000;
+ ur = dr2000*PAL__PMF;
+ ud = dd2000*PAL__PMF;
+ px = p2000;
+ rv = v2000;
+
+/* Spherical to Cartesian. */
+ sr = sin( r );
+ cr = cos( r );
+ sd = sin( d );
+ cd = cos( d );
+
+ x = cr*cd;
+ y = sr*cd;
+ z = sd;
+
+ w = PAL__VF*rv*px;
+
+ v1[ 0 ] = x;
+ v1[ 1 ] = y;
+ v1[ 2 ] = z;
+
+ v1[ 3 ] = -ur*y - cr*sd*ud + w*x;
+ v1[ 4 ] = ur*x - sr*sd*ud + w*y;
+ v1[ 5 ] = cd*ud + w*z;
+
+/* Convert position+velocity vector to BN system. */
+ for( i = 0; i < 6; i++ ) {
+ w = 0.0;
+ for( j = 0; j < 6; j++ ) {
+ w += emi[ i ][ j ]*v1[ j ];
+ }
+ v2[ i ] = w;
+ }
+
+/* Position vector components and magnitude. */
+ x = v2[ 0 ];
+ y = v2[ 1 ];
+ z = v2[ 2 ];
+ rxyz = sqrt( x*x + y*y + z*z );
+
+/* Apply E-terms to position. */
+ w = x*a[ 0 ] + y*a[ 1 ] + z*a[ 2 ];
+ x += a[ 0 ]*rxyz - w*x;
+ y += a[ 1 ]*rxyz - w*y;
+ z += a[ 2 ]*rxyz - w*z;
+
+/* Recompute magnitude. */
+ rxyz = sqrt( x*x + y*y + z*z );
+
+/* Apply E-terms to both position and velocity. */
+ x = v2[ 0 ];
+ y = v2[ 1 ];
+ z = v2[ 2 ];
+ w = x*a[ 0 ] + y*a[ 1 ] + z*a[ 2 ];
+ wd = x*a[ 3 ] + y*a[ 4 ] + z*a[ 5 ];
+ x += a[ 0 ]*rxyz - w*x;
+ y += a[ 1 ]*rxyz - w*y;
+ z += a[ 2 ]*rxyz - w*z;
+ xd = v2[ 3 ] + a[ 3 ]*rxyz - wd*x;
+ yd = v2[ 4 ] + a[ 4 ]*rxyz - wd*y;
+ zd = v2[ 5 ] + a[ 5 ]*rxyz - wd*z;
+
+/* Convert to spherical. */
+ rxysq = x*x + y*y;
+ rxy = sqrt( rxysq );
+
+ if( x == 0.0 && y == 0.0 ) {
+ r = 0.0;
+ } else {
+ r = atan2( y, x );
+ if( r < 0.0 ) r += PAL__D2PI;
+ }
+ d = atan2( z, rxy );
+
+ if( rxy > tiny ) {
+ ur = ( x*yd - y*xd )/rxysq;
+ ud = ( zd*rxysq - z*( x*xd + y*yd ) )/( ( rxysq + z*z )*rxy );
+ }
+
+/* Radial velocity and parallax. */
+ if( px > tiny ) {
+ rv = ( x*xd + y*yd + z*zd )/( px*PAL__VF*rxyz );
+ px /= rxyz;
+ }
+
+/* Return results. */
+ *r1950 = r;
+ *d1950 = d;
+ *dr1950 = ur/PAL__PMF;
+ *dd1950 = ud/PAL__PMF;
+ *p1950 = px;
+ *v1950 = rv;
+}
diff --git a/pal/palFk54z.c b/pal/palFk54z.c
new file mode 100644
index 0000000..30c6aa6
--- /dev/null
+++ b/pal/palFk54z.c
@@ -0,0 +1,111 @@
+/*
+*+
+* Name:
+* palFk54z
+
+* Purpose:
+* Convert a J2000.0 FK5 star position to B1950.0 FK4 assuming
+* zero proper motion and parallax.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* palFk54z( double r2000, double d2000, double bepoch, double *r1950,
+* double *d1950, double *dr1950, double *dd1950 )
+
+* Arguments:
+* r2000 = double (Given)
+* J2000.0 FK5 RA (radians).
+* d2000 = double (Given)
+* J2000.0 FK5 Dec (radians).
+* bepoch = double (Given)
+* Besselian epoch (e.g. 1950.0).
+* r1950 = double * (Returned)
+* B1950 FK4 RA (radians) at epoch "bepoch".
+* d1950 = double * (Returned)
+* B1950 FK4 Dec (radians) at epoch "bepoch".
+* dr1950 = double * (Returned)
+* B1950 FK4 proper motion (RA) (radians/trop.yr)).
+* dr1950 = double * (Returned)
+* B1950 FK4 proper motion (Dec) (radians/trop.yr)).
+
+* Description:
+* This function converts star positions from the IAU 1976,
+* FK5, Fricke system to the Bessel-Newcomb, FK4 system.
+
+* Notes:
+* - The proper motion in RA is dRA/dt rather than cos(Dec)*dRA/dt.
+* - Conversion from Julian epoch 2000.0 to Besselian epoch 1950.0
+* only is provided for. Conversions involving other epochs will
+* require use of the appropriate precession functions before and
+* after this function is called.
+* - The FK5 proper motions, the parallax and the radial velocity
+* are presumed zero.
+* - It is the intention that FK5 should be a close approximation
+* to an inertial frame, so that distant objects have zero proper
+* motion; such objects have (in general) non-zero proper motion
+* in FK4, and this function returns those fictitious proper
+* motions.
+* - The position returned by this function is in the B1950
+* reference frame but at Besselian epoch BEPOCH. For comparison
+* with catalogues the "bepoch" argument will frequently be 1950.0.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* DSB: David Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-13 (DSB):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+void palFk54z( double r2000, double d2000, double bepoch, double *r1950,
+ double *d1950, double *dr1950, double *dd1950 ){
+
+/* Local Variables: */
+ double r, d, px, rv, y;
+
+/* FK5 equinox J2000 (any epoch) to FK4 equinox B1950 epoch B1950. */
+ palFk524( r2000, d2000, 0.0, 0.0, 0.0, 0.0, &r, &d, dr1950, dd1950,
+ &px, &rv );
+
+/* Fictitious proper motion to epoch "bepoch". */
+ y = bepoch - 1950.0;
+ *r1950 = r + *dr1950*y;
+ *d1950 = d + *dd1950*y;
+
+}
+
diff --git a/pal/palGaleq.c b/pal/palGaleq.c
new file mode 100644
index 0000000..0fa0ad0
--- /dev/null
+++ b/pal/palGaleq.c
@@ -0,0 +1,114 @@
+/*
+*+
+* Name:
+* palGaleq
+
+* Purpose:
+* Convert from galactic to J2000.0 equatorial coordinates
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palGaleq ( double dl, double db, double *dr, double *dd );
+
+* Arguments:
+* dl = double (Given)
+* Galactic longitude (radians).
+* db = double (Given)
+* Galactic latitude (radians).
+* dr = double * (Returned)
+* J2000.0 RA (radians)
+* dd = double * (Returned)
+* J2000.0 Dec (radians)
+
+* Description:
+* Transformation from IAU 1958 galactic coordinates to
+* J2000.0 equatorial coordinates.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* Notes:
+* The equatorial coordinates are J2000.0. Use the routine
+* palGe50 if conversion to B1950.0 'FK4' coordinates is
+* required.
+
+* See Also:
+* Blaauw et al, Mon.Not.R.Astron.Soc.,121,123 (1960)
+
+* History:
+* 2012-02-12(TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+void palGaleq ( double dl, double db, double *dr, double *dd ) {
+
+ double v1[3];
+ double v2[3];
+
+/*
+* L2,B2 system of galactic coordinates
+*
+* P = 192.25 RA of galactic north pole (mean B1950.0)
+* Q = 62.6 inclination of galactic to mean B1950.0 equator
+* R = 33 longitude of ascending node
+*
+* P,Q,R are degrees
+*
+* Equatorial to galactic rotation matrix (J2000.0), obtained by
+* applying the standard FK4 to FK5 transformation, for zero proper
+* motion in FK5, to the columns of the B1950 equatorial to
+* galactic rotation matrix:
+*/
+ double rmat[3][3] = {
+ { -0.054875539726,-0.873437108010,-0.483834985808 },
+ { +0.494109453312,-0.444829589425,+0.746982251810 },
+ { -0.867666135858,-0.198076386122,+0.455983795705 }
+ };
+
+ /* Spherical to Cartesian */
+ iauS2c( dl, db, v1 );
+
+ /* Galactic to equatorial */
+ iauTrxp( rmat, v1, v2 );
+
+ /* Cartesian to spherical */
+ iauC2s( v2, dr, dd );
+
+ /* Express in conventional ranges */
+ *dr = iauAnp( *dr );
+ *dd = iauAnpm( *dd );
+
+}
diff --git a/pal/palGalsup.c b/pal/palGalsup.c
new file mode 100644
index 0000000..115100d
--- /dev/null
+++ b/pal/palGalsup.c
@@ -0,0 +1,113 @@
+/*
+*+
+* Name:
+* palGalsup
+
+* Purpose:
+* Convert from galactic to supergalactic coordinates
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palGalsup ( double dl, double db, double *dsl, double *dsb );
+
+* Arguments:
+* dl = double (Given)
+* Galactic longitude.
+* db = double (Given)
+* Galactic latitude.
+* dsl = double * (Returned)
+* Supergalactic longitude.
+* dsb = double * (Returned)
+* Supergalactic latitude.
+
+* Description:
+* Transformation from IAU 1958 galactic coordinates to
+* de Vaucouleurs supergalactic coordinates.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* See Also:
+* - de Vaucouleurs, de Vaucouleurs, & Corwin, Second Reference
+* Catalogue of Bright Galaxies, U. Texas, page 8.
+* - Systems & Applied Sciences Corp., Documentation for the
+* machine-readable version of the above catalogue,
+* Contract NAS 5-26490.
+*
+* (These two references give different values for the galactic
+* longitude of the supergalactic origin. Both are wrong; the
+* correct value is L2=137.37.)
+
+* History:
+* 2012-02-12(TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+void palGalsup ( double dl, double db, double *dsl, double *dsb ) {
+
+ double v1[3];
+ double v2[3];
+
+/*
+* System of supergalactic coordinates:
+*
+* SGL SGB L2 B2 (deg)
+* - +90 47.37 +6.32
+* 0 0 - 0
+*
+* Galactic to supergalactic rotation matrix:
+*/
+ double rmat[3][3] = {
+ { -0.735742574804,+0.677261296414,+0.000000000000 },
+ { -0.074553778365,-0.080991471307,+0.993922590400 },
+ { +0.673145302109,+0.731271165817,+0.110081262225 }
+ };
+
+ /* Spherical to Cartesian */
+ iauS2c( dl, db, v1 );
+
+ /* Galactic to Supergalactic */
+ iauRxp( rmat, v1, v2 );
+
+ /* Cartesian to spherical */
+ iauC2s( v2, dsl, dsb );
+
+ /* Express in conventional ranges */
+ *dsl = iauAnp( *dsl );
+ *dsb = iauAnpm( *dsb );
+
+}
diff --git a/pal/palMappa.c b/pal/palMappa.c
new file mode 100644
index 0000000..e9729d6
--- /dev/null
+++ b/pal/palMappa.c
@@ -0,0 +1,119 @@
+/*
+*+
+* Name:
+* palMappa
+
+* Purpose:
+* Compute parameters needed by palAmpqk and palMapqk.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palMappa( double eq, double date, double amprms[21] )
+
+* Arguments:
+* eq = double (Given)
+* epoch of mean equinox to be used (Julian)
+* date = double (Given)
+* TDB (JD-2400000.5)
+* amprms = double[21] (Returned)
+* star-independent mean-to-apparent parameters:
+* (0) time interval for proper motion (Julian years)
+* (1-3) barycentric position of the Earth (AU)
+* (4-6) not used
+* (7) not used
+* (8-10) abv: barycentric Earth velocity in units of c
+* (11) sqrt(1-v**2) where v=modulus(abv)
+* (12-20) precession/nutation (3,3) matrix
+
+* Description:
+* Compute star-independent parameters in preparation for
+* transformations between mean place and geocentric apparent place.
+*
+* The parameters produced by this function are required in the
+* parallax, aberration, and nutation/bias/precession parts of the
+* mean/apparent transformations.
+*
+* The reference systems and timescales used are IAU 2006.
+
+* Notes:
+* - For date, the distinction between the required TDB and TT
+* is always negligible. Moreover, for all but the most
+* critical applications UTC is adequate.
+* - The vector amprms(1-3) is referred to the mean equinox and
+* equator of epoch eq.
+* - The parameters amprms produced by this function are used by
+* palAmpqk, palMapqk and palMapqkz.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-13 (PTW):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "palmac.h"
+#include "sofa.h"
+
+#include <string.h>
+
+void palMappa( double eq, double date, double amprms[21] ){
+
+/* Local Variables; */
+ int i;
+ double ebd[ 3 ], ehd[ 3 ], eh[ 3 ], e, vn[ 3 ], vm;
+
+/* Initialise so that unsused values are returned holding zero */
+ memset( amprms, 0, 21*sizeof( *amprms ) );
+
+/* Time interval for proper motion correction. */
+ amprms[ 0 ] = iauEpj( PAL__MJD0, date ) - eq;
+
+/* Get Earth barycentric and heliocentric position and velocity. */
+ palEvp( date, eq, ebd, &rms[ 1 ], ehd, eh );
+
+/* Heliocentric direction of Earth (normalized) and modulus. */
+ iauPn( eh, &e, &rms[ 4 ] );
+
+/* Aberration parameters. */
+ for( i = 0; i < 3; i++ ) {
+ amprms[ i + 8 ] = ebd[ i ]*PAL__CR;
+ }
+ iauPn( &rms[8], &vm, vn );
+ amprms[ 11 ] = sqrt( 1.0 - vm*vm );
+
+/* NPB matrix. */
+ palPrenut( eq, date, (double(*)[ 3 ]) &rms[ 12 ] );
+}
diff --git a/pal/palMapqkz.c b/pal/palMapqkz.c
new file mode 100644
index 0000000..7a1f12d
--- /dev/null
+++ b/pal/palMapqkz.c
@@ -0,0 +1,125 @@
+/*
+*+
+* Name:
+* palMapqkz
+
+* Purpose:
+* Quick mean to apparent place.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palMapqkz( double rm, double dm, double amprms[21],
+* double *ra, double *da )
+
+* Arguments:
+* rm = double (Given)
+* Mean RA (radians).
+* dm = double (Given)
+* Mean Dec (radians).
+* amprms = double[21] (Given)
+* Star-independent mean-to-apparent parameters (see palMappa):
+* (0-3) not used
+* (4-6) not used
+* (7) not used
+* (8-10) abv: barycentric Earth velocity in units of c
+* (11) sqrt(1-v**2) where v=modulus(abv)
+* (12-20) precession/nutation (3,3) matrix
+* ra = double * (Returned)
+* Apparent RA (radians).
+* da = double * (Returned)
+* Apparent Dec (radians).
+
+* Description:
+* Quick mean to apparent place: transform a star RA,dec from
+* mean place to geocentric apparent place, given the
+* star-independent parameters, and assuming zero parallax
+* and proper motion.
+*
+* Use of this function is appropriate when efficiency is important
+* and where many star positions, all with parallax and proper
+* motion either zero or already allowed for, and all referred to
+* the same equator and equinox, are to be transformed for one
+* epoch. The star-independent parameters can be obtained by
+* calling the palMappa function.
+*
+* The corresponding function for the case of non-zero parallax
+* and proper motion is palMapqk.
+*
+* The reference systems and timescales used are IAU 2006.
+*
+* Strictly speaking, the function is not valid for solar-system
+* sources, though the error will usually be extremely small.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-13 (PTW):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+void palMapqkz ( double rm, double dm, double amprms[21], double *ra,
+ double *da ){
+
+/* Local Variables: */
+ int i;
+ double ab1, abv[3], p[3], w, p1dv, p1dvp1, p2[3], p3[3];
+
+/* Unpack scalar and vector parameters. */
+ ab1 = amprms[11];
+ for( i = 0; i < 3; i++ ) {
+ abv[i] = amprms[i+8];
+ }
+
+/* Spherical to x,y,z. */
+ iauS2c( rm, dm, p );
+
+/* Aberration. */
+ p1dv = iauPdp( p, abv );
+ p1dvp1 = p1dv + 1.0;
+ w = 1.0 + p1dv / ( ab1 + 1.0 );
+ for( i = 0; i < 3; i++ ) {
+ p2[i] = ( ( ab1 * p[i] ) + ( w * abv[i] ) ) / p1dvp1;
+ }
+
+/* Precession and nutation. */
+ iauRxp( (double(*)[3]) &rms[12], p2, p3 );
+
+/* Geocentric apparent RA,dec. */
+ iauC2s( p3, ra, da );
+ *ra = iauAnp( *ra );
+}
diff --git a/pal/palOne2One.c b/pal/palOne2One.c
new file mode 100644
index 0000000..63756ab
--- /dev/null
+++ b/pal/palOne2One.c
@@ -0,0 +1,223 @@
+/*
+*+
+* Name:
+* palOne2One
+
+* Purpose:
+* File containing simple PAL wrappers for SLA routines that are identical in SOFA
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Description:
+* Some SOFA routines are identical to their SLA counterparts. PAL provides
+* direct counterparts to these although it is generally a better idea to
+* use the SOFA routine directly in new code.
+
+* Authors:
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* Notes:
+* - Do not call these functions from other PAL functions. Always use
+* the SOFA routines directly in new code.
+* - These are implemented as real functions rather than C preprocessor
+* macros so there may be a performance penalty in using the PAL
+* version instead of the SOFA version.
+* - Routines that take MJDs have SOFA equivalents that have an explicit
+* MJD offset included.
+* - palGeoc uses the WGS84 model.
+* - palGmst uses the IAU 2006 precession.
+
+* History:
+* 2012-02-10 (TIMJ):
+* Initial version
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "palmac.h"
+#include "sofa.h"
+
+void palCldj ( int iy, int im, int id, double *djm, int *j ) {
+ double djm0;
+ *j = iauCal2jd( iy, im, id, &djm0, djm );
+}
+
+double palDbear ( double a1, double b1, double a2, double b2 ) {
+ return iauPas( a1, b1, a2, b2 );
+}
+
+/* Arguments differ slightly. Assumes that the sign is always positive
+ and dealt with externally. */
+void palDaf2r ( int ideg, int iamin, double asec, double *rad, int *j ) {
+ *j = iauAf2a( ' ', ideg, iamin, asec, rad );
+}
+
+void palDav2m ( double axvec[3], double rmat[3][3] ) {
+ iauRv2m( axvec, rmat );
+}
+
+void palDcc2s ( double v[3], double *a, double *b ) {
+ iauC2s( v, a, b );
+}
+
+void palDcs2c ( double a, double b, double v[3] ) {
+ iauS2c( a, b, v );
+}
+
+void palDd2tf ( int ndp, double days, char *sign, int ihmsf[4] ) {
+ iauD2tf( ndp, days, sign, ihmsf );
+}
+
+void palDimxv ( double dm[3][3], double va[3], double vb[3] ) {
+ iauTrxp( dm, va, vb );
+}
+
+void palDm2av ( double rmat[3][3], double axvec[3] ) {
+ iauRm2v( rmat, axvec );
+}
+
+/* Requires additional SLA MJD reference date */
+void palDjcl ( double djm, int *iy, int *im, int *id, double *fd, int *j ) {
+ *j = iauJd2cal( PAL__MJD0, djm, iy, im, id, fd );
+}
+
+void palDmxm ( double a[3][3], double b[3][3], double c[3][3] ) {
+ iauRxr( a, b, c );
+}
+
+void palDmxv ( double dm[3][3], double va[3], double vb[3] ) {
+ iauRxp( dm, va, vb );
+}
+
+double palDpav ( double v1[3], double v2[3] ) {
+ return iauPap( v1, v2 );
+}
+
+double palDrange ( double angle ) {
+ return iauAnpm( angle );
+}
+
+double palDranrm ( double angle ) {
+ return iauAnp( angle );
+}
+
+double palDsep ( double a1, double b1, double a2, double b2 ) {
+ return iauSeps( a1, b1, a2, b2 );
+}
+
+double palDsepv ( double v1[3], double v2[3] ) {
+ return iauSepp( v1, v2 );
+}
+
+/* Assumes that the sign is always positive and is dealt with externally */
+void palDtf2d ( int ihour, int imin, double sec, double *days, int *j ) {
+ *j = iauTf2d( ' ', ihour, imin, sec, days );
+}
+
+/* Assumes that the sign is dealt with outside this routine */
+void palDtf2r ( int ihour, int imin, double sec, double *rad, int *j ) {
+ *j = iauTf2a( ' ', ihour, imin, sec, rad );
+}
+
+double palDvdv ( double va[3], double vb[3] ) {
+ return iauPdp( va, vb );
+}
+
+/* Note that the arguments are flipped */
+void palDvn ( double v[3], double uv[3], double *vm ) {
+ iauPn( v, vm, uv );
+}
+
+void palDvxv ( double va[3], double vb[3], double vc[3] ) {
+ iauPxp( va, vb, vc );
+}
+
+/* Requires additional SLA MJD reference date */
+double palEpb ( double date ) {
+ return iauEpb( PAL__MJD0, date );
+}
+
+double palEpb2d ( double epb ) {
+ double djm0, djm;
+ iauEpb2jd( epb, &djm0, &djm );
+ return djm;
+}
+
+/* Requires additional SLA MJD reference date */
+double palEpj ( double date ) {
+ return iauEpj( PAL__MJD0, date );
+}
+
+double palEpj2d ( double epj ) {
+ double djm0, djm;
+ iauEpj2jd( epj, &djm0, &djm );
+ return djm;
+}
+
+/* Requires additional SLA MJD reference date */
+double palEqeqx ( double date ) {
+ return iauEe06a( PAL__MJD0, date );
+}
+
+/* Do not use palEvp just yet */
+
+void palFk5hz ( double r5, double d5, double epoch,
+ double *rh, double *dh ) {
+ /* Need to convert epoch to Julian date first */
+ double date1, date2;
+ iauEpj2jd( epoch, &date1, &date2 );
+ iauFk5hz( r5, d5, date1, date2, rh, dh );
+}
+
+void palGeoc ( double p, double h, double *r, double *z ) {
+ double xyz[3];
+ const double elong = 0.0; /* Use zero longitude */
+ const double AU = 1.49597870E11;
+ /* WGS84 looks to be the closest match */
+ iauGd2gc( 1, elong, p, h, xyz );
+ *r = xyz[0] / (AU * cos(elong) );
+ *z = xyz[2] / AU;
+}
+
+/* Note that SOFA has more accurate time arguments and we use the 2006 precession model */
+double palGmst ( double ut1 ) {
+ return iauGmst06( PAL__MJD0, ut1, PAL__MJD0, ut1 );
+}
+
+void palHfk5z ( double rh, double dh, double epoch,
+ double *r5, double *d5, double *dr5, double *dd5 ) {
+ /* Need to convert epoch to Julian date first */
+ double date1, date2;
+ iauEpj2jd( epoch, &date1, &date2 );
+ iauHfk5z( rh, dh, date1, date2, r5, d5, dr5, dd5 );
+}
+
diff --git a/pal/palPrebn.c b/pal/palPrebn.c
new file mode 100644
index 0000000..b85bee4
--- /dev/null
+++ b/pal/palPrebn.c
@@ -0,0 +1,95 @@
+/*
+*+
+* Name:
+* palPrebn
+
+* Purpose:
+* Generate the matrix of precession between two objects (old)
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palPrebn ( double bep0, double bep1, double rmatp[3][3] );
+
+* Arguments:
+* bep0 = double (Given)
+* Beginning Besselian epoch.
+* bep1 = double (Given)
+* Ending Besselian epoch
+* rmatp = double[3][3] (Returned)
+* precession matrix in the sense V(BEP1) = RMATP * V(BEP0)
+
+* Description:
+* Generate the matrix of precession between two epochs,
+* using the old, pre-IAU1976, Bessel-Newcomb model, using
+* Kinoshita's formulation
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* See Also:
+* Kinoshita, H. (1975) 'Formulas for precession', SAO Special
+* Report No. 364, Smithsonian Institution Astrophysical
+* Observatory, Cambridge, Massachusetts.
+
+* History:
+* 2012-02-12(TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "palmac.h"
+
+void palPrebn ( double bep0, double bep1, double rmatp[3][3] ) {
+
+ double t,bigt, zeta, theta, z, tas2r, w;
+
+ /* Interval between basic epoch B1850.0 and beginning epoch in TC */
+ bigt = (bep0-1850)/100.;
+
+ /* Interval over which precession required, in tropical centuries */
+ t = (bep1-bep0)/100.;
+
+ /* Euler angles */
+ tas2r = t * PAL__DAS2R;
+ w = 2303.5548 + ( 1.39720 + 0.000059 * bigt) * bigt;
+
+ zeta = ( w + ( 0.30242 - 0.000269 * bigt + 0.017996 * t ) * t ) * tas2r;
+ z = ( w + ( 1.09478 + 0.000387 * bigt + 0.018324 * t ) * t ) * tas2r;
+ theta = ( 2005.1125 + ( -0.85294 - 0.000365 * bigt ) * bigt +
+ (-0.42647 - 0.000365 * bigt - 0.041802 * t ) * t ) * tas2r;
+
+ /* Rotation matrix */
+ palDeuler("ZYZ", -zeta, theta, -z, rmatp);
+
+}
diff --git a/pal/palPrec.c b/pal/palPrec.c
new file mode 100644
index 0000000..db1ae12
--- /dev/null
+++ b/pal/palPrec.c
@@ -0,0 +1,106 @@
+/*
+*+
+* Name:
+* palPrec
+
+* Purpose:
+* Form the matrix of precession between two epochs (IAU 2006)
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* palPrec( double ep0, double ep1, double rmatp[3][3] )
+
+* Arguments:
+* ep0 = double (Given)
+* Beginning epoch
+* ep1 = double (Given)
+* Ending epoch
+* rmatp = double[3][3] (Returned)
+* Precession matrix
+
+* Description:
+* The IAU 2006 precession matrix from ep0 to ep1 is found and
+* returned. The matrix is in the sense V(EP1) = RMATP * V(EP0).
+* The epochs are TDB (loosely TT) Julian epochs.
+*
+* Though the matrix method itself is rigorous, the precession
+* angles are expressed through canonical polynomials which are
+* valid only for a limited time span of a few hundred years around
+* the current epoch.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* DSB: David Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-10 (DSB):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+#include "sofam.h"
+
+void palPrec( double ep0, double ep1, double rmatp[3][3] ){
+
+/* Local Variables: */
+ double rmatq[3][3];
+ double ep0_days;
+ double ep1_days;
+
+/* Convert supplied dates to days since J2000 */
+ ep0_days = ( ep0 - 2000.0 )*DJY;
+ ep1_days = ( ep1 - 2000.0 )*DJY;
+
+/* If beginning epoch is J2000, just return the rotation matrix from
+ J2000 to EP1. */
+ if( ep0 == 2000.0 ) {
+ iauPmat06( DJ00, ep1_days, rmatp );
+
+/* If end epoch is J2000, get the rotation matrix from J2000 to EP0 and
+ then transpose it to get the rotation matrix from EP0 to J2000. */
+ } else if( ep1 == 2000.0 ) {
+ iauPmat06( DJ00, ep0_days, rmatp );
+ iauTr( rmatp, rmatp );
+
+/* Otherwise. get the two matrices used above and multiply them
+ together. */
+ } else {
+ iauPmat06( DJ00, ep0_days, rmatp );
+ iauTr( rmatp, rmatp );
+ iauPmat06( DJ00, ep1_days, rmatq );
+ iauRxr( rmatp, rmatq, rmatp );
+ }
+
+}
diff --git a/pal/palPrenut.c b/pal/palPrenut.c
new file mode 100644
index 0000000..41cfde6
--- /dev/null
+++ b/pal/palPrenut.c
@@ -0,0 +1,110 @@
+/*
+*+
+* Name:
+* palPrenut
+
+* Purpose:
+* Form the matrix of bias-precession-nutation (IAU 2006/2000A)
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palPrenut( double epoch, double date, double rmatpn[3][3] )
+
+* Arguments:
+* epoch = double (Returned)
+* Julian epoch for mean coordinates.
+* date = double (Returned)
+* Modified Julian Date (JD-2400000.5) for true coordinates.
+* rmatpn = double[3][3] (Returned)
+* combined NPB matrix
+
+* Description:
+* Form the matrix of bias-precession-nutation (IAU 2006/2000A).
+* The epoch and date are TT (but TDB is usually close enough).
+* The matrix is in the sense v(true) = rmatpn * v(mean).
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-10 (PTW):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "palmac.h"
+#include "sofa.h"
+
+void palPrenut ( double epoch, double date, double rmatpn[3][3] ){
+
+/* Local Variables: */
+ double bpa;
+ double bpia;
+ double bqa;
+ double chia;
+ double d1;
+ double d2;
+ double eps0;
+ double epsa;
+ double gam;
+ double oma;
+ double pa;
+ double phi;
+ double pia;
+ double psi;
+ double psia;
+ double r1[3][3];
+ double r2[3][3];
+ double thetaa;
+ double za;
+ double zetaa;
+
+/* Specified Julian epoch as a 2-part JD. */
+ iauEpj2jd( epoch, &d1, &d2 );
+
+/* P matrix, from specified epoch to J2000.0. */
+ iauP06e( d1, d2, &eps0, &psia, &oma, &bpa, &bqa, &pia, &bpia, &epsa,
+ &chia, &za, &zetaa, &thetaa, &pa, &gam, &phi, &psi );
+ iauIr( r1 );
+ iauRz( -chia, r1 );
+ iauRx( oma, r1 );
+ iauRz( psia, r1 );
+ iauRx( -eps0, r1 );
+
+/* NPB matrix, from J2000.0 to date. */
+ iauPnm06a( PAL__MJD0, date, r2 );
+
+/* NPB matrix, from specified epoch to date. */
+ iauRxr( r2, r1, rmatpn );
+}
diff --git a/pal/palPvobs.c b/pal/palPvobs.c
new file mode 100644
index 0000000..b8ff5a3
--- /dev/null
+++ b/pal/palPvobs.c
@@ -0,0 +1,106 @@
+/*
+*+
+* Name:
+* palPvobs
+
+* Purpose:
+* Position and velocity of an observing station.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* palPvobs( double p, double h, double stl, double pv[6] )
+
+* Arguments:
+* p = double (Given)
+* Latitude (geodetic, radians).
+* h = double (Given)
+* Height above reference spheroid (geodetic, metres).
+* stl = double (Given)
+* Local apparent sidereal time (radians).
+* pv = double[ 6 ] (Returned)
+* position/velocity 6-vector (AU, AU/s, true equator
+* and equinox of date).
+
+* Description:
+* Returns the position and velocity of an observing station.
+
+* Notes:
+* - The WGS84 reference ellipsoid is used.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* DSB: David Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-16 (DSB):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "palmac.h"
+#include "palmac.h"
+#include "sofam.h"
+
+void palPvobs( double p, double h, double stl, double pv[6] ){
+
+/* Local Variables: */
+ double xyz[3], z, r, s, c, v;
+
+/* Geodetic to geocentric conversion (WGS84 reference ellipsoid). */
+ iauGd2gc( 1, 0.0, p, h, xyz );
+
+/* Convert from metres to AU */
+ r = xyz[ 0 ]/DAU;
+ z = xyz[ 2 ]/DAU;
+
+/* Functions of ST. */
+ s = sin( stl );
+ c = cos( stl );
+
+/* Speed. */
+ v = PAL__SR*r;
+
+/* Position. */
+ pv[ 0 ] = r*c;
+ pv[ 1 ] = r*s;
+ pv[ 2 ] = z;
+
+/* Velocity. */
+ pv[ 3 ] = -v*s;
+ pv[ 4 ] = v*c;
+ pv[ 5 ] = 0.0;
+
+}
+
+
diff --git a/pal/palRvgalc.c b/pal/palRvgalc.c
new file mode 100644
index 0000000..3bccd2d
--- /dev/null
+++ b/pal/palRvgalc.c
@@ -0,0 +1,109 @@
+/*
+*+
+* Name:
+* palRvgalc
+
+* Purpose:
+* Velocity component in a given direction due to the rotation
+* of the Galaxy.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* double palRvgalc( double r2000, double d2000 )
+
+* Arguments:
+* r2000 = double (Given)
+* J2000.0 mean RA (radians)
+* d2000 = double (Given)
+* J2000.0 mean Dec (radians)
+
+* Returned Value:
+* Component of dynamical LSR motion in direction R2000,D2000 (km/s).
+
+* Description:
+* This function returns the Component of dynamical LSR motion in
+* the direction of R2000,D2000. The result is +ve when the dynamical
+* LSR is receding from the given point on the sky.
+*
+* Notes:
+* - The Local Standard of Rest used here is a point in the
+* vicinity of the Sun which is in a circular orbit around
+* the Galactic centre. Sometimes called the "dynamical" LSR,
+* it is not to be confused with a "kinematical" LSR, which
+* is the mean standard of rest of star catalogues or stellar
+* populations.
+*
+* Reference:
+* - The orbital speed of 220 km/s used here comes from Kerr &
+* Lynden-Bell (1986), MNRAS, 221, p1023.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* DSB: David Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-16 (DSB):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+double palRvgalc( double r2000, double d2000 ){
+
+/* Local Variables: */
+ double vb[ 3 ];
+
+/*
+* LSR velocity due to Galactic rotation
+*
+* Speed = 220 km/s
+* Apex = L2,B2 90deg, 0deg
+* = RA,Dec 21 12 01.1 +48 19 47 J2000.0
+*
+* This is expressed in the form of a J2000.0 x,y,z vector:
+*
+* VA(1) = X = -SPEED*COS(RA)*COS(DEC)
+* VA(2) = Y = -SPEED*SIN(RA)*COS(DEC)
+* VA(3) = Z = -SPEED*SIN(DEC)
+*/
+
+ double va[ 3 ] = { -108.70408, +97.86251, -164.33610 };
+
+/* Convert given J2000 RA,Dec to x,y,z. */
+ iauS2c( r2000, d2000, vb );
+
+/* Compute dot product with LSR motion vector. */
+ return iauPdp( va, vb );
+}
diff --git a/pal/palRvlg.c b/pal/palRvlg.c
new file mode 100644
index 0000000..0caf688
--- /dev/null
+++ b/pal/palRvlg.c
@@ -0,0 +1,104 @@
+/*
+*+
+* Name:
+* palRvlg
+
+* Purpose:
+* Velocity component in a given direction due to Galactic rotation
+* and motion of the local group.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* double palRvlg( double r2000, double d2000 )
+
+* Arguments:
+* r2000 = double (Given)
+* J2000.0 mean RA (radians)
+* d2000 = double (Given)
+* J2000.0 mean Dec (radians)
+
+* Returned Value:
+* Component of SOLAR motion in direction R2000,D2000 (km/s).
+
+* Description:
+* This function returns the velocity component in a given
+* direction due to the combination of the rotation of the
+* Galaxy and the motion of the Galaxy relative to the mean
+* motion of the local group. The result is +ve when the Sun
+* is receding from the given point on the sky.
+*
+* Reference:
+* - IAU Trans 1976, 168, p201.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* DSB: David Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-16 (DSB):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+double palRvlg( double r2000, double d2000 ){
+
+/* Local Variables: */
+ double vb[ 3 ];
+
+/*
+*
+* Solar velocity due to Galactic rotation and translation
+*
+* Speed = 300 km/s
+*
+* Apex = L2,B2 90deg, 0deg
+* = RA,Dec 21 12 01.1 +48 19 47 J2000.0
+*
+* This is expressed in the form of a J2000.0 x,y,z vector:
+*
+* VA(1) = X = -SPEED*COS(RA)*COS(DEC)
+* VA(2) = Y = -SPEED*SIN(RA)*COS(DEC)
+* VA(3) = Z = -SPEED*SIN(DEC)
+*/
+
+ double va[ 3 ] = { -148.23284, +133.44888, -224.09467 };
+
+/* Convert given J2000 RA,Dec to x,y,z. */
+ iauS2c( r2000, d2000, vb );
+
+/* Compute dot product with Solar motion vector. */
+ return iauPdp( va, vb );
+}
diff --git a/pal/palRvlsrd.c b/pal/palRvlsrd.c
new file mode 100644
index 0000000..22ae8b9
--- /dev/null
+++ b/pal/palRvlsrd.c
@@ -0,0 +1,114 @@
+/*
+*+
+* Name:
+* palRvlsrd
+
+* Purpose:
+* Velocity component in a given direction due to the Sun's motion
+* with respect to the dynamical Local Standard of Rest.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* double palRvlsrd( double r2000, double d2000 )
+
+* Arguments:
+* r2000 = double (Given)
+* J2000.0 mean RA (radians)
+* d2000 = double (Given)
+* J2000.0 mean Dec (radians)
+
+* Returned Value:
+* Component of "peculiar" solar motion in direction R2000,D2000 (km/s).
+
+* Description:
+* This function returns the velocity component in a given direction
+* due to the Sun's motion with respect to the dynamical Local Standard
+* of Rest. The result is +ve when the Sun is receding from the given
+* point on the sky.
+
+* Notes:
+* - The Local Standard of Rest used here is the "dynamical" LSR,
+* a point in the vicinity of the Sun which is in a circular orbit
+* around the Galactic centre. The Sun's motion with respect to the
+* dynamical LSR is called the "peculiar" solar motion.
+* - There is another type of LSR, called a "kinematical" LSR. A
+* kinematical LSR is the mean standard of rest of specified star
+* catalogues or stellar populations, and several slightly different
+* kinematical LSRs are in use. The Sun's motion with respect to an
+* agreed kinematical LSR is known as the "standard" solar motion.
+* To obtain a radial velocity correction with respect to an adopted
+* kinematical LSR use the routine sla_RVLSRK.
+
+* Reference:
+* - Delhaye (1965), in "Stars and Stellar Systems", vol 5, p73.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* DSB: David Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-16 (DSB):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+double palRvlsrd( double r2000, double d2000 ){
+
+/* Local Variables: */
+ double vb[ 3 ];
+
+/*
+* Peculiar solar motion from Delhaye 1965: in Galactic Cartesian
+* coordinates (+9,+12,+7) km/s. This corresponds to about 16.6 km/s
+* towards Galactic coordinates L2 = 53 deg, B2 = +25 deg, or RA,Dec
+* 17 49 58.7 +28 07 04 J2000.
+*
+* The solar motion is expressed here in the form of a J2000.0
+* equatorial Cartesian vector:
+*
+* VA(1) = X = -SPEED*COS(RA)*COS(DEC)
+* VA(2) = Y = -SPEED*SIN(RA)*COS(DEC)
+* VA(3) = Z = -SPEED*SIN(DEC)
+*/
+
+ double va[ 3 ] = { +0.63823, +14.58542, -7.80116 };
+
+/* Convert given J2000 RA,Dec to x,y,z. */
+ iauS2c( r2000, d2000, vb );
+
+/* Compute dot product with Solar motion vector. */
+ return iauPdp( va, vb );
+}
diff --git a/pal/palRvlsrk.c b/pal/palRvlsrk.c
new file mode 100644
index 0000000..590f895
--- /dev/null
+++ b/pal/palRvlsrk.c
@@ -0,0 +1,114 @@
+/*
+*+
+* Name:
+* palRvlsrk
+
+* Purpose:
+* Velocity component in a given direction due to the Sun's motion
+* with respect to an adopted kinematic Local Standard of Rest.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* double palRvlsrk( double r2000, double d2000 )
+
+* Arguments:
+* r2000 = double (Given)
+* J2000.0 mean RA (radians)
+* d2000 = double (Given)
+* J2000.0 mean Dec (radians)
+
+* Returned Value:
+* Component of "standard" solar motion in direction R2000,D2000 (km/s).
+
+* Description:
+* This function returns the velocity component in a given direction
+* due to the Sun's motion with respect to an adopted kinematic
+* Local Standard of Rest. The result is +ve when the Sun is receding
+* from the given point on the sky.
+
+* Notes:
+* - The Local Standard of Rest used here is one of several
+* "kinematical" LSRs in common use. A kinematical LSR is the mean
+* standard of rest of specified star catalogues or stellar
+* populations. The Sun's motion with respect to a kinematical LSR
+* is known as the "standard" solar motion.
+* - There is another sort of LSR, the "dynamical" LSR, which is a
+* point in the vicinity of the Sun which is in a circular orbit
+* around the Galactic centre. The Sun's motion with respect to
+* the dynamical LSR is called the "peculiar" solar motion. To
+* obtain a radial velocity correction with respect to the
+* dynamical LSR use the routine sla_RVLSRD.
+
+* Reference:
+* - Delhaye (1965), in "Stars and Stellar Systems", vol 5, p73.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* DSB: David Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 2012-02-16 (DSB):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+double palRvlsrk( double r2000, double d2000 ){
+
+/* Local Variables: */
+ double vb[ 3 ];
+
+/*
+* Standard solar motion (from Methods of Experimental Physics, ed Meeks,
+* vol 12, part C, sec 6.1.5.2, p281):
+*
+* 20 km/s towards RA 18h Dec +30d (1900).
+*
+* The solar motion is expressed here in the form of a J2000.0
+* equatorial Cartesian vector:
+*
+* VA(1) = X = -SPEED*COS(RA)*COS(DEC)
+* VA(2) = Y = -SPEED*SIN(RA)*COS(DEC)
+* VA(3) = Z = -SPEED*SIN(DEC)
+*/
+
+ double va[ 3 ] = { -0.29000, +17.31726, -10.00141 };
+
+/* Convert given J2000 RA,Dec to x,y,z. */
+ iauS2c( r2000, d2000, vb );
+
+/* Compute dot product with Solar motion vector. */
+ return iauPdp( va, vb );
+}
diff --git a/pal/palSubet.c b/pal/palSubet.c
new file mode 100644
index 0000000..8f879b1
--- /dev/null
+++ b/pal/palSubet.c
@@ -0,0 +1,109 @@
+/*
+*+
+* Name:
+* palSubet
+
+* Purpose:
+* Remove the E-terms from a pre IAU 1976 catalogue RA,Dec
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palSubet ( double rc, double dc, double eq,
+* double *rm, double *dm );
+
+* Arguments:
+* rc = double (Given)
+* RA with E-terms included (radians)
+* dc = double (Given)
+* Dec with E-terms included (radians)
+* eq = double (Given)
+* Besselian epoch of mean equator and equinox
+* rm = double * (Returned)
+* RA without E-terms (radians)
+* dm = double * (Returned)
+* Dec without E-terms (radians)
+
+* Description:
+* Remove the E-terms (elliptic component of annual aberration)
+* from a pre IAU 1976 catalogue RA,Dec to give a mean place.
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* Notes:
+* Most star positions from pre-1984 optical catalogues (or
+* derived from astrometry using such stars) embody the
+* E-terms. This routine converts such a position to a
+* formal mean place (allowing, for example, comparison with a
+* pulsar timing position).
+
+* See Also:
+* Explanatory Supplement to the Astronomical Ephemeris,
+* section 2D, page 48.
+
+* History:
+* 2012-02-12(TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+void palSubet ( double rc, double dc, double eq, double *rm, double *dm ) {
+ double a[3]; /* The E-terms */
+ double v[3];
+ double f;
+ int i;
+
+ /* Note the preference for IAU routines */
+
+ /* Retrieve the E-terms */
+ palEtrms( eq, a );
+
+ /* Spherical to Cartesian */
+ iauS2c( rc, dc, v );
+
+ /* Include the E-terms */
+ f = 1.0 + iauPdp( v, a );
+ for (i=0; i<3; i++) {
+ v[i] = f*v[i] - a[i];
+ }
+
+ /* Cartesian to spherical */
+ iauC2s( v, rm, dm );
+
+ /* Bring RA into conventional range */
+ *rm = iauAnp( *rm );
+
+}
diff --git a/pal/palSupgal.c b/pal/palSupgal.c
new file mode 100644
index 0000000..1096a7a
--- /dev/null
+++ b/pal/palSupgal.c
@@ -0,0 +1,113 @@
+/*
+*+
+* Name:
+* palSupgal
+
+* Purpose:
+* Convert from supergalactic to galactic coordinates
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Library routine
+
+* Invocation:
+* void palSupgal ( double dsl, double dsb, double *dl, double *db );
+
+* Arguments:
+* dsl = double (Given)
+* Supergalactic longitude.
+* dsb = double (Given)
+* Supergalactic latitude.
+* dl = double * (Returned)
+* Galactic longitude.
+* db = double * (Returned)
+* Galactic latitude.
+
+* Description:
+* Transformation from de Vaucouleurs supergalactic coordinates
+* to IAU 1958 galactic coordinates
+
+* Authors:
+* PTW: Pat Wallace (STFC)
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* See Also:
+* - de Vaucouleurs, de Vaucouleurs, & Corwin, Second Reference
+* Catalogue of Bright Galaxies, U. Texas, page 8.
+* - Systems & Applied Sciences Corp., Documentation for the
+* machine-readable version of the above catalogue,
+* Contract NAS 5-26490.
+*
+* (These two references give different values for the galactic
+* longitude of the supergalactic origin. Both are wrong; the
+* correct value is L2=137.37.)
+
+* History:
+* 2012-02-12(TIMJ):
+* Initial version with documentation taken from Fortran SLA
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "sofa.h"
+
+void palSupgal ( double dsl, double dsb, double *dl, double *db ) {
+
+ double v1[3];
+ double v2[3];
+
+/*
+* System of supergalactic coordinates:
+*
+* SGL SGB L2 B2 (deg)
+* - +90 47.37 +6.32
+* 0 0 - 0
+*
+* Galactic to supergalactic rotation matrix:
+*/
+ double rmat[3][3] = {
+ { -0.735742574804,+0.677261296414,+0.000000000000 },
+ { -0.074553778365,-0.080991471307,+0.993922590400 },
+ { +0.673145302109,+0.731271165817,+0.110081262225 }
+ };
+
+ /* Spherical to Cartesian */
+ iauS2c( dsl, dsb, v1 );
+
+ /* Supergalactic to galactic */
+ iauTrxp( rmat, v1, v2 );
+
+ /* Cartesian to spherical */
+ iauC2s( v2, dl, db );
+
+ /* Express in conventional ranges */
+ *dl = iauAnp( *dl );
+ *db = iauAnpm( *db );
+
+}
diff --git a/pal/palmac.h b/pal/palmac.h
new file mode 100644
index 0000000..9b9b17b
--- /dev/null
+++ b/pal/palmac.h
@@ -0,0 +1,97 @@
+#ifndef PALMACDEF
+#define PALMACDEF
+
+/*
+*+
+* Name:
+* palmac.h
+
+* Purpose:
+* Macros used by the PAL library
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Include file
+
+* Description:
+* A collection of useful macros provided and used by the PAL library
+
+* Authors:
+* TIMJ: Tim Jenness (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* Notes:
+*
+
+* History:
+* 2012-02-08 (TIMJ):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+/* Pi */
+static const double PAL__DPI = 3.1415926535897932384626433832795028841971693993751;
+
+/* 2Pi */
+static const double PAL__D2PI = 6.2831853071795864769252867665590057683943387987502;
+
+/* pi/180: degrees to radians */
+static const double PAL__DD2R = 0.017453292519943295769236907684886127134428718885417;
+
+/* Radians to arcseconds */
+static const double PAL__DR2AS = 2.0626480624709635515647335733077861319665970087963e5;
+
+/* Arcseconds to radians */
+static const double PAL__DAS2R = 4.8481368110953599358991410235794797595635330237270e-6;
+
+/* Start of SLA modified Julian date epoch */
+static const double PAL__MJD0 = 2400000.5;
+
+/* Light time for 1 AU (sec) */
+static const double PAL__CR = 499.004782;
+
+/* Km per sec to AU per tropical century
+ = 86400 * 36524.2198782 / 149597870 */
+static const double PAL__VF = 21.095;
+
+/* Radians per year to arcsec per century. Note - must be a macro since
+ its value is not a literal constant (i.e. it refers to PAL__D2PI). */
+#define PAL__PMF (100.0*60.0*60.0*360.0/PAL__D2PI)
+
+/* Mean sidereal rate - the rotational angular velocity of Earth
+ in radians/sec from IERS Conventions (2003). */
+static const double PAL__SR = 7.2921150e-5;
+
+/* DNINT(A) - round to nearest whole number (double) */
+#define DNINT(A) ((A)<0.0?ceil((A)-0.5):floor((A)+0.5))
+
+
+
+
+#endif
diff --git a/pal2ast.h b/pal2ast.h
new file mode 100644
index 0000000..52e61b7
--- /dev/null
+++ b/pal2ast.h
@@ -0,0 +1,134 @@
+#if !defined( PAL2AST_INCLUDED ) /* Include this file only once */
+#define PAL2AST_INCLUDED
+/*
+* Name:
+* pal2ast.h
+
+* Type:
+* C include file.
+
+* Purpose:
+* Defines new names for symbols exported by the PAL library.
+
+* Invocation:
+* #include "pal2ast.h"
+
+* Description:
+* This include file defines a new name for each public function
+* defined by the pal library. The names defined by PAL itself are
+* of the form "palXxx" (e.g. palPvobs) - this include file defines
+* a macro that translates each such name to the form "astPalXxx"
+* (e.g. astPalPvobs). This is done so that the names do not clash
+* with any external PAL library with which the application is linked.
+*
+* It should be included at the start of any AST source file that refers
+* to PAL functions using the standard names (e.g. palPvobs).
+
+* Copyright:
+* Copyright (C) 2012 Science & Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public Licence as
+* published by the Free Software Foundation; either version 2 of
+* the Licence, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful,but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public Licence for more details.
+*
+* You should have received a copy of the GNU General Public Licence
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street,Fifth Floor, Boston, MA
+* 02110-1301, USA
+
+* Authors:
+* DSB: D.S. Berry (Starlink)
+
+* History:
+* 16-FEB-2012 (DSB):
+* Original version.
+*/
+
+/* Rename all PAL functions */
+#define palAddet astPalAddet
+#define palAmpqk astPalAmpqk
+#define palCaldj astPalCaldj
+#define palDat astPalDat
+#define palDe2h astPalDe2h
+#define palDeuler astPalDeuler
+#define palDh2e astPalDh2e
+#define palDjcal astPalDjcal
+#define palDmat astPalDmat
+#define palDs2tp astPalDs2tp
+#define palDtp2s astPalDtp2s
+#define palDtps2c astPalDtps2c
+#define palDtt astPalDtt
+#define palEcmat astPalEcmat
+#define palEqgal astPalEqgal
+#define palEtrms astPalEtrms
+#define palEvp astPalEvp
+#define palFk45z astPalFk45z
+#define palFk524 astPalFk524
+#define palFk54z astPalFk54z
+#define palGaleq astPalGaleq
+#define palGalsup astPalGalsup
+#define palMappa astPalMappa
+#define palMapqkz astPalMapqkz
+#define palPrebn astPalPrebn
+#define palPrec astPalPrec
+#define palPrenut astPalPrenut
+#define palPvobs astPalPvobs
+#define palRvgalc astPalRvgalc
+#define palRvlg astPalRvlg
+#define palRvlsrd astPalRvlsrd
+#define palRvlsrk astPalRvlsrk
+#define palSubet astPalSubet
+#define palSupgal astPalSupgal
+#define palCldj astPalCldj
+#define palDaf2r astPalDaf2r
+#define palDav2m astPalDav2m
+#define palDbear astPalDbear
+#define palDcc2s astPalDcc2s
+#define palDcs2c astPalDcs2c
+#define palDd2tf astPalDd2tf
+#define palDimxv astPalDimxv
+#define palDjcl astPalDjcl
+#define palDm2av astPalDm2av
+#define palDmxm astPalDmxm
+#define palDmxv astPalDmxv
+#define palDpav astPalDpav
+#define palDrange astPalDrange
+#define palDranrm astPalDranrm
+#define palDsep astPalDsep
+#define palDsepv astPalDsepv
+#define palDtf2d astPalDtf2d
+#define palDtf2r astPalDtf2r
+#define palDvdv astPalDvdv
+#define palDvn astPalDvn
+#define palDvxv astPalDvxv
+#define palEpb astPalEpb
+#define palEpb2d astPalEpb2d
+#define palEpj astPalEpj
+#define palEpj2d astPalEpj2d
+#define palEqeqx astPalEqeqx
+#define palFk5hz astPalFk5hz
+#define palGeoc astPalGeoc
+#define palGmst astPalGmst
+#define palHfk5z astPalHfk5z
+
+/* Rename all PAL global variables */
+#define PAL__DPI AST__PALDPI
+#define PAL__D2PI AST__PALD2PI
+#define PAL__DD2R AST__PALDD2R
+#define PAL__DR2AS AST__PALDR2AS
+#define PAL__DAS2R AST__PALDAS2R
+#define PAL__MJD0 AST__PALMJD0
+#define PAL__CR AST__PALCR
+#define PAL__VF AST__PALVF
+#define PAL__SR AST__PALSR
+
+
+#endif
diff --git a/polymap.c b/polymap.c
index ada5079..4281b30 100644
--- a/polymap.c
+++ b/polymap.c
@@ -1777,7 +1777,7 @@ static void IterInverse( AstPolyMap *this, AstPointSet *out, AstPointSet *result
/* Allocate memory to hold the offset vector. */
vec = astMalloc( sizeof( double )*ncoord );
-/* Allocate memory to hold work space for palSlaDmat. */
+/* Allocate memory to hold work space for palDmat. */
iw = astMalloc( sizeof( int )*ncoord );
/* Check pointers can be used safely. */
@@ -1862,7 +1862,7 @@ static void IterInverse( AstPolyMap *this, AstPointSet *out, AstPointSet *result
/* Find the corresponding offset from the current input position to the required
input position. */
- palSlaDmat( ncoord, mat, vec, &det, &sing, iw );
+ palDmat( ncoord, mat, vec, &det, &sing, iw );
/* If the matrix was singular, the input position cannot be evaluated so
store a bad value for it and indicate it has converged. */
diff --git a/proj.c b/proj.c
index 3a51d51..d604433 100644
--- a/proj.c
+++ b/proj.c
@@ -15,7 +15,7 @@
*
* You should have received a copy of the GNU Library General Public License
* along with this library; if not, write to the Free Software Foundation,
-* Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
+* Inc., 51 Franklin Street,Fifth Floor, Boston, MA 02110-1301, USA
*
* Correspondence concerning WCSLIB may be directed to:
* Internet email: mcalabre at atnf.csiro.au
diff --git a/proj.h b/proj.h
index c832867..d4b4467 100644
--- a/proj.h
+++ b/proj.h
@@ -15,7 +15,7 @@
*
* You should have received a copy of the GNU Library General Public License
* along with this library; if not, write to the Free Software Foundation,
-* Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
+* Inc., 51 Franklin Street,Fifth Floor, Boston, MA 02110-1301, USA
*
* Correspondence concerning WCSLIB may be directed to:
* Internet email: mcalabre at atnf.csiro.au
diff --git a/skyaxis.c b/skyaxis.c
index 8dc80f3..a550304 100644
--- a/skyaxis.c
+++ b/skyaxis.c
@@ -447,7 +447,7 @@ static double AxisDistance( AstAxis *this_axis, double v1, double v2, int *statu
/* Check both axis values are OK, and form the returned increment,
normalizing it into the range +PI to -PI. */
- if( v1 != AST__BAD && v2 != AST__BAD ) result = palSlaDrange( v2 - v1 );
+ if( v1 != AST__BAD && v2 != AST__BAD ) result = palDrange( v2 - v1 );
/* Return the result. */
return result;
@@ -1093,8 +1093,8 @@ static void AxisNorm( AstAxis *this_axis, double *value, int *status ) {
centrezero = astGetAxisCentreZero( this );
/* Wrap the value into the appropriate range. */
- if ( astOK ) *value = centrezero ? palSlaDrange( *value ) :
- palSlaDranrm( *value );
+ if ( astOK ) *value = centrezero ? palDrange( *value ) :
+ palDranrm( *value );
}
}
@@ -3148,9 +3148,9 @@ void astInitSkyAxisVtab_( AstSkyAxisVtab *vtab, const char *name, int *status )
/* Initialize constants for converting between hours, degrees and radians. */
LOCK_MUTEX2
- palSlaDtf2r( 1, 0, 0.0, &hr2rad, &stat );
- palSlaDaf2r( 1, 0, 0.0, °2rad, &stat );
- palSlaDaf2r( 180, 0, 0.0, &pi, &stat );
+ palDtf2r( 1, 0, 0.0, &hr2rad, &stat );
+ palDaf2r( 1, 0, 0.0, °2rad, &stat );
+ palDaf2r( 180, 0, 0.0, &pi, &stat );
piby2 = 0.5*pi;
UNLOCK_MUTEX2
diff --git a/skyframe.c b/skyframe.c
index 2f1301a..2b4c69f 100644
--- a/skyframe.c
+++ b/skyframe.c
@@ -1108,10 +1108,10 @@ static double Angle( AstFrame *this_frame, const double a[],
if( cc[ 0 ] != bb[ 0 ] || cc[ 1 ] != bb[ 1 ] ) {
/* Find the angle from north to the line BA. */
- anga = palSlaDbear( bb[ 0 ], bb[ 1 ], aa[ 0 ], aa[ 1 ] );
+ anga = palDbear( bb[ 0 ], bb[ 1 ], aa[ 0 ], aa[ 1 ] );
/* Find the angle from north to the line BC. */
- angc = palSlaDbear( bb[ 0 ], bb[ 1 ], cc[ 0 ], cc[ 1 ] );
+ angc = palDbear( bb[ 0 ], bb[ 1 ], cc[ 0 ], cc[ 1 ] );
/* Find the difference. */
result = angc - anga;
@@ -1122,7 +1122,7 @@ static double Angle( AstFrame *this_frame, const double a[],
if( perm[ 0 ] != 0 ) result = piby2 - result;
/* Fold the result into the range +/- PI. */
- result = palSlaDrange( result );
+ result = palDrange( result );
}
}
}
@@ -1903,7 +1903,7 @@ static double Distance( AstFrame *this_frame,
p2[ perm[ 1 ] ] = point2[ 1 ];
/* Calculate the great circle distance between the points in radians. */
- result = palSlaDsep( p1[ 0 ], p1[ 1 ], p2[ 0 ], p2[ 1 ] );
+ result = palDsep( p1[ 0 ], p1[ 1 ], p2[ 0 ], p2[ 1 ] );
}
}
@@ -2102,8 +2102,8 @@ static AstPointSet *FrameGrid( AstFrame *this_object, int size, const double *lb
lolon != AST__BAD && hilon != AST__BAD ) {
/* Ensure the longitude bounds are in the range 0-2PI. */
- lolon = palSlaDranrm( lolon );
- hilon = palSlaDranrm( hilon );
+ lolon = palDranrm( lolon );
+ hilon = palDranrm( hilon );
/* If the upper longitude limit is less than the lower limit, add 2.PI */
if( hilon <= lolon &&
@@ -2573,8 +2573,8 @@ static const char *GetAttrib( AstObject *this_object, const char *attrib, int *s
/* Format the Equinox as decimal years. Use a Besselian epoch if it
will be less than 1984.0, otherwise use a Julian epoch. */
- result = astFmtDecimalYr( ( equinox < palSlaEpj2d( 1984.0 ) ) ?
- palSlaEpb( equinox ) : palSlaEpj( equinox ),
+ result = astFmtDecimalYr( ( equinox < palEpj2d( 1984.0 ) ) ?
+ palEpb( equinox ) : palEpj( equinox ),
DBL_DIG );
}
@@ -3100,9 +3100,9 @@ static double GetEpoch( AstFrame *this_frame, int *status ) {
setting. */
system = astGetSystem( this );
if( system == AST__FK4 || system == AST__FK4_NO_E ) {
- result = palSlaEpb2d( 1950.0 );
+ result = palEpb2d( 1950.0 );
} else {
- result = palSlaEpj2d( 2000.0 );
+ result = palEpj2d( 2000.0 );
}
}
@@ -3615,7 +3615,7 @@ static double GetDiurab( AstSkyFrame *this, int *status ) {
value will be reset to AST__BAD if the ObsLat attribute value is
changed. This code is transliterated from SLA_AOPPA. */
if( this->diurab == AST__BAD ) {
- palSlaGeoc( astGetObsLat( this ), astGetObsAlt( this ), &uau, &vau );
+ palGeoc( astGetObsLat( this ), astGetObsAlt( this ), &uau, &vau );
this->diurab = 2*AST__DPI*uau*SOLSID/C;
}
@@ -4386,11 +4386,11 @@ static const char *GetTitle( AstFrame *this_frame, int *status ) {
pos = sprintf( gettitle_buff, "FK4 equatorial %s", word );
if( astTestEquinox( this ) || astGetUseDefs( this ) ) {
pos += sprintf( gettitle_buff + pos, "; mean equinox B%s",
- astFmtDecimalYr( palSlaEpb( equinox ), 9 ) );
+ astFmtDecimalYr( palEpb( equinox ), 9 ) );
}
if( astTestEpoch( this ) || astGetUseDefs( this ) ) {
pos += sprintf( gettitle_buff + pos,
- "; epoch B%s", astFmtDecimalYr( palSlaEpb( epoch ), 9 ) );
+ "; epoch B%s", astFmtDecimalYr( palEpb( epoch ), 9 ) );
}
break;
@@ -4401,11 +4401,11 @@ static const char *GetTitle( AstFrame *this_frame, int *status ) {
pos = sprintf( gettitle_buff, "FK4 equatorial %s; no E-terms", word );
if( astTestEquinox( this ) || astGetUseDefs( this ) ) {
pos += sprintf( gettitle_buff + pos, "; mean equinox B%s",
- astFmtDecimalYr( palSlaEpb( equinox ), 9 ) );
+ astFmtDecimalYr( palEpb( equinox ), 9 ) );
}
if( astTestEpoch( this ) || astGetUseDefs( this ) ) {
pos += sprintf( gettitle_buff + pos,
- "; epoch B%s", astFmtDecimalYr( palSlaEpb( epoch ), 9 ) );
+ "; epoch B%s", astFmtDecimalYr( palEpb( epoch ), 9 ) );
}
break;
@@ -4416,7 +4416,7 @@ static const char *GetTitle( AstFrame *this_frame, int *status ) {
pos = sprintf( gettitle_buff, "FK5 equatorial %s", word );
if( astTestEquinox( this ) || astGetUseDefs( this ) ) {
pos += sprintf( gettitle_buff + pos, "; mean equinox J%s",
- astFmtDecimalYr( palSlaEpj( equinox ), 9 ) );
+ astFmtDecimalYr( palEpj( equinox ), 9 ) );
}
break;
@@ -4448,7 +4448,7 @@ static const char *GetTitle( AstFrame *this_frame, int *status ) {
case AST__GAPPT:
pos = sprintf( gettitle_buff,
"Geocentric apparent equatorial %s; "
- "; epoch J%s", word, astFmtDecimalYr( palSlaEpj( epoch ), 9 ) );
+ "; epoch J%s", word, astFmtDecimalYr( palEpj( epoch ), 9 ) );
break;
/* Ecliptic coordinates. */
@@ -4458,7 +4458,7 @@ static const char *GetTitle( AstFrame *this_frame, int *status ) {
pos = sprintf( gettitle_buff, "Ecliptic %s", word );
if( astTestEquinox( this ) || astGetUseDefs( this ) ) {
pos += sprintf( gettitle_buff + pos, "; mean equinox J%s",
- astFmtDecimalYr( palSlaEpj( equinox ), 9 ) );
+ astFmtDecimalYr( palEpj( equinox ), 9 ) );
}
break;
@@ -4469,7 +4469,7 @@ static const char *GetTitle( AstFrame *this_frame, int *status ) {
pos = sprintf( gettitle_buff, "Helio-ecliptic %s; mean equinox J2000", word );
if( astTestEpoch( this ) || astGetUseDefs( this ) ) {
pos += sprintf( gettitle_buff + pos, "; epoch J%s",
- astFmtDecimalYr( palSlaEpj( epoch ), 9 ) );
+ astFmtDecimalYr( palEpj( epoch ), 9 ) );
}
break;
@@ -4876,9 +4876,9 @@ void astInitSkyFrameVtab_( AstSkyFrameVtab *vtab, const char *name, int *status
/* Initialize constants for converting between hours, degrees and
radians, etc.. */
LOCK_MUTEX2
- palSlaDtf2r( 1, 0, 0.0, &hr2rad, &stat );
- palSlaDaf2r( 1, 0, 0.0, °2rad, &stat );
- palSlaDaf2r( 180, 0, 0.0, &pi, &stat );
+ palDtf2r( 1, 0, 0.0, &hr2rad, &stat );
+ palDaf2r( 1, 0, 0.0, °2rad, &stat );
+ palDaf2r( 180, 0, 0.0, &pi, &stat );
piby2 = 0.5*pi;
UNLOCK_MUTEX2
@@ -5011,32 +5011,32 @@ static void Intersect( AstFrame *this_frame, const double a1[2],
}
/* Convert each (lon,lat) pair into a unit length 3-vector. */
- palSlaDcs2c( aa1[ 0 ], aa1[ 1 ], va1 );
- palSlaDcs2c( aa2[ 0 ], aa2[ 1 ], va2 );
- palSlaDcs2c( bb1[ 0 ], bb1[ 1 ], vb1 );
- palSlaDcs2c( bb2[ 0 ], bb2[ 1 ], vb2 );
+ palDcs2c( aa1[ 0 ], aa1[ 1 ], va1 );
+ palDcs2c( aa2[ 0 ], aa2[ 1 ], va2 );
+ palDcs2c( bb1[ 0 ], bb1[ 1 ], vb1 );
+ palDcs2c( bb2[ 0 ], bb2[ 1 ], vb2 );
/* Find the normal vectors to the two great cicles. */
- palSlaDvxv( va1, va2, na );
- palSlaDvxv( vb1, vb2, nb );
+ palDvxv( va1, va2, na );
+ palDvxv( vb1, vb2, nb );
/* The cross product of the two normal vectors points to one of the
two diametrically opposite intersections. */
- palSlaDvxv( na, nb, vp );
+ palDvxv( na, nb, vp );
/* Normalise the "vp" vector, also obtaining its original modulus. */
- palSlaDvn( vp, vpn, &vmod );
+ palDvn( vp, vpn, &vmod );
if( vmod != 0.0 ) {
/* We want the intersection which is closest to "a1". The dot product
gives the cos(distance) between two positions. So find the dot
product between "a1" and "vpn", and then between "a1" and the point
diametrically opposite "vpn". */
- d1 = palSlaDvdv( vpn, va1 );
+ d1 = palDvdv( vpn, va1 );
vpn[ 0 ] = -vpn[ 0 ];
vpn[ 1 ] = -vpn[ 1 ];
vpn[ 2 ] = -vpn[ 2 ];
- d2 = palSlaDvdv( vpn, va1 );
+ d2 = palDvdv( vpn, va1 );
/* Revert to "vpn" if it is closer to "a1". */
if( d1 > d2 ) {
@@ -5047,8 +5047,8 @@ static void Intersect( AstFrame *this_frame, const double a1[2],
/* Convert the vector back into a (lon,lat) pair, and put the longitude
into the range 0 to 2.pi. */
- palSlaDcc2s( vpn, cc, cc + 1 );
- *cc = palSlaDranrm( *cc );
+ palDcc2s( vpn, cc, cc + 1 );
+ *cc = palDranrm( *cc );
/* Permute the result coordinates to undo the effect of the SkyFrame
axis permutation array. */
@@ -5206,7 +5206,7 @@ static int LineContains( AstFrame *this, AstLineDef *l, int def, double *point,
if ( perm ) {
p1[ perm[ 0 ] ] = point[ 0 ];
p1[ perm[ 1 ] ] = point[ 1 ];
- palSlaDcs2c( p1[ 0 ], p1[ 1 ], bb );
+ palDcs2c( p1[ 0 ], p1[ 1 ], bb );
b = bb;
} else {
b = NULL;
@@ -5224,7 +5224,7 @@ static int LineContains( AstFrame *this, AstLineDef *l, int def, double *point,
/* Check that the point is 90 degrees away from the pole of the great
circle containing the line. */
- t1 = palSlaDvdv( sl->q, b );
+ t1 = palDvdv( sl->q, b );
t2 = 1.0E-7*sl->length;
if( t2 < 1.0E-10 ) t2 = 1.0E-10;
if( fabs( t1 ) <= t2 ) result = 1;
@@ -5346,9 +5346,9 @@ static int LineCrossing( AstFrame *this, AstLineDef *l1, AstLineDef *l2,
/* Point of intersection of the two great circles is perpendicular to the
pole vectors of both great circles. Put the Cartesian coords in elements
2 to 4 of the returned array. */
- palSlaDvxv( sl1->q, sl2->q, temp );
+ palDvxv( sl1->q, sl2->q, temp );
b = crossing + 2;
- palSlaDvn( temp, b, &len );
+ palDvn( temp, b, &len );
/* See if this point is within the length of both arcs. If so return it. */
if( LineIncludes( sl2, b, status ) && LineIncludes( sl1, b, status ) ) {
@@ -5364,7 +5364,7 @@ static int LineCrossing( AstFrame *this, AstLineDef *l1, AstLineDef *l2,
}
/* Store the spherical coords in elements 0 and 1 of the returned array. */
- palSlaDcc2s( b, p, p + 1 );
+ palDcc2s( b, p, p + 1 );
/* Permute the spherical axis value into the order used by the SkyFrame. */
perm = astGetPerm( this );
@@ -5475,12 +5475,12 @@ static AstLineDef *LineDef( AstFrame *this, const double start[2],
/* Convert each point into a 3-vector of unit length and store in the
returned structure. */
- palSlaDcs2c( p1[ 0 ], p1[ 1 ], result->start );
- palSlaDcs2c( p2[ 0 ], p2[ 1 ], result->end );
+ palDcs2c( p1[ 0 ], p1[ 1 ], result->start );
+ palDcs2c( p2[ 0 ], p2[ 1 ], result->end );
/* Calculate the great circle distance between the points in radians and
store in the result structure. */
- result->length = acos( palSlaDvdv( result->start, result->end ) );
+ result->length = acos( palDvdv( result->start, result->end ) );
/* Find a unit vector representing the pole of the system in which the
equator is given by the great circle. This is such that going the
@@ -5489,16 +5489,16 @@ static AstLineDef *LineDef( AstFrame *this, const double start[2],
If the line has zero length, or 180 degrees length, the pole is
undefined, so we use an arbitrary value. */
if( result->length == 0.0 || result->length > pi - 5.0E-11 ) {
- palSlaDcs2c( p1[ 0 ] + 0.01, p1[ 1 ] + 0.01, temp );
- palSlaDvxv( temp, result->start, result->dir );
+ palDcs2c( p1[ 0 ] + 0.01, p1[ 1 ] + 0.01, temp );
+ palDvxv( temp, result->start, result->dir );
} else {
- palSlaDvxv( result->end, result->start, result->dir );
+ palDvxv( result->end, result->start, result->dir );
}
- palSlaDvn( result->dir, result->q, &len );
+ palDvn( result->dir, result->q, &len );
/* Also store a point which is 90 degrees along the great circle from the
start. */
- palSlaDvxv( result->start, result->q, result->dir );
+ palDvxv( result->start, result->q, result->dir );
/* Store a pointer to the defining SkyFrame. */
result->frame = this;
@@ -5582,9 +5582,9 @@ static int LineIncludes( SkyLineDef *l, double point[3], int *status ) {
line in the range 0 - 180 degs. Check it is less than the line length.
Then check that the point is not more than 90 degs away from the quarter
point. */
- t1 = palSlaDvdv( l->start, point );
+ t1 = palDvdv( l->start, point );
t2 = acos( t1 );
- t3 = palSlaDvdv( l->dir, point );
+ t3 = palDvdv( l->dir, point );
return ( ((l->length > 0) ? t2 < l->length : t2 == 0.0 ) && t3 >= -1.0E-8 );
}
@@ -5683,7 +5683,7 @@ static void LineOffset( AstFrame *this, AstLineDef *line, double par,
}
/* Convert to lon/lat */
- palSlaDcc2s( v, p, p + 1 );
+ palDcc2s( v, p, p + 1 );
/* Permute the spherical axis value into the order used by the SkyFrame. */
perm = astGetPerm( this );
@@ -5922,10 +5922,10 @@ static int MakeSkyMapping( AstSkyFrame *target, AstSkyFrame *result,
/* Convert the equinox and epoch values (stored as Modified Julian
Dates) into the equivalent Besselian and Julian epochs (as decimal
years). */
- equinox_B = palSlaEpb( equinox );
- equinox_J = palSlaEpj( equinox );
- epoch_B = palSlaEpb( epoch );
- epoch_J = palSlaEpj( epoch );
+ equinox_B = palEpb( equinox );
+ equinox_J = palEpj( equinox );
+ epoch_B = palEpb( epoch );
+ epoch_J = palEpj( epoch );
/* Formulate the conversion... */
@@ -6160,10 +6160,10 @@ static int MakeSkyMapping( AstSkyFrame *target, AstSkyFrame *result,
Dates) into the equivalent Besselian and Julian epochs (as decimal
years). */
if( astOK ) {
- equinox_B = palSlaEpb( equinox );
- equinox_J = palSlaEpj( equinox );
- epoch_B = palSlaEpb( epoch );
- epoch_J = palSlaEpj( epoch );
+ equinox_B = palEpb( equinox );
+ equinox_J = palEpj( equinox );
+ epoch_B = palEpb( epoch );
+ epoch_J = palEpj( epoch );
}
/* Check we need to do the conversion. */
@@ -6916,8 +6916,8 @@ static void Norm( AstFrame *this_frame, double value[], int *status ) {
/* Fold the longitude value into the range 0 to 2*pi and the latitude into
the range -pi to +pi. */
- sky_long = palSlaDranrm( sky_long );
- sky_lat = palSlaDrange( sky_lat );
+ sky_long = palDranrm( sky_long );
+ sky_lat = palDrange( sky_lat );
/* If the latitude now exceeds pi/2, shift the longitude by pi in whichever
direction will keep it in the range 0 to 2*pi. */
@@ -6940,11 +6940,11 @@ static void Norm( AstFrame *this_frame, double value[], int *status ) {
/* If only the longitude value is valid, wrap it into the range 0 to 2*pi. */
} else if ( sky_long != AST__BAD ) {
- sky_long = palSlaDranrm( sky_long );
+ sky_long = palDranrm( sky_long );
/* If only the latitude value is valid, wrap it into the range -pi to +pi. */
} else if ( sky_lat != AST__BAD ) {
- sky_lat = palSlaDrange( sky_lat );
+ sky_lat = palDrange( sky_lat );
/* Then refect through one of the poles (as above), if necessary, to move it
into the range -pi/2 to +pi/2. */
@@ -6962,7 +6962,7 @@ static void Norm( AstFrame *this_frame, double value[], int *status ) {
/* If the NegLon attribute is set, and the longitude value is good,
convert it into the range -pi to +pi. */
if( sky_long != AST__BAD && astGetNegLon( this ) ) {
- sky_long = palSlaDrange( sky_long );
+ sky_long = palDrange( sky_long );
}
/* Return the new values, allowing for any axis permutation. */
@@ -7072,8 +7072,8 @@ static void NormBox( AstFrame *this_frame, double lbnd[], double ubnd[],
/* Find the lowest latitude after normalisation. */
if( ub[ 1 ] != AST__BAD && lb[ 1 ] != AST__BAD ){
- t = palSlaDrange( ub[ 1 ] );
- t2 = palSlaDrange( lb[ 1 ] );
+ t = palDrange( ub[ 1 ] );
+ t2 = palDrange( lb[ 1 ] );
if( t2 < t ) t = t2;
} else {
t = AST__BAD;
@@ -7095,8 +7095,8 @@ static void NormBox( AstFrame *this_frame, double lbnd[], double ubnd[],
/* Find the highest latitude after normalisation. */
if( ub[ 1 ] != AST__BAD && lb[ 1 ] != AST__BAD ){
- t = palSlaDrange( ub[ 1 ] );
- t2 = palSlaDrange( lb[ 1 ] );
+ t = palDrange( ub[ 1 ] );
+ t2 = palDrange( lb[ 1 ] );
if( t2 > t ) t = t2;
} else {
t = AST__BAD;
@@ -7224,17 +7224,17 @@ static void Offset( AstFrame *this_frame, const double point1[],
p2[ perm[ 1 ] ] = point2[ 1 ];
/* Convert each point into a 3-vector of unit length. */
- palSlaDcs2c( p1[ 0 ], p1[ 1 ], v1 );
- palSlaDcs2c( p2[ 0 ], p2[ 1 ], v2 );
+ palDcs2c( p1[ 0 ], p1[ 1 ], v1 );
+ palDcs2c( p2[ 0 ], p2[ 1 ], v2 );
/* Find the cross product between these two vectors (the vector order
is reversed here to compensate for the sense of rotation introduced
- by palSlaDav2m and palSlaDmxv below). */
- palSlaDvxv( v2, v1, v3 );
+ by palDav2m and palDmxv below). */
+ palDvxv( v2, v1, v3 );
/* Normalise the cross product vector, also obtaining its original
modulus. */
- palSlaDvn( v3, vrot, &vmod );
+ palDvn( v3, vrot, &vmod );
/* If the original modulus was zero, the input points are either
coincident or diametrically opposite, so do not uniquely define a
@@ -7251,9 +7251,9 @@ static void Offset( AstFrame *this_frame, const double point1[],
/* Convert the 3-vector back into spherical cooordinates and then
constrain the longitude result to lie in the range 0 to 2*pi
- (palSlaDcc2s doesn't do this itself). */
- palSlaDcc2s( v3, &p3[ 0 ], &p3[ 1 ] );
- p3[ 0 ] = palSlaDranrm( p3[ 0 ] );
+ (palDcc2s doesn't do this itself). */
+ palDcc2s( v3, &p3[ 0 ], &p3[ 1 ] );
+ p3[ 0 ] = palDranrm( p3[ 0 ] );
/* If the offset was not a multiple of pi, generate "bad" output
coordinates. */
@@ -7273,13 +7273,13 @@ static void Offset( AstFrame *this_frame, const double point1[],
/* Generate the rotation matrix that implements this rotation and use
it to rotate the first input point (3-vector) to give the required
result (3-vector). */
- palSlaDav2m( vrot, mrot );
- palSlaDmxv( mrot, v1, v3 );
+ palDav2m( vrot, mrot );
+ palDmxv( mrot, v1, v3 );
/* Convert the 3-vector back into spherical cooordinates and then
constrain the longitude result to lie in the range 0 to 2*pi. */
- palSlaDcc2s( v3, &p3[ 0 ], &p3[ 1 ] );
- p3[ 0 ] = palSlaDranrm( p3[ 0 ] );
+ palDcc2s( v3, &p3[ 0 ], &p3[ 1 ] );
+ p3[ 0 ] = palDranrm( p3[ 0 ] );
}
/* Permute the result coordinates to undo the effect of the SkyFrame
@@ -7391,16 +7391,16 @@ f function is invoked with STATUS set to an error value, or if it
/* Convert each point into a 3-vector of unit length. The SkyRef position
defines the X axis in the offset coord system. */
- palSlaDcs2c( astGetSkyRef( this, lonaxis ), astGetSkyRef( this, lataxis ), vx );
- palSlaDcs2c( astGetSkyRefP( this, lonaxis ), astGetSkyRefP( this, lataxis ), vp );
+ palDcs2c( astGetSkyRef( this, lonaxis ), astGetSkyRef( this, lataxis ), vx );
+ palDcs2c( astGetSkyRefP( this, lonaxis ), astGetSkyRefP( this, lataxis ), vp );
/* The Y axis is perpendicular to both the X axis and the skyrefp
position. That is, it is parallel to the cross product of the 2 above
vectors.*/
- palSlaDvxv( vp, vx, vy );
+ palDvxv( vp, vx, vy );
/* Normalize the y vector. */
- palSlaDvn( vy, vy, &vmod );
+ palDvn( vy, vy, &vmod );
/* Report an error if the modulus of the vector is zero.*/
if( vmod == 0.0 ) {
@@ -7410,7 +7410,7 @@ f function is invoked with STATUS set to an error value, or if it
/* If OK, form the Z axis as the cross product of the x and y axes. */
} else {
- palSlaDvxv( vx, vy, vz );
+ palDvxv( vx, vy, vz );
}
@@ -7420,16 +7420,16 @@ f function is invoked with STATUS set to an error value, or if it
/* Convert each point into a 3-vector of unit length. The SkyRef position
defines the Z axis in the offset coord system. */
- palSlaDcs2c( astGetSkyRef( this, lonaxis ), astGetSkyRef( this, lataxis ), vz );
- palSlaDcs2c( astGetSkyRefP( this, lonaxis ), astGetSkyRefP( this, lataxis ), vp );
+ palDcs2c( astGetSkyRef( this, lonaxis ), astGetSkyRef( this, lataxis ), vz );
+ palDcs2c( astGetSkyRefP( this, lonaxis ), astGetSkyRefP( this, lataxis ), vp );
/* The Y axis is perpendicular to both the Z axis and the skyrefp
position. That is, it is parallel to the cross product of the 2 above
vectors.*/
- palSlaDvxv( vz, vp, vy );
+ palDvxv( vz, vp, vy );
/* Normalize the y vector. */
- palSlaDvn( vy, vy, &vmod );
+ palDvn( vy, vy, &vmod );
/* Report an error if the modulus of the vector is zero.*/
if( vmod == 0.0 ) {
@@ -7439,7 +7439,7 @@ f function is invoked with STATUS set to an error value, or if it
/* If OK, form the X axis as the cross product of the y and z axes. */
} else {
- palSlaDvxv( vy, vz, vx );
+ palDvxv( vy, vz, vx );
}
}
@@ -7631,13 +7631,13 @@ static double Offset2( AstFrame *this_frame, const double point1[2],
/* Calculate the position angle of the great circle at the required
point. */
- pa = atan2( palSlaDvdv( q3, q2 ), palSlaDvdv( q3, q1 ) );
+ pa = atan2( palDvdv( q3, q2 ), palDvdv( q3, q1 ) );
/* Convert this from a pa into the required angle. */
result = ( perm[ 0 ] == 0 )? pa: piby2 - pa;
/* Ensure that the end angle is in the range 0 to 2*pi. */
- result = palSlaDranrm( result );
+ result = palDranrm( result );
/* Permute the result coordinates to undo the effect of the SkyFrame
axis permutation array. */
@@ -7969,15 +7969,15 @@ static void Resolve( AstFrame *this_frame, const double point1[],
p3[ perm[ 1 ] ] = point3[ 1 ];
/* Convert each point into a 3-vector of unit length. */
- palSlaDcs2c( p1[ 0 ], p1[ 1 ], v1 );
- palSlaDcs2c( p2[ 0 ], p2[ 1 ], v2 );
- palSlaDcs2c( p3[ 0 ], p3[ 1 ], v3 );
+ palDcs2c( p1[ 0 ], p1[ 1 ], v1 );
+ palDcs2c( p2[ 0 ], p2[ 1 ], v2 );
+ palDcs2c( p3[ 0 ], p3[ 1 ], v3 );
/* Find the cross product between the first two vectors, and normalize is.
This is the unit normal to the great circle plane defining parallel
distance. */
- palSlaDvxv( v2, v1, vtemp );
- palSlaDvn( vtemp, n1, &vmod );
+ palDvxv( v2, v1, vtemp );
+ palDvn( vtemp, n1, &vmod );
/* Return with bad values if the normal is undefined (i.e. if the first two
vectors are identical or diametrically opposite). */
@@ -7986,13 +7986,13 @@ static void Resolve( AstFrame *this_frame, const double point1[],
/* Now take the cross product of the normal vector and v1. This gives a
point, v5, on the great circle which is 90 degrees away from v1, in the
direction of v2. */
- palSlaDvxv( v1, n1, v5 );
+ palDvxv( v1, n1, v5 );
/* Find the cross product of the outlying point (point 3), and the vector
n1 found above, and normalize it. This is the unit normal to the great
circle plane defining perpendicular distance. */
- palSlaDvxv( v3, n1, vtemp );
- palSlaDvn( vtemp, n2, &vmod );
+ palDvxv( v3, n1, vtemp );
+ palDvn( vtemp, n2, &vmod );
/* Return with bad values if the normal is undefined (i.e. if the
outlying point is normal to the great circle defining the basis
@@ -8004,24 +8004,24 @@ static void Resolve( AstFrame *this_frame, const double point1[],
This is the cross product of n1 and n2. No need to normalize this time
since both n1 and n2 are unit vectors, and so v4 will already be a
unit vector. */
- palSlaDvxv( n1, n2, v4 );
+ palDvxv( n1, n2, v4 );
/* The dot product of v4 and v1 is the cos of the parallel distance,
d1, whilst the dot product of v4 and v5 is the sin of the parallel
distance. Use these to get the parallel distance with the correct
sign, in the range -PI to +PI. */
- *d1 = atan2( palSlaDvdv( v4, v5 ), palSlaDvdv( v4, v1 ) );
+ *d1 = atan2( palDvdv( v4, v5 ), palDvdv( v4, v1 ) );
/* The dot product of v4 and v3 is the cos of the perpendicular distance,
d2, whilst the dot product of n1 and v3 is the sin of the perpendicular
distance. Use these to get the perpendicular distance. */
- *d2 = fabs( atan2( palSlaDvdv( v3, n1 ), palSlaDvdv( v3, v4 ) ) );
+ *d2 = fabs( atan2( palDvdv( v3, n1 ), palDvdv( v3, v4 ) ) );
/* Convert the 3-vector representing the intersection of the two planes
back into spherical cooordinates and then constrain the longitude result
to lie in the range 0 to 2*pi. */
- palSlaDcc2s( v4, &p4[ 0 ], &p4[ 1 ] );
- p4[ 0 ] = palSlaDranrm( p4[ 0 ] );
+ palDcc2s( v4, &p4[ 0 ], &p4[ 1 ] );
+ p4[ 0 ] = palDranrm( p4[ 0 ] );
/* Permute the result coordinates to undo the effect of the SkyFrame
axis permutation array. */
@@ -8225,13 +8225,13 @@ static AstPointSet *ResolvePoints( AstFrame *this_frame, const double point1[],
p2[ perm[ 1 ] ] = point2[ 1 ];
/* Convert these points into 3-vectors of unit length. */
- palSlaDcs2c( p1[ 0 ], p1[ 1 ], v1 );
- palSlaDcs2c( p2[ 0 ], p2[ 1 ], v2 );
+ palDcs2c( p1[ 0 ], p1[ 1 ], v1 );
+ palDcs2c( p2[ 0 ], p2[ 1 ], v2 );
/* Find the cross product between the vectors, and normalize it. This is the
unit normal to the great circle plane defining parallel distance. */
- palSlaDvxv( v2, v1, vtemp );
- palSlaDvn( vtemp, n1, &vmod );
+ palDvxv( v2, v1, vtemp );
+ palDvn( vtemp, n1, &vmod );
/* Return with bad values if the normal is undefined (i.e. if the first two
vectors are identical or diametrically opposite). */
@@ -8242,7 +8242,7 @@ static AstPointSet *ResolvePoints( AstFrame *this_frame, const double point1[],
/* Now take the cross product of the normal vector and v1. This gives a
point, v5, on the great circle which is 90 degrees away from v1, in the
direction of v2. */
- palSlaDvxv( v1, n1, v5 );
+ palDvxv( v1, n1, v5 );
}
/* Store pointers to the first two axis arrays in the returned PointSet. */
@@ -8274,13 +8274,13 @@ static AstPointSet *ResolvePoints( AstFrame *this_frame, const double point1[],
p3[ perm[ 1 ] ] = *point3y;
/* Convert into a 3-vector of unit length. */
- palSlaDcs2c( p3[ 0 ], p3[ 1 ], v3 );
+ palDcs2c( p3[ 0 ], p3[ 1 ], v3 );
/* Find the cross product of the outlying point (point 3), and the vector
n1 found above, and normalize it. This is the unit normal to the great
circle plane defining perpendicular distance. */
- palSlaDvxv( v3, n1, vtemp );
- palSlaDvn( vtemp, n2, &vmod );
+ palDvxv( v3, n1, vtemp );
+ palDvn( vtemp, n2, &vmod );
/* Return with bad values if the normal is undefined (i.e. if the
outlying point is normal to the great circle defining the basis
@@ -8295,18 +8295,18 @@ static AstPointSet *ResolvePoints( AstFrame *this_frame, const double point1[],
This is the cross product of n1 and n2. No need to normalize this time
since both n1 and n2 are unit vectors, and so v4 will already be a
unit vector. */
- palSlaDvxv( n1, n2, v4 );
+ palDvxv( n1, n2, v4 );
/* The dot product of v4 and v1 is the cos of the parallel distance,
d1, whilst the dot product of v4 and v5 is the sin of the parallel
distance. Use these to get the parallel distance with the correct
sign, in the range -PI to +PI. */
- *d1 = atan2( palSlaDvdv( v4, v5 ), palSlaDvdv( v4, v1 ) );
+ *d1 = atan2( palDvdv( v4, v5 ), palDvdv( v4, v1 ) );
/* The dot product of v4 and v3 is the cos of the perpendicular distance,
d2, whilst the dot product of n1 and v3 is the sin of the perpendicular
distance. Use these to get the perpendicular distance. */
- *d2 = sign*atan2( palSlaDvdv( v3, n1 ), palSlaDvdv( v3, v4 ) );
+ *d2 = sign*atan2( palDvdv( v3, n1 ), palDvdv( v3, v4 ) );
}
}
}
@@ -10822,7 +10822,7 @@ astMAKE_GET(SkyFrame,Equinox,double,AST__BAD,(
( this->equinox != AST__BAD ) ? this->equinox :
( ( ( astGetSystem( this ) == AST__FK4 ) ||
( astGetSystem( this ) == AST__FK4_NO_E ) ) ?
- palSlaEpb2d( 1950.0 ) : palSlaEpj2d( 2000.0 ) ) ))
+ palEpb2d( 1950.0 ) : palEpj2d( 2000.0 ) ) ))
/* Allow any Equinox value to be set, unless the System is Helio-ecliptic
(in which case clear the value so that J2000 is used). */
@@ -11430,8 +11430,8 @@ static void Dump( AstObject *this_object, AstChannel *channel, int *status ) {
( system == AST__ECLIPTIC ) );
/* Convert MJD to Besselian or Julian years, depending on the value. */
- bessyr = ( dval < palSlaEpj2d( 1984.0 ) );
- dval = bessyr ? palSlaEpb( dval ) : palSlaEpj( dval );
+ bessyr = ( dval < palEpj2d( 1984.0 ) );
+ dval = bessyr ? palEpb( dval ) : palEpj( dval );
astWriteDouble( channel, "Eqnox", set, helpful, dval,
bessyr ? "Besselian epoch of mean equinox" :
"Julian epoch of mean equinox" );
@@ -11921,8 +11921,8 @@ AstSkyFrame *astLoadSkyFrame_( void *mem, size_t size,
/* Interpret this as Besselian or Julian depending on its value. */
new->equinox = astReadDouble( channel, "eqnox", AST__BAD );
if ( TestEquinox( new, status ) ) {
- SetEquinox( new, ( new->equinox < 1984.0 ) ? palSlaEpb2d( new->equinox ) :
- palSlaEpj2d( new->equinox ), status );
+ SetEquinox( new, ( new->equinox < 1984.0 ) ? palEpb2d( new->equinox ) :
+ palEpj2d( new->equinox ), status );
}
/* NegLon. */
diff --git a/slamap.c b/slamap.c
index e961cab..ce1288a 100644
--- a/slamap.c
+++ b/slamap.c
@@ -74,7 +74,7 @@ f - AST_SLAADD: Add a celestial coordinate conversion to an SlaMap
* 25-APR-1996 (RFWS):
* Original version.
* 28-MAY-1996 (RFWS):
-* Fixed bug in argument order to palSlaMappa for AST__SLA_AMP case.
+* Fixed bug in argument order to palMappa for AST__SLA_AMP case.
* 26-SEP-1996 (RFWS):
* Added external interface and I/O facilities.
* 23-MAY-1997 (RFWS):
@@ -98,7 +98,7 @@ f - AST_SLAADD: Add a celestial coordinate conversion to an SlaMap
* 14-FEB-2006 (DSB):
* Override astGetObjSize.
* 22-FEB-2006 (DSB):
-* Cache results returned by palSlaMappa in order to increase speed.
+* Cache results returned by palMappa in order to increase speed.
* 10-MAY-2006 (DSB):
* Override astEqual.
* 31-AUG-2007 (DSB):
@@ -186,6 +186,7 @@ f - AST_SLAADD: Add a celestial coordinate conversion to an SlaMap
#include "object.h" /* Base Object class */
#include "pointset.h" /* Sets of points/coordinates */
#include "mapping.h" /* Coordinate Mappings (parent class) */
+#include "wcsmap.h" /* Required for AST__DPI */
#include "unitmap.h" /* Unit (null) Mappings */
#include "slamap.h" /* Interface definition for this class */
@@ -237,7 +238,7 @@ astMAKE_INITGLOBALS(SlaMap)
variables. */
#else
-/* A cache used to store the most recent results from palSlaMappa in order
+/* A cache used to store the most recent results from palMappa in order
to avoid continuously recalculating the same values. */
static double eq_cache = AST__BAD;
static double ep_cache = AST__BAD;
@@ -267,6 +268,8 @@ static int Equal( AstObject *, AstObject *, int * );
static int MapMerge( AstMapping *, int, int, int *, AstMapping ***, int **, int * );
static void AddSlaCvt( AstSlaMap *, int, const double *, int * );
static void Copy( const AstObject *, AstObject *, int * );
+static void De2h( double, double, double, double, double *, double *, int * );
+static void Dh2e( double, double, double, double, double *, double *, int * );
static void Delete( AstObject *, int * );
static void Dump( AstObject *, AstChannel *, int * );
static void Earth( double, double[3], int * );
@@ -282,8 +285,139 @@ static void STPConv( double, int, int, int, double[3], double *[3], int, double[
static void J2000H( int, int, double *, double *, int * );
static int GetObjSize( AstObject *, int * );
+
/* Member functions. */
/* ================= */
+
+static void De2h( double ha, double dec, double phi, double diurab,
+ double *az, double *el, int *status ){
+
+/* Not quite like slaDe2h since it converts from apparent (ha,dec) to
+ topocentric (az,el). This includes a correction for diurnal
+ aberration. The magnitude of the diurnal aberration vector should be
+ supplied in parameter "diurab". The extra code is taken from the
+ Fortran routine SLA_AOPQK. */
+
+/* Local Variables: */
+ double a;
+ double cd;
+ double ch;
+ double cp;
+ double f;
+ double r;
+ double sd;
+ double sh;
+ double sp;
+ double x;
+ double xhd;
+ double xhdt;
+ double y;
+ double yhd;
+ double yhdt;
+ double z;
+ double zhd;
+ double zhdt;
+
+/* Check inherited status */
+ if( !astOK ) return;
+
+/* Pre-compute common values */
+ sh = sin( ha );
+ ch = cos( ha );
+ sd = sin( dec );
+ cd = cos( dec );
+ sp = sin( phi );
+ cp = cos( phi );
+
+/* Components of cartesian (-ha,dec) vector. */
+ xhd = ch*cd;
+ yhd = -sh*cd;
+ zhd = sd;
+
+/* Modify the above vector to apply diurnal aberration. */
+ f = ( 1.0 - diurab*yhd );
+ xhdt = f*xhd;
+ yhdt = f*( yhd + diurab );
+ zhdt = f*zhd;
+
+/* Convert to cartesian (az,el). */
+ x = -xhdt*sp + zhdt*cp;
+ y = yhdt;
+ z = xhdt*cp + zhdt*sp;
+
+/* Convert to spherical (az,el). */
+ r = sqrt( x*x + y*y );
+ if( r == 0.0 ) {
+ a = 0.0;
+ } else {
+ a = atan2( y, x );
+ }
+
+ while( a < 0.0 ) a += 2*AST__DPI;
+
+ *az = a;
+ *el = atan2( z, r );
+}
+
+static void Dh2e( double az, double el, double phi, double diurab, double *ha,
+ double *dec, int *status ){
+
+/* Not quite like slaDh2e since it converts from topocentric (az,el) to
+ apparent (ha,dec). This includes a correction for diurnal aberration.
+ The magnitude of the diurnal aberration vector should be supplied in
+ parameter "diurab". The extra code is taken from the Fortran routine
+ SLA_OAPQK. */
+
+/* Local Variables: */
+ double ca;
+ double ce;
+ double cp;
+ double f;
+ double r;
+ double sa;
+ double se;
+ double sp;
+ double x;
+ double xmhda;
+ double y;
+ double ymhda;
+ double z;
+ double zmhda;
+
+/* Check inherited status */
+ if( !astOK ) return;
+
+/* Pre-compute common values. */
+ sa = sin( az );
+ ca = cos( az );
+ se = sin( el );
+ ce = cos( el );
+ sp = sin( phi );
+ cp = cos( phi );
+
+/* Cartesian (az,el) to Cartesian (ha,dec) - note, +ha, not -ha. */
+ xmhda = -ca*ce*sp + se*cp;
+ ymhda = -sa*ce;
+ zmhda = ca*ce*cp + se*sp;
+
+/* Correct this vector for diurnal aberration. Since the above
+ expressions produce +ha rather than -ha, we do not negate "diurab"
+ before using it. Compare this to SLA_AOPQK. */
+ f = ( 1 - diurab*ymhda );
+ x = f*xmhda;
+ y = f*( ymhda + diurab );
+ z = f*zmhda;
+
+/* Cartesian (ha,dec) to spherical (ha,dec). */
+ r = sqrt( x*x + y*y );
+ if( r == 0.0 ) {
+ *ha = 0.0;
+ } else {
+ *ha = atan2( y, x );
+ }
+ *dec = atan2( z, r );
+}
+
static int Equal( AstObject *this_object, AstObject *that_object, int *status ) {
/*
* Name:
@@ -1130,11 +1264,11 @@ static void Earth( double mjd, double earth[3], int *status ) {
/* Get the position of the earth at the given date in the AST__HAQC coord
system (dph). */
- palSlaEvp( mjd, 2000.0, dvb, dpb, dvh, dph );
+ palEvp( mjd, 2000.0, dvb, dpb, dvh, dph );
/* Now rotate the earths position vector into AST__HAEC coords. */
- palSlaEcmat( palSlaEpj2d( 2000.0 ), ecmat );
- palSlaDmxv( ecmat, dph, earth );
+ palEcmat( palEpj2d( 2000.0 ), ecmat );
+ palDmxv( ecmat, dph, earth );
/* Convert from AU to metres. */
earth[0] *= AST__AU;
@@ -1214,11 +1348,11 @@ static void Hgc( double mjd, double mat[3][3], double offset[3], int *status ) {
/* The HG Y axis is perpendicular to both the polar axis and the
sun-earth line. Obtain a Y vector by taking the cross product of the
two vectors, and then normalize it into a unit vector. */
- palSlaDvxv( zhg, earth, ytemp );
- palSlaDvn( ytemp, yhg, &len );
+ palDvxv( zhg, earth, ytemp );
+ palDvn( ytemp, yhg, &len );
/* The HG X axis is perpendicular to both Z and Y, */
- palSlaDvxv( yhg, zhg, xhg );
+ palDvxv( yhg, zhg, xhg );
/* The HG X, Y and Z unit vectors form the columns of the required matrix.
The origins of the two systems are co-incident, so return the zero offset
@@ -1299,7 +1433,7 @@ static void Gsec( double mjd, double mat[3][3], double offset[3], int *status )
in terms of the AST__HAEC (X,Y,Z) axes. The GSEC X axis starts at the
earth and passes through the centre of the sun. This is just the
normalized opposite of the earth's position vector. */
- palSlaDvn( earth, xgs, &len );
+ palDvn( earth, xgs, &len );
xgs[0] *= -1.0;
xgs[1] *= -1.0;
xgs[2] *= -1.0;
@@ -1313,15 +1447,15 @@ static void Gsec( double mjd, double mat[3][3], double offset[3], int *status )
/* Find the GSEC Y axis by taking the vector product of the X axis and
the ecliptic north pole vector, and then normalize it into a unit
vector. */
- palSlaDvxv( pole, xgs, ytemp );
- palSlaDvn( ytemp, ygs, &len );
+ palDvxv( pole, xgs, ytemp );
+ palDvn( ytemp, ygs, &len );
/* The GSEC Z axis is perpendicular to both X and Y axis, and forms a
right-handed system. The resulting vector will be of unit length
since the x and y vectors are both of unit length, and are
perpendicular to each other. It therefore does not need to be
normalized.*/
- palSlaDvxv( xgs, ygs, zgs );
+ palDvxv( xgs, ygs, zgs );
/* The GSEC X, Y and Z unit vectors form the columns of the required matrix. */
for( i = 0; i < 3; i++ ) {
@@ -1439,7 +1573,7 @@ static void Haqc( double mjd, double mat[3][3], double offset[3], int *status )
if ( !astOK ) return;
/* Return the required matrix. */
- palSlaEcmat( palSlaEpj2d( 2000.0 ), mat );
+ palEcmat( palEpj2d( 2000.0 ), mat );
return;
}
@@ -1518,7 +1652,7 @@ static void Hpcc( double mjd, double obs[3], double mat[3][3], double offset[3],
in terms of the AST__HAEC (X,Y,Z) axes. The HPCC X axis starts at the
observer and passes through the centre of the sun. This is just the
normalized opposite of the supplied observer's position vector. */
- palSlaDvn( obs, xhpc, &len );
+ palDvn( obs, xhpc, &len );
xhpc[0] *= -1.0;
xhpc[1] *= -1.0;
xhpc[2] *= -1.0;
@@ -1530,15 +1664,15 @@ static void Hpcc( double mjd, double obs[3], double mat[3][3], double offset[3],
/* Find the HPC Y axis by taking the vector product of the X axis and
the solar north pole vector, and then normalize it into a unit vector.
Note, HPC (X,Y,Z) axes form a left-handed system! */
- palSlaDvxv( xhpc, pole, ytemp );
- palSlaDvn( ytemp, yhpc, &len );
+ palDvxv( xhpc, pole, ytemp );
+ palDvn( ytemp, yhpc, &len );
/* The HPC Z axis is perpendicular to both X and Y axis, and forms a
left-handed system. The resulting vector will be of unit length
since the x and y vectors are both of unit length, and are
perpendicular to each other. It therefore does not need to be
normalized.*/
- palSlaDvxv( yhpc, xhpc, zhpc );
+ palDvxv( yhpc, xhpc, zhpc );
/* The HPC X, Y and Z unit vectors form the columns of the required matrix. */
for( i = 0; i < 3; i++ ) {
@@ -1625,7 +1759,7 @@ static void Hprc( double mjd, double obs[3], double mat[3][3], double offset[3],
in terms of the AST__HAEC (X,Y,Z) axes. The HPRC Z axis starts at the
observer and passes through the centre of the sun. This is just the
normalized opposite of the supplied observer's position vector. */
- palSlaDvn( obs, zhpr, &len );
+ palDvn( obs, zhpr, &len );
zhpr[0] *= -1.0;
zhpr[1] *= -1.0;
zhpr[2] *= -1.0;
@@ -1637,15 +1771,15 @@ static void Hprc( double mjd, double obs[3], double mat[3][3], double offset[3],
/* Find the HPR Y axis by taking the vector product of the Z axis and
the solar north pole vector, and then normalize it into a unit vector.
Note, HPR (X,Y,Z) axes form a left-handed system! */
- palSlaDvxv( pole, zhpr, ytemp );
- palSlaDvn( ytemp, yhpr, &len );
+ palDvxv( pole, zhpr, ytemp );
+ palDvn( ytemp, yhpr, &len );
/* The HPRC X axis is perpendicular to both Y and Z axis, and forms a
left-handed system. The resulting vector will be of unit length
since the y and z vectors are both of unit length, and are
perpendicular to each other. It therefore does not need to be
normalized.*/
- palSlaDvxv( zhpr, yhpr, xhpr );
+ palDvxv( zhpr, yhpr, xhpr );
/* The HPRC X, Y and Z unit vectors form the columns of the required matrix. */
for( i = 0; i < 3; i++ ) {
@@ -1701,24 +1835,24 @@ static void J2000H( int forward, int npoint, double *alpha, double *delta, int *
if ( !astOK ) return;
/* Get the J2000 to ICRS rotation matrix (supplied by P.T. Wallace) */
- palSlaDeuler( "XYZ", -0.0068192*AS2R, 0.0166172*AS2R, 0.0146000*AS2R,
+ palDeuler( "XYZ", -0.0068192*AS2R, 0.0166172*AS2R, 0.0146000*AS2R,
rmat );
/* Loop round all points. */
for( i = 0; i < npoint; i++ ) {
/* Convert from (alpha,delta) to 3-vector */
- palSlaDcs2c( alpha[ i ], delta[ i ], v1 );
+ palDcs2c( alpha[ i ], delta[ i ], v1 );
/* Rotate the 3-vector */
if( forward ) {
- palSlaDmxv( rmat, v1, v2 );
+ palDmxv( rmat, v1, v2 );
} else {
- palSlaDimxv( rmat, v1, v2 );
+ palDimxv( rmat, v1, v2 );
}
/* Convert from 3-vector to (alpha,delta) */
- palSlaDcc2s( v2, alpha + i, delta + i );
+ palDcc2s( v2, alpha + i, delta + i );
}
}
@@ -2101,7 +2235,7 @@ static void STPConv( double mjd, int ignore_origins, int n, int in_sys,
if( p[ 0 ] != AST__BAD &&
p[ 1 ] != AST__BAD &&
p[ 2 ] != AST__BAD ) {
- palSlaDcs2c( p[ 0 ], p[ 1 ], q );
+ palDcs2c( p[ 0 ], p[ 1 ], q );
*(px++) = q[ 0 ]*p[ 2 ];
*(py++) = q[ 1 ]*p[ 2 ];
*(pz++) = q[ 2 ]*p[ 2 ];
@@ -2216,12 +2350,12 @@ static void STPConv( double mjd, int ignore_origins, int n, int in_sys,
off4[ 1 ] = 0.0;
off4[ 2 ] = 0.0;
} else {
- palSlaDmxv( mat3, off3, off4 );
+ palDmxv( mat3, off3, off4 );
}
/* Concatentate the two matrices to get the matrix which rotates from the
current system to the output cartesian system. */
- palSlaDmxm( mat3, mat1, mat4 );
+ palDmxm( mat3, mat1, mat4 );
/* Use the matrix and offset to convert current positions to output
cartesian positions. */
@@ -2237,7 +2371,7 @@ static void STPConv( double mjd, int ignore_origins, int n, int in_sys,
if( p[ 0 ] != AST__BAD &&
p[ 1 ] != AST__BAD &&
p[ 2 ] != AST__BAD ) {
- palSlaDmxv( mat4, p, q );
+ palDmxv( mat4, p, q );
*(px++) = q[ 0 ] + off4[ 0 ];
*(py++) = q[ 1 ] + off4[ 1 ];
*(pz++) = q[ 2 ] + off4[ 2 ];
@@ -2271,9 +2405,9 @@ static void STPConv( double mjd, int ignore_origins, int n, int in_sys,
if( p[ 0 ] != AST__BAD &&
p[ 1 ] != AST__BAD &&
p[ 2 ] != AST__BAD ) {
- palSlaDvn( p, q, &radius );
- palSlaDcc2s( q, &lng, &lat );
- *(px++) = palSlaDranrm( lng );
+ palDvn( p, q, &radius );
+ palDcc2s( q, &lng, &lat );
+ *(px++) = palDranrm( lng );
*(py++) = lat;
*(pz++) = radius;
} else {
@@ -3294,7 +3428,7 @@ static void SolarPole( double mjd, double pole[3], int *status ) {
J2000. We assume T is in days. The text does not explicitly say so,
but we assume that this longitude value (Omega) is with respect to the
mean equinox of J2000.0. */
- omega = 75.76 + 0.01397*( palSlaEpj(mjd) - 2000.0 );
+ omega = 75.76 + 0.01397*( palEpj(mjd) - 2000.0 );
/* Convert this to the ecliptic longitude of the projection of the sun's
north pole onto the ecliptic, in radians. */
@@ -3475,11 +3609,11 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
in turn, returning the results to the same arrays. */
case AST__SLA_ADDET:
if ( forward ) {
- TRAN_ARRAY(palSlaAddet( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palAddet( alpha[ point ], delta[ point ],
args[ 0 ],
alpha + point, delta + point );)
} else {
- TRAN_ARRAY(palSlaSubet( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palSubet( alpha[ point ], delta[ point ],
args[ 0 ],
alpha + point, delta + point );)
}
@@ -3491,11 +3625,11 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
transposed. */
case AST__SLA_SUBET:
if ( forward ) {
- TRAN_ARRAY(palSlaSubet( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palSubet( alpha[ point ], delta[ point ],
args[ 0 ],
alpha + point, delta + point );)
} else {
- TRAN_ARRAY(palSlaAddet( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palAddet( alpha[ point ], delta[ point ],
args[ 0 ],
alpha + point, delta + point );)
}
@@ -3513,16 +3647,16 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
double precess_matrix[ 3 ][ 3 ];
double vec1[ 3 ];
double vec2[ 3 ];
- palSlaPrebn( epoch1, epoch2, precess_matrix );
+ palPrebn( epoch1, epoch2, precess_matrix );
/* For each point in the (alpha,delta) arrays, convert to Cartesian
coordinates, apply the precession matrix, convert back to polar coordinates
and then constrain the longitude result to lie in the range 0 to 2*pi
- (palSlaDcc2s doesn't do this itself). */
- TRAN_ARRAY(palSlaDcs2c( alpha[ point ], delta[ point ], vec1 );
- palSlaDmxv( precess_matrix, vec1, vec2 );
- palSlaDcc2s( vec2, alpha + point, delta + point );
- alpha[ point ] = palSlaDranrm( alpha[ point ] );)
+ (palDcc2s doesn't do this itself). */
+ TRAN_ARRAY(palDcs2c( alpha[ point ], delta[ point ], vec1 );
+ palDmxv( precess_matrix, vec1, vec2 );
+ palDcc2s( vec2, alpha + point, delta + point );
+ alpha[ point ] = palDranrm( alpha[ point ] );)
}
break;
@@ -3537,11 +3671,11 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
double precess_matrix[ 3 ][ 3 ];
double vec1[ 3 ];
double vec2[ 3 ];
- palSlaPrec( epoch1, epoch2, precess_matrix );
- TRAN_ARRAY(palSlaDcs2c( alpha[ point ], delta[ point ], vec1 );
- palSlaDmxv( precess_matrix, vec1, vec2 );
- palSlaDcc2s( vec2, alpha + point, delta + point );
- alpha[ point ] = palSlaDranrm( alpha[ point ] );)
+ palPrec( epoch1, epoch2, precess_matrix );
+ TRAN_ARRAY(palDcs2c( alpha[ point ], delta[ point ], vec1 );
+ palDmxv( precess_matrix, vec1, vec2 );
+ palDcc2s( vec2, alpha + point, delta + point );
+ alpha[ point ] = palDranrm( alpha[ point ] );)
}
break;
@@ -3550,7 +3684,7 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
/* Apply the conversion to each point. */
case AST__SLA_FK45Z:
if ( forward ) {
- TRAN_ARRAY(palSlaFk45z( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palFk45z( alpha[ point ], delta[ point ],
args[ 0 ],
alpha + point, delta + point );)
@@ -3559,7 +3693,7 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
} else {
double dr1950;
double dd1950;
- TRAN_ARRAY(palSlaFk54z( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palFk54z( alpha[ point ], delta[ point ],
args[ 0 ],
alpha + point, delta + point,
&dr1950, &dd1950 );)
@@ -3574,12 +3708,12 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
if ( forward ) {
double dr1950;
double dd1950;
- TRAN_ARRAY(palSlaFk54z( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palFk54z( alpha[ point ], delta[ point ],
args[ 0 ],
alpha + point, delta + point,
&dr1950, &dd1950 );)
} else {
- TRAN_ARRAY(palSlaFk45z( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palFk45z( alpha[ point ], delta[ point ],
args[ 0 ],
alpha + point, delta + point );)
}
@@ -3598,7 +3732,7 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
args[ 0 ] != ep_cache ) {
eq_cache = args[ 1 ];
ep_cache = args[ 0 ];
- palSlaMappa( eq_cache, ep_cache, amprms_cache );
+ palMappa( eq_cache, ep_cache, amprms_cache );
}
extra = astStore( NULL, amprms_cache,
@@ -3607,14 +3741,14 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
}
if ( forward ) {
- TRAN_ARRAY(palSlaAmpqk( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palAmpqk( alpha[ point ], delta[ point ],
extra,
alpha + point, delta + point );)
/* The inverse uses the same parameter array but converts from mean place
to geocentric apparent. */
} else {
- TRAN_ARRAY(palSlaMapqkz( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palMapqkz( alpha[ point ], delta[ point ],
extra,
alpha + point, delta + point );)
}
@@ -3633,7 +3767,7 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
args[ 1 ] != ep_cache ) {
eq_cache = args[ 0 ];
ep_cache = args[ 1 ];
- palSlaMappa( eq_cache, ep_cache, amprms_cache );
+ palMappa( eq_cache, ep_cache, amprms_cache );
}
extra = astStore( NULL, amprms_cache,
@@ -3642,11 +3776,11 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
}
if ( forward ) {
- TRAN_ARRAY(palSlaMapqkz( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palMapqkz( alpha[ point ], delta[ point ],
extra,
alpha + point, delta + point );)
} else {
- TRAN_ARRAY(palSlaAmpqk( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palAmpqk( alpha[ point ], delta[ point ],
extra,
alpha + point, delta + point );)
}
@@ -3668,33 +3802,33 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
/* Obtain the matrix that precesses equatorial coordinates from J2000.0 to the
required date. Also obtain the rotation matrix that converts from
equatorial to ecliptic coordinates. */
- palSlaPrec( 2000.0, palSlaEpj( args[ 0 ] ), precess_matrix );
- palSlaEcmat( args[ 0 ], rotate_matrix );
+ palPrec( 2000.0, palEpj( args[ 0 ] ), precess_matrix );
+ palEcmat( args[ 0 ], rotate_matrix );
/* Multiply these matrices to give the overall matrix that converts from
equatorial J2000.0 coordinates to ecliptic coordinates for the required
date. */
- palSlaDmxm( rotate_matrix, precess_matrix, convert_matrix );
+ palDmxm( rotate_matrix, precess_matrix, convert_matrix );
/* Apply the conversion by transforming from polar to Cartesian coordinates,
multiplying by the inverse conversion matrix and converting back to polar
coordinates. Then constrain the longitude result to lie in the range
- 0 to 2*pi (palSlaDcc2s doesn't do this itself). */
+ 0 to 2*pi (palDcc2s doesn't do this itself). */
if ( forward ) {
- TRAN_ARRAY(palSlaDcs2c( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palDcs2c( alpha[ point ], delta[ point ],
vec1 );
- palSlaDimxv( convert_matrix, vec1, vec2 );
- palSlaDcc2s( vec2, alpha + point, delta + point );
- alpha[ point ] = palSlaDranrm ( alpha[ point ] );)
+ palDimxv( convert_matrix, vec1, vec2 );
+ palDcc2s( vec2, alpha + point, delta + point );
+ alpha[ point ] = palDranrm ( alpha[ point ] );)
/* The inverse conversion is the same except that we multiply by the forward
- conversion matrix (palSlaDmxv instead of palSlaDimxv). */
+ conversion matrix (palDmxv instead of palDimxv). */
} else {
- TRAN_ARRAY(palSlaDcs2c( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palDcs2c( alpha[ point ], delta[ point ],
vec1 );
- palSlaDmxv( convert_matrix, vec1, vec2 );
- palSlaDcc2s( vec2, alpha + point, delta + point );
- alpha[ point ] = palSlaDranrm ( alpha[ point ] );)
+ palDmxv( convert_matrix, vec1, vec2 );
+ palDcc2s( vec2, alpha + point, delta + point );
+ alpha[ point ] = palDranrm ( alpha[ point ] );)
}
}
break;
@@ -3712,23 +3846,23 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
double vec2[ 3 ];
/* Create the conversion matrix. */
- palSlaPrec( 2000.0, palSlaEpj( args[ 0 ] ), precess_matrix );
- palSlaEcmat( args[ 0 ], rotate_matrix );
- palSlaDmxm( rotate_matrix, precess_matrix, convert_matrix );
+ palPrec( 2000.0, palEpj( args[ 0 ] ), precess_matrix );
+ palEcmat( args[ 0 ], rotate_matrix );
+ palDmxm( rotate_matrix, precess_matrix, convert_matrix );
/* Apply it. */
if ( forward ) {
- TRAN_ARRAY(palSlaDcs2c( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palDcs2c( alpha[ point ], delta[ point ],
vec1 );
- palSlaDmxv( convert_matrix, vec1, vec2 );
- palSlaDcc2s( vec2, alpha + point, delta + point );
- alpha[ point ] = palSlaDranrm ( alpha[ point ] );)
+ palDmxv( convert_matrix, vec1, vec2 );
+ palDcc2s( vec2, alpha + point, delta + point );
+ alpha[ point ] = palDranrm ( alpha[ point ] );)
} else {
- TRAN_ARRAY(palSlaDcs2c( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palDcs2c( alpha[ point ], delta[ point ],
vec1 );
- palSlaDimxv( convert_matrix, vec1, vec2 );
- palSlaDcc2s( vec2, alpha + point, delta + point );
- alpha[ point ] = palSlaDranrm ( alpha[ point ] );)
+ palDimxv( convert_matrix, vec1, vec2 );
+ palDcc2s( vec2, alpha + point, delta + point );
+ alpha[ point ] = palDranrm ( alpha[ point ] );)
}
}
break;
@@ -3740,14 +3874,14 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
if ( forward ) {
double dr5;
double dd5;
- TRAN_ARRAY(palSlaHfk5z( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palHfk5z( alpha[ point ], delta[ point ],
args[ 0 ],
alpha + point, delta + point,
&dr5, &dd5 );)
/* The inverse simply uses the inverse SLALIB function. */
} else {
- TRAN_ARRAY(palSlaFk5hz( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palFk5hz( alpha[ point ], delta[ point ],
args[ 0 ],
alpha + point, delta + point );)
}
@@ -3759,7 +3893,7 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
transposed. */
case AST__SLA_FK5HZ:
if ( forward ) {
- TRAN_ARRAY(palSlaFk5hz( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palFk5hz( alpha[ point ], delta[ point ],
args[ 0 ],
alpha + point, delta + point );)
@@ -3767,7 +3901,7 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
} else {
double dr5;
double dd5;
- TRAN_ARRAY(palSlaHfk5z( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palHfk5z( alpha[ point ], delta[ point ],
args[ 0 ],
alpha + point, delta + point,
&dr5, &dd5 );)
@@ -3779,15 +3913,15 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
/* Apply the conversion to each point. */
case AST__SLA_DH2E:
if ( forward ) {
- TRAN_ARRAY(palSlaDh2e( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(Dh2e( alpha[ point ], delta[ point ],
args[ 0 ], args[ 1 ],
- alpha + point, delta + point );)
+ alpha + point, delta + point, status );)
/* The inverse simply uses the inverse SLALIB function. */
} else {
- TRAN_ARRAY(palSlaDe2h( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(De2h( alpha[ point ], delta[ point ],
args[ 0 ], args[ 1 ],
- alpha + point, delta + point );)
+ alpha + point, delta + point, status );)
}
break;
@@ -3797,15 +3931,15 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
transposed. */
case AST__SLA_DE2H:
if ( forward ) {
- TRAN_ARRAY(palSlaDe2h( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(De2h( alpha[ point ], delta[ point ],
args[ 0 ], args[ 1 ],
- alpha + point, delta + point );)
+ alpha + point, delta + point, status );)
/* The inverse simply uses the inverse SLALIB function. */
} else {
- TRAN_ARRAY(palSlaDh2e( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(Dh2e( alpha[ point ], delta[ point ],
args[ 0 ], args[ 1 ],
- alpha + point, delta + point );)
+ alpha + point, delta + point, status );)
}
break;
@@ -3814,12 +3948,12 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
/* Apply the conversion to each point. */
case AST__SLA_GALEQ:
if ( forward ) {
- TRAN_ARRAY(palSlaGaleq( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palGaleq( alpha[ point ], delta[ point ],
alpha + point, delta + point );)
/* The inverse simply uses the inverse SLALIB function. */
} else {
- TRAN_ARRAY(palSlaEqgal( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palEqgal( alpha[ point ], delta[ point ],
alpha + point, delta + point );)
}
break;
@@ -3830,10 +3964,10 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
transposed. */
case AST__SLA_EQGAL:
if ( forward ) {
- TRAN_ARRAY(palSlaEqgal( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palEqgal( alpha[ point ], delta[ point ],
alpha + point, delta + point );)
} else {
- TRAN_ARRAY(palSlaGaleq( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palGaleq( alpha[ point ], delta[ point ],
alpha + point, delta + point );)
}
break;
@@ -3843,12 +3977,12 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
/* Apply the conversion to each point. */
case AST__SLA_GALSUP:
if ( forward ) {
- TRAN_ARRAY(palSlaGalsup( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palGalsup( alpha[ point ], delta[ point ],
alpha + point, delta + point );)
/* The inverse simply uses the inverse SLALIB function. */
} else {
- TRAN_ARRAY(palSlaSupgal( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palSupgal( alpha[ point ], delta[ point ],
alpha + point, delta + point );)
}
break;
@@ -3859,10 +3993,10 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
transposed. */
case AST__SLA_SUPGAL:
if ( forward ) {
- TRAN_ARRAY(palSlaSupgal( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palSupgal( alpha[ point ], delta[ point ],
alpha + point, delta + point );)
} else {
- TRAN_ARRAY(palSlaGalsup( alpha[ point ], delta[ point ],
+ TRAN_ARRAY(palGalsup( alpha[ point ], delta[ point ],
alpha + point, delta + point );)
}
break;
diff --git a/sofa.h b/sofa.h
new file mode 100644
index 0000000..00737b6
--- /dev/null
+++ b/sofa.h
@@ -0,0 +1,72 @@
+#if !defined( SOFA_INCLUDED ) /* Include this file only once */
+#define SOFA_INCLUDED
+/*
+*+
+* Name:
+* sofa.h
+
+* Purpose:
+* Function prototypes for SOFA routines.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Include file
+
+* Description:
+* Function prototypes for SOFA routines. Note, the
+* --with-external_pal configuration option implies that an external
+* SOFA library will also be used.
+
+* Authors:
+* DSBJ: David S Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 23-FEB-2012 (DSB):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+/* Include configuration results in order to get any definition for the
+ EXTERNAL_PAL macro. This macro is set if the --with-external_pal
+ option was set when AST was configured. */
+#if HAVE_CONFIG_H
+#include <config.h>
+#endif
+
+/* If we not using an external SOFA library, rename all SOFA functions so
+ that references to "iauXxx" below get translated to "astIauXxx". */
+#ifndef EXTERNAL_PAL
+#include "sofa2ast.h"
+#endif
+
+/* Include the prototypes defined in the sofa header file. */
+#include "sofa/sofa.h"
+
+#endif
diff --git a/sofa/00READ.ME b/sofa/00READ.ME
new file mode 100644
index 0000000..c298d95
--- /dev/null
+++ b/sofa/00READ.ME
@@ -0,0 +1,49 @@
+
+SOFA-Issue: 2012-03-01
+
+This is the IAU Standards of Fundamental Astronomy (SOFA) Libraries product,
+issued on 2012-03-01. The tag `SOFA-Issue' above defines this release and
+differentiates it from previous or subsequent releases of the SOFA product.
+The 00READ.ME file must remain with this distribution set.
+
+Changes made since the previous release are noted in the file changes.lis.
+
+Notes:
+
+1/ Unix users: The distribution set contains a simple makefile which
+ can be used to create a single object library for the SOFA Libraries.
+ To build the object library:
+
+ a/ Examine the makefile to be sure definition of the C compiler
+ is correct for your system. You need an ANSI standard compliant
+ C compiler. Edit the CCOMPC macro in the makefile as necessary.
+
+ b/ To create libsofa.a, execute make:
+
+ % make
+
+ (where % is the shell prompt).
+
+ c/ To remove the object files:
+
+ % make clean
+
+ To link with the SOFA library, include the library in the compile/link
+ command in the normal Unix fashion, eg:
+
+ % gcc myprog.c -o myprog libsofa.a
+
+ You should specify the appropriate C compiler name for `gcc'
+ in the above command sequence.
+
+
+2/ Windows/DOS/Mac users: There is no `build' procedure to create a linkable
+ object library or DLL for the SOFA Libraries. This is due to the many
+ different C compilers and development environments available on
+ Windows/DOS and Mac machines.
+
+ To use the SOFA routines with your program(s), you must use your preferred
+ development environment to create the appropriate library or DLL.
+
+IAU SOFA Center
+2012/02/29
diff --git a/sofa/a2af.c b/sofa/a2af.c
new file mode 100644
index 0000000..a6ddfb9
--- /dev/null
+++ b/sofa/a2af.c
@@ -0,0 +1,170 @@
+#include "sofam.h"
+
+void iauA2af(int ndp, double angle, char *sign, int idmsf[4])
+/*
+** - - - - - - - -
+** i a u A 2 a f
+** - - - - - - - -
+**
+** Decompose radians into degrees, arcminutes, arcseconds, fraction.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** ndp int resolution (Note 1)
+** angle double angle in radians
+**
+** Returned:
+** sign char '+' or '-'
+** idmsf int[4] degrees, arcminutes, arcseconds, fraction
+**
+** Called:
+** iauD2tf decompose days to hms
+**
+** Notes:
+**
+** 1) The argument ndp is interpreted as follows:
+**
+** ndp resolution
+** : ...0000 00 00
+** -7 1000 00 00
+** -6 100 00 00
+** -5 10 00 00
+** -4 1 00 00
+** -3 0 10 00
+** -2 0 01 00
+** -1 0 00 10
+** 0 0 00 01
+** 1 0 00 00.1
+** 2 0 00 00.01
+** 3 0 00 00.001
+** : 0 00 00.000...
+**
+** 2) The largest positive useful value for ndp is determined by the
+** size of angle, the format of doubles on the target platform, and
+** the risk of overflowing idmsf[3]. On a typical platform, for
+** angle up to 2pi, the available floating-point precision might
+** correspond to ndp=12. However, the practical limit is typically
+** ndp=9, set by the capacity of a 32-bit int, or ndp=4 if int is
+** only 16 bits.
+**
+** 3) The absolute value of angle may exceed 2pi. In cases where it
+** does not, it is up to the caller to test for and handle the
+** case where angle is very nearly 2pi and rounds up to 360 degrees,
+** by testing for idmsf[0]=360 and setting idmsf[0-3] to zero.
+**
+** This revision: 2008 May 27
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Hours to degrees * radians to turns */
+ const double F = 15.0 / D2PI;
+
+
+/* Scale then use days to h,m,s function. */
+ iauD2tf(ndp, angle*F, sign, idmsf);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/a2tf.c b/sofa/a2tf.c
new file mode 100644
index 0000000..ec068c6
--- /dev/null
+++ b/sofa/a2tf.c
@@ -0,0 +1,166 @@
+#include "sofam.h"
+
+void iauA2tf(int ndp, double angle, char *sign, int ihmsf[4])
+/*
+** - - - - - - - -
+** i a u A 2 t f
+** - - - - - - - -
+**
+** Decompose radians into hours, minutes, seconds, fraction.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** ndp int resolution (Note 1)
+** angle double angle in radians
+**
+** Returned:
+** sign char '+' or '-'
+** ihmsf int[4] hours, minutes, seconds, fraction
+**
+** Called:
+** iauD2tf decompose days to hms
+**
+** Notes:
+**
+** 1) The argument ndp is interpreted as follows:
+**
+** ndp resolution
+** : ...0000 00 00
+** -7 1000 00 00
+** -6 100 00 00
+** -5 10 00 00
+** -4 1 00 00
+** -3 0 10 00
+** -2 0 01 00
+** -1 0 00 10
+** 0 0 00 01
+** 1 0 00 00.1
+** 2 0 00 00.01
+** 3 0 00 00.001
+** : 0 00 00.000...
+**
+** 2) The largest positive useful value for ndp is determined by the
+** size of angle, the format of doubles on the target platform, and
+** the risk of overflowing ihmsf[3]. On a typical platform, for
+** angle up to 2pi, the available floating-point precision might
+** correspond to ndp=12. However, the practical limit is typically
+** ndp=9, set by the capacity of a 32-bit int, or ndp=4 if int is
+** only 16 bits.
+**
+** 3) The absolute value of angle may exceed 2pi. In cases where it
+** does not, it is up to the caller to test for and handle the
+** case where angle is very nearly 2pi and rounds up to 24 hours,
+** by testing for ihmsf[0]=24 and setting ihmsf(0-3) to zero.
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Scale then use days to h,m,s function. */
+ iauD2tf(ndp, angle/D2PI, sign, ihmsf);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/af2a.c b/sofa/af2a.c
new file mode 100644
index 0000000..e4353de
--- /dev/null
+++ b/sofa/af2a.c
@@ -0,0 +1,157 @@
+#include "sofam.h"
+#include <stdlib.h>
+
+int iauAf2a(char s, int ideg, int iamin, double asec, double *rad)
+/*
+** - - - - - - - -
+** i a u A f 2 a
+** - - - - - - - -
+**
+** Convert degrees, arcminutes, arcseconds to radians.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** s char sign: '-' = negative, otherwise positive
+** ideg int degrees
+** iamin int arcminutes
+** asec double arcseconds
+**
+** Returned:
+** rad double angle in radians
+**
+** Returned (function value):
+** int status: 0 = OK
+** 1 = ideg outside range 0-359
+** 2 = iamin outside range 0-59
+** 3 = asec outside range 0-59.999...
+**
+** Notes:
+**
+** 1) The result is computed even if any of the range checks fail.
+**
+** 2) Negative ideg, iamin and/or asec produce a warning status, but
+** the absolute value is used in the conversion.
+**
+** 3) If there are multiple errors, the status value reflects only the
+** first, the smallest taking precedence.
+**
+** This revision: 2012 February 13
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+
+/* Compute the interval. */
+ *rad = ( s == '-' ? -1.0 : 1.0 ) *
+ ( 60.0 * ( 60.0 * ( (double) abs(ideg) ) +
+ ( (double) abs(iamin) ) ) +
+ fabs(asec) ) * DAS2R;
+
+/* Validate arguments and return status. */
+ if ( ideg < 0 || ideg > 359 ) return 1;
+ if ( iamin < 0 || iamin > 59 ) return 2;
+ if ( asec < 0.0 || asec >= 60.0 ) return 3;
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/anp.c b/sofa/anp.c
new file mode 100644
index 0000000..66c7d44
--- /dev/null
+++ b/sofa/anp.c
@@ -0,0 +1,132 @@
+#include "sofam.h"
+
+double iauAnp(double a)
+/*
+** - - - - - - -
+** i a u A n p
+** - - - - - - -
+**
+** Normalize angle into the range 0 <= a < 2pi.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double angle (radians)
+**
+** Returned (function value):
+** double angle in range 0-2pi
+**
+** This revision: 2008 May 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double w;
+
+
+ w = fmod(a, D2PI);
+ if (w < 0) w += D2PI;
+
+ return w;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/anpm.c b/sofa/anpm.c
new file mode 100644
index 0000000..5fbe119
--- /dev/null
+++ b/sofa/anpm.c
@@ -0,0 +1,132 @@
+#include "sofam.h"
+
+double iauAnpm(double a)
+/*
+** - - - - - - - -
+** i a u A n p m
+** - - - - - - - -
+**
+** Normalize angle into the range -pi <= a < +pi.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double angle (radians)
+**
+** Returned (function value):
+** double angle in range +/-pi
+**
+** This revision: 2008 May 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double w;
+
+
+ w = fmod(a, D2PI);
+ if (fabs(w) >= DPI) w -= dsign(D2PI, a);
+
+ return w;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/bi00.c b/sofa/bi00.c
new file mode 100644
index 0000000..fff915e
--- /dev/null
+++ b/sofa/bi00.c
@@ -0,0 +1,166 @@
+#include "sofam.h"
+
+void iauBi00(double *dpsibi, double *depsbi, double *dra)
+/*
+** - - - - - - - -
+** i a u B i 0 0
+** - - - - - - - -
+**
+** Frame bias components of IAU 2000 precession-nutation models (part
+** of MHB2000 with additions).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Returned:
+** dpsibi,depsbi double longitude and obliquity corrections
+** dra double the ICRS RA of the J2000.0 mean equinox
+**
+** Notes:
+**
+** 1) The frame bias corrections in longitude and obliquity (radians)
+** are required in order to correct for the offset between the GCRS
+** pole and the mean J2000.0 pole. They define, with respect to the
+** GCRS frame, a J2000.0 mean pole that is consistent with the rest
+** of the IAU 2000A precession-nutation model.
+**
+** 2) In addition to the displacement of the pole, the complete
+** description of the frame bias requires also an offset in right
+** ascension. This is not part of the IAU 2000A model, and is from
+** Chapront et al. (2002). It is returned in radians.
+**
+** 3) This is a supplemented implementation of one aspect of the IAU
+** 2000A nutation model, formally adopted by the IAU General
+** Assembly in 2000, namely MHB2000 (Mathews et al. 2002).
+**
+** References:
+**
+** Chapront, J., Chapront-Touze, M. & Francou, G., Astron.
+** Astrophys., 387, 700, 2002.
+**
+** Mathews, P.M., Herring, T.A., Buffet, B.A., "Modeling of nutation
+** and precession New nutation series for nonrigid Earth and
+** insights into the Earth's interior", J.Geophys.Res., 107, B4,
+** 2002. The MHB2000 code itself was obtained on 9th September 2002
+** from ftp://maia.usno.navy.mil/conv2000/chapter5/IAU2000A.
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* The frame bias corrections in longitude and obliquity */
+ const double DPBIAS = -0.041775 * DAS2R,
+ DEBIAS = -0.0068192 * DAS2R;
+
+/* The ICRS RA of the J2000.0 equinox (Chapront et al., 2002) */
+ const double DRA0 = -0.0146 * DAS2R;
+
+
+/* Return the results (which are fixed). */
+ *dpsibi = DPBIAS;
+ *depsbi = DEBIAS;
+ *dra = DRA0;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/bp00.c b/sofa/bp00.c
new file mode 100644
index 0000000..0f506c2
--- /dev/null
+++ b/sofa/bp00.c
@@ -0,0 +1,223 @@
+#include "sofam.h"
+
+void iauBp00(double date1, double date2,
+ double rb[3][3], double rp[3][3], double rbp[3][3])
+/*
+** - - - - - - - -
+** i a u B p 0 0
+** - - - - - - - -
+**
+** Frame bias and precession, IAU 2000.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rb double[3][3] frame bias matrix (Note 2)
+** rp double[3][3] precession matrix (Note 3)
+** rbp double[3][3] bias-precession matrix (Note 4)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix rb transforms vectors from GCRS to mean J2000.0 by
+** applying frame bias.
+**
+** 3) The matrix rp transforms vectors from J2000.0 mean equator and
+** equinox to mean equator and equinox of date by applying
+** precession.
+**
+** 4) The matrix rbp transforms vectors from GCRS to mean equator and
+** equinox of date by applying frame bias then precession. It is
+** the product rp x rb.
+**
+** 5) It is permissible to re-use the same array in the returned
+** arguments. The arrays are filled in the order given.
+**
+** Called:
+** iauBi00 frame bias components, IAU 2000
+** iauPr00 IAU 2000 precession adjustments
+** iauIr initialize r-matrix to identity
+** iauRx rotate around X-axis
+** iauRy rotate around Y-axis
+** iauRz rotate around Z-axis
+** iauCr copy r-matrix
+** iauRxr product of two r-matrices
+**
+** Reference:
+** "Expressions for the Celestial Intermediate Pole and Celestial
+** Ephemeris Origin consistent with the IAU 2000A precession-
+** nutation model", Astron.Astrophys. 400, 1145-1154 (2003)
+**
+** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
+** intermediate origin" (CIO) by IAU 2006 Resolution 2.
+**
+** This revision: 2010 January 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* J2000.0 obliquity (Lieske et al. 1977) */
+ const double EPS0 = 84381.448 * DAS2R;
+
+ double t, dpsibi, depsbi;
+ double dra0, psia77, oma77, chia, dpsipr, depspr, psia, oma,
+ rbw[3][3];
+
+
+/* Interval between fundamental epoch J2000.0 and current date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* Frame bias. */
+ iauBi00(&dpsibi, &depsbi, &dra0);
+
+/* Precession angles (Lieske et al. 1977) */
+ psia77 = (5038.7784 + (-1.07259 + (-0.001147) * t) * t) * t * DAS2R;
+ oma77 = EPS0 + ((0.05127 + (-0.007726) * t) * t) * t * DAS2R;
+ chia = ( 10.5526 + (-2.38064 + (-0.001125) * t) * t) * t * DAS2R;
+
+/* Apply IAU 2000 precession corrections. */
+ iauPr00(date1, date2, &dpsipr, &depspr);
+ psia = psia77 + dpsipr;
+ oma = oma77 + depspr;
+
+/* Frame bias matrix: GCRS to J2000.0. */
+ iauIr(rbw);
+ iauRz(dra0, rbw);
+ iauRy(dpsibi * sin(EPS0), rbw);
+ iauRx(-depsbi, rbw);
+ iauCr(rbw, rb);
+
+/* Precession matrix: J2000.0 to mean of date. */
+ iauIr(rp);
+ iauRx(EPS0, rp);
+ iauRz(-psia, rp);
+ iauRx(-oma, rp);
+ iauRz(chia, rp);
+
+/* Bias-precession matrix: GCRS to mean of date. */
+ iauRxr(rp, rbw, rbp);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/bp06.c b/sofa/bp06.c
new file mode 100644
index 0000000..04bbb59
--- /dev/null
+++ b/sofa/bp06.c
@@ -0,0 +1,186 @@
+#include "sofam.h"
+
+void iauBp06(double date1, double date2,
+ double rb[3][3], double rp[3][3], double rbp[3][3])
+/*
+** - - - - - - - -
+** i a u B p 0 6
+** - - - - - - - -
+**
+** Frame bias and precession, IAU 2006.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rb double[3][3] frame bias matrix (Note 2)
+** rp double[3][3] precession matrix (Note 3)
+** rbp double[3][3] bias-precession matrix (Note 4)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix rb transforms vectors from GCRS to mean J2000.0 by
+** applying frame bias.
+**
+** 3) The matrix rp transforms vectors from mean J2000.0 to mean of
+** date by applying precession.
+**
+** 4) The matrix rbp transforms vectors from GCRS to mean of date by
+** applying frame bias then precession. It is the product rp x rb.
+**
+** Called:
+** iauPfw06 bias-precession F-W angles, IAU 2006
+** iauFw2m F-W angles to r-matrix
+** iauPmat06 PB matrix, IAU 2006
+** iauTr transpose r-matrix
+** iauRxr product of two r-matrices
+**
+** References:
+**
+** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855
+**
+** Wallace, P.T. & Capitaine, N., 2006, Astron.Astrophys. 459, 981
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double gamb, phib, psib, epsa, rbt[3][3];
+
+
+/* B matrix. */
+ iauPfw06(DJM0, DJM00, &gamb, &phib, &psib, &epsa);
+ iauFw2m(gamb, phib, psib, epsa, rb);
+
+/* PxB matrix. */
+ iauPmat06(date1, date2, rbp);
+
+/* P matrix. */
+ iauTr(rb, rbt);
+ iauRxr(rbp, rbt, rp);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/bpn2xy.c b/sofa/bpn2xy.c
new file mode 100644
index 0000000..c64b38e
--- /dev/null
+++ b/sofa/bpn2xy.c
@@ -0,0 +1,150 @@
+#include "sofam.h"
+
+void iauBpn2xy(double rbpn[3][3], double *x, double *y)
+/*
+** - - - - - - - - - -
+** i a u B p n 2 x y
+** - - - - - - - - - -
+**
+** Extract from the bias-precession-nutation matrix the X,Y coordinates
+** of the Celestial Intermediate Pole.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** rbpn double[3][3] celestial-to-true matrix (Note 1)
+**
+** Returned:
+** x,y double Celestial Intermediate Pole (Note 2)
+**
+** Notes:
+**
+** 1) The matrix rbpn transforms vectors from GCRS to true equator (and
+** CIO or equinox) of date, and therefore the Celestial Intermediate
+** Pole unit vector is the bottom row of the matrix.
+**
+** 2) The arguments x,y are components of the Celestial Intermediate
+** Pole unit vector in the Geocentric Celestial Reference System.
+**
+** Reference:
+**
+** "Expressions for the Celestial Intermediate Pole and Celestial
+** Ephemeris Origin consistent with the IAU 2000A precession-
+** nutation model", Astron.Astrophys. 400, 1145-1154
+** (2003)
+**
+** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
+** intermediate origin" (CIO) by IAU 2006 Resolution 2.
+**
+** This revision: 2010 January 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Extract the X,Y coordinates. */
+ *x = rbpn[2][0];
+ *y = rbpn[2][1];
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2i00a.c b/sofa/c2i00a.c
new file mode 100644
index 0000000..936c010
--- /dev/null
+++ b/sofa/c2i00a.c
@@ -0,0 +1,189 @@
+#include "sofam.h"
+
+void iauC2i00a(double date1, double date2, double rc2i[3][3])
+/*
+** - - - - - - - - - -
+** i a u C 2 i 0 0 a
+** - - - - - - - - - -
+**
+** Form the celestial-to-intermediate matrix for a given date using the
+** IAU 2000A precession-nutation model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rc2i double[3][3] celestial-to-intermediate matrix (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix rc2i is the first stage in the transformation from
+** celestial to terrestrial coordinates:
+**
+** [TRS] = RPOM * R_3(ERA) * rc2i * [CRS]
+**
+** = rc2t * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003), ERA is the Earth
+** Rotation Angle and RPOM is the polar motion matrix.
+**
+** 3) A faster, but slightly less accurate result (about 1 mas), can be
+** obtained by using instead the iauC2i00b function.
+**
+** Called:
+** iauPnm00a classical NPB matrix, IAU 2000A
+** iauC2ibpn celestial-to-intermediate matrix, given NPB matrix
+**
+** References:
+**
+** "Expressions for the Celestial Intermediate Pole and Celestial
+** Ephemeris Origin consistent with the IAU 2000A precession-
+** nutation model", Astron.Astrophys. 400, 1145-1154
+** (2003)
+**
+** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
+** intermediate origin" (CIO) by IAU 2006 Resolution 2.
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2010 January 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rbpn[3][3];
+
+
+/* Obtain the celestial-to-true matrix (IAU 2000A). */
+ iauPnm00a(date1, date2, rbpn);
+
+/* Form the celestial-to-intermediate matrix. */
+ iauC2ibpn(date1, date2, rbpn, rc2i);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2i00b.c b/sofa/c2i00b.c
new file mode 100644
index 0000000..24a48d3
--- /dev/null
+++ b/sofa/c2i00b.c
@@ -0,0 +1,189 @@
+#include "sofam.h"
+
+void iauC2i00b(double date1, double date2, double rc2i[3][3])
+/*
+** - - - - - - - - - -
+** i a u C 2 i 0 0 b
+** - - - - - - - - - -
+**
+** Form the celestial-to-intermediate matrix for a given date using the
+** IAU 2000B precession-nutation model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rc2i double[3][3] celestial-to-intermediate matrix (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix rc2i is the first stage in the transformation from
+** celestial to terrestrial coordinates:
+**
+** [TRS] = RPOM * R_3(ERA) * rc2i * [CRS]
+**
+** = rc2t * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003), ERA is the Earth
+** Rotation Angle and RPOM is the polar motion matrix.
+**
+** 3) The present function is faster, but slightly less accurate (about
+** 1 mas), than the iauC2i00a function.
+**
+** Called:
+** iauPnm00b classical NPB matrix, IAU 2000B
+** iauC2ibpn celestial-to-intermediate matrix, given NPB matrix
+**
+** References:
+**
+** "Expressions for the Celestial Intermediate Pole and Celestial
+** Ephemeris Origin consistent with the IAU 2000A precession-
+** nutation model", Astron.Astrophys. 400, 1145-1154
+** (2003)
+**
+** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
+** intermediate origin" (CIO) by IAU 2006 Resolution 2.
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2010 January 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rbpn[3][3];
+
+
+/* Obtain the celestial-to-true matrix (IAU 2000B). */
+ iauPnm00b(date1, date2, rbpn);
+
+/* Form the celestial-to-intermediate matrix. */
+ iauC2ibpn(date1, date2, rbpn, rc2i);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2i06a.c b/sofa/c2i06a.c
new file mode 100644
index 0000000..3ed93cc
--- /dev/null
+++ b/sofa/c2i06a.c
@@ -0,0 +1,186 @@
+#include "sofam.h"
+
+void iauC2i06a(double date1, double date2, double rc2i[3][3])
+/*
+** - - - - - - - - - -
+** i a u _ c 2 i 0 6 a
+** - - - - - - - - - -
+**
+** Form the celestial-to-intermediate matrix for a given date using the
+** IAU 2006 precession and IAU 2000A nutation models.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rc2i double[3][3] celestial-to-intermediate matrix (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix rc2i is the first stage in the transformation from
+** celestial to terrestrial coordinates:
+**
+** [TRS] = RPOM * R_3(ERA) * rc2i * [CRS]
+**
+** = RC2T * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003), ERA is the Earth
+** Rotation Angle and RPOM is the polar motion matrix.
+**
+** Called:
+** iauPnm06a classical NPB matrix, IAU 2006/2000A
+** iauBpn2xy extract CIP X,Y coordinates from NPB matrix
+** iauS06 the CIO locator s, Given X,Y, IAU 2006
+** iauC2ixys celestial-to-intermediate matrix, Given X,Y and s
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), 2004, IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG
+**
+** This revision: 2008 May 13
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rbpn[3][3], x, y, s;
+
+
+/* Obtain the celestial-to-true matrix (IAU 2006/2000A). */
+ iauPnm06a(date1, date2, rbpn);
+
+/* Extract the X,Y coordinates. */
+ iauBpn2xy(rbpn, &x, &y);
+
+/* Obtain the CIO locator. */
+ s = iauS06(date1, date2, x, y);
+
+/* Form the celestial-to-intermediate matrix. */
+ iauC2ixys(x, y, s, rc2i);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2ibpn.c b/sofa/c2ibpn.c
new file mode 100644
index 0000000..ff0ebe7
--- /dev/null
+++ b/sofa/c2ibpn.c
@@ -0,0 +1,192 @@
+#include "sofam.h"
+
+void iauC2ibpn(double date1, double date2, double rbpn[3][3],
+ double rc2i[3][3])
+/*
+** - - - - - - - - - -
+** i a u C 2 i b p n
+** - - - - - - - - - -
+**
+** Form the celestial-to-intermediate matrix for a given date given
+** the bias-precession-nutation matrix. IAU 2000.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+** rbpn double[3][3] celestial-to-true matrix (Note 2)
+**
+** Returned:
+** rc2i double[3][3] celestial-to-intermediate matrix (Note 3)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix rbpn transforms vectors from GCRS to true equator (and
+** CIO or equinox) of date. Only the CIP (bottom row) is used.
+**
+** 3) The matrix rc2i is the first stage in the transformation from
+** celestial to terrestrial coordinates:
+**
+** [TRS] = RPOM * R_3(ERA) * rc2i * [CRS]
+**
+** = RC2T * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003), ERA is the Earth
+** Rotation Angle and RPOM is the polar motion matrix.
+**
+** 4) Although its name does not include "00", This function is in fact
+** specific to the IAU 2000 models.
+**
+** Called:
+** iauBpn2xy extract CIP X,Y coordinates from NPB matrix
+** iauC2ixy celestial-to-intermediate matrix, given X,Y
+**
+** References:
+** "Expressions for the Celestial Intermediate Pole and Celestial
+** Ephemeris Origin consistent with the IAU 2000A precession-
+** nutation model", Astron.Astrophys. 400, 1145-1154 (2003)
+**
+** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
+** intermediate origin" (CIO) by IAU 2006 Resolution 2.
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2010 January 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double x, y;
+
+
+/* Extract the X,Y coordinates. */
+ iauBpn2xy(rbpn, &x, &y);
+
+/* Form the celestial-to-intermediate matrix (n.b. IAU 2000 specific). */
+ iauC2ixy(date1, date2, x, y, rc2i);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2ixy.c b/sofa/c2ixy.c
new file mode 100644
index 0000000..3c53b40
--- /dev/null
+++ b/sofa/c2ixy.c
@@ -0,0 +1,181 @@
+#include "sofam.h"
+
+void iauC2ixy(double date1, double date2, double x, double y,
+ double rc2i[3][3])
+/*
+** - - - - - - - - -
+** i a u C 2 i x y
+** - - - - - - - - -
+**
+** Form the celestial to intermediate-frame-of-date matrix for a given
+** date when the CIP X,Y coordinates are known. IAU 2000.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+** x,y double Celestial Intermediate Pole (Note 2)
+**
+** Returned:
+** rc2i double[3][3] celestial-to-intermediate matrix (Note 3)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The Celestial Intermediate Pole coordinates are the x,y components
+** of the unit vector in the Geocentric Celestial Reference System.
+**
+** 3) The matrix rc2i is the first stage in the transformation from
+** celestial to terrestrial coordinates:
+**
+** [TRS] = RPOM * R_3(ERA) * rc2i * [CRS]
+**
+** = RC2T * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003), ERA is the Earth
+** Rotation Angle and RPOM is the polar motion matrix.
+**
+** 4) Although its name does not include "00", This function is in fact
+** specific to the IAU 2000 models.
+**
+** Called:
+** iauC2ixys celestial-to-intermediate matrix, given X,Y and s
+** iauS00 the CIO locator s, given X,Y, IAU 2000A
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+
+{
+/* Compute s and then the matrix. */
+ iauC2ixys(x, y, iauS00(date1, date2, x, y), rc2i);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2ixys.c b/sofa/c2ixys.c
new file mode 100644
index 0000000..6c5b650
--- /dev/null
+++ b/sofa/c2ixys.c
@@ -0,0 +1,173 @@
+#include "sofam.h"
+
+void iauC2ixys(double x, double y, double s, double rc2i[3][3])
+/*
+** - - - - - - - - - -
+** i a u C 2 i x y s
+** - - - - - - - - - -
+**
+** Form the celestial to intermediate-frame-of-date matrix given the CIP
+** X,Y and the CIO locator s.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** x,y double Celestial Intermediate Pole (Note 1)
+** s double the CIO locator s (Note 2)
+**
+** Returned:
+** rc2i double[3][3] celestial-to-intermediate matrix (Note 3)
+**
+** Notes:
+**
+** 1) The Celestial Intermediate Pole coordinates are the x,y
+** components of the unit vector in the Geocentric Celestial
+** Reference System.
+**
+** 2) The CIO locator s (in radians) positions the Celestial
+** Intermediate Origin on the equator of the CIP.
+**
+** 3) The matrix rc2i is the first stage in the transformation from
+** celestial to terrestrial coordinates:
+**
+** [TRS] = RPOM * R_3(ERA) * rc2i * [CRS]
+**
+** = RC2T * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003), ERA is the Earth
+** Rotation Angle and RPOM is the polar motion matrix.
+**
+** Called:
+** iauIr initialize r-matrix to identity
+** iauRz rotate around Z-axis
+** iauRy rotate around Y-axis
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double r2, e, d;
+
+
+/* Obtain the spherical angles E and d. */
+ r2 = x*x + y*y;
+ e = (r2 != 0.0) ? atan2(y, x) : 0.0;
+ d = atan(sqrt(r2 / (1.0 - r2)));
+
+/* Form the matrix. */
+ iauIr(rc2i);
+ iauRz(e, rc2i);
+ iauRy(d, rc2i);
+ iauRz(-(e+s), rc2i);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2s.c b/sofa/c2s.c
new file mode 100644
index 0000000..02e5128
--- /dev/null
+++ b/sofa/c2s.c
@@ -0,0 +1,146 @@
+#include "sofam.h"
+
+void iauC2s(double p[3], double *theta, double *phi)
+/*
+** - - - - - - -
+** i a u C 2 s
+** - - - - - - -
+**
+** P-vector to spherical coordinates.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** p double[3] p-vector
+**
+** Returned:
+** theta double longitude angle (radians)
+** phi double latitude angle (radians)
+**
+** Notes:
+**
+** 1) The vector p can have any magnitude; only its direction is used.
+**
+** 2) If p is null, zero theta and phi are returned.
+**
+** 3) At either pole, zero theta is returned.
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double x, y, z, d2;
+
+
+ x = p[0];
+ y = p[1];
+ z = p[2];
+ d2 = x*x + y*y;
+
+ *theta = (d2 == 0.0) ? 0.0 : atan2(y, x);
+ *phi = (z == 0.0) ? 0.0 : atan2(z, sqrt(d2));
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2t00a.c b/sofa/c2t00a.c
new file mode 100644
index 0000000..ecd5fef
--- /dev/null
+++ b/sofa/c2t00a.c
@@ -0,0 +1,204 @@
+#include "sofam.h"
+
+void iauC2t00a(double tta, double ttb, double uta, double utb,
+ double xp, double yp, double rc2t[3][3])
+/*
+** - - - - - - - - - -
+** i a u C 2 t 0 0 a
+** - - - - - - - - - -
+**
+** Form the celestial to terrestrial matrix given the date, the UT1 and
+** the polar motion, using the IAU 2000A nutation model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** tta,ttb double TT as a 2-part Julian Date (Note 1)
+** uta,utb double UT1 as a 2-part Julian Date (Note 1)
+** xp,yp double coordinates of the pole (radians, Note 2)
+**
+** Returned:
+** rc2t double[3][3] celestial-to-terrestrial matrix (Note 3)
+**
+** Notes:
+**
+** 1) The TT and UT1 dates tta+ttb and uta+utb are Julian Dates,
+** apportioned in any convenient way between the arguments uta and
+** utb. For example, JD(UT1)=2450123.7 could be expressed in any of
+** these ways, among others:
+**
+** uta utb
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution is
+** acceptable. The J2000 and MJD methods are good compromises
+** between resolution and convenience. In the case of uta,utb, the
+** date & time method is best matched to the Earth rotation angle
+** algorithm used: maximum precision is delivered when the uta
+** argument is for 0hrs UT1 on the day in question and the utb
+** argument lies in the range 0 to 1, or vice versa.
+**
+** 2) The arguments xp and yp are the coordinates (in radians) of the
+** Celestial Intermediate Pole with respect to the International
+** Terrestrial Reference System (see IERS Conventions 2003),
+** measured along the meridians to 0 and 90 deg west respectively.
+**
+** 3) The matrix rc2t transforms from celestial to terrestrial
+** coordinates:
+**
+** [TRS] = RPOM * R_3(ERA) * RC2I * [CRS]
+**
+** = rc2t * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003), RC2I is the
+** celestial-to-intermediate matrix, ERA is the Earth rotation
+** angle and RPOM is the polar motion matrix.
+**
+** 4) A faster, but slightly less accurate result (about 1 mas), can
+** be obtained by using instead the iauC2t00b function.
+**
+** Called:
+** iauC2i00a celestial-to-intermediate matrix, IAU 2000A
+** iauEra00 Earth rotation angle, IAU 2000
+** iauSp00 the TIO locator s', IERS 2000
+** iauPom00 polar motion matrix
+** iauC2tcio form CIO-based celestial-to-terrestrial matrix
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2009 April 1
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rc2i[3][3], era, sp, rpom[3][3];
+
+
+/* Form the celestial-to-intermediate matrix for this TT (IAU 2000A). */
+ iauC2i00a(tta, ttb, rc2i );
+
+/* Predict the Earth rotation angle for this UT1. */
+ era = iauEra00(uta, utb);
+
+/* Estimate s'. */
+ sp = iauSp00(tta, ttb);
+
+/* Form the polar motion matrix. */
+ iauPom00(xp, yp, sp, rpom);
+
+/* Combine to form the celestial-to-terrestrial matrix. */
+ iauC2tcio(rc2i, era, rpom, rc2t);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2t00b.c b/sofa/c2t00b.c
new file mode 100644
index 0000000..b6116ef
--- /dev/null
+++ b/sofa/c2t00b.c
@@ -0,0 +1,200 @@
+#include "sofam.h"
+
+void iauC2t00b(double tta, double ttb, double uta, double utb,
+ double xp, double yp, double rc2t[3][3])
+/*
+** - - - - - - - - - -
+** i a u C 2 t 0 0 b
+** - - - - - - - - - -
+**
+** Form the celestial to terrestrial matrix given the date, the UT1 and
+** the polar motion, using the IAU 2000B nutation model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** tta,ttb double TT as a 2-part Julian Date (Note 1)
+** uta,utb double UT1 as a 2-part Julian Date (Note 1)
+** xp,yp double coordinates of the pole (radians, Note 2)
+**
+** Returned:
+** rc2t double[3][3] celestial-to-terrestrial matrix (Note 3)
+**
+** Notes:
+**
+** 1) The TT and UT1 dates tta+ttb and uta+utb are Julian Dates,
+** apportioned in any convenient way between the arguments uta and
+** utb. For example, JD(UT1)=2450123.7 could be expressed in any of
+** these ways, among others:
+**
+** uta utb
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution is
+** acceptable. The J2000 and MJD methods are good compromises
+** between resolution and convenience. In the case of uta,utb, the
+** date & time method is best matched to the Earth rotation angle
+** algorithm used: maximum precision is delivered when the uta
+** argument is for 0hrs UT1 on the day in question and the utb
+** argument lies in the range 0 to 1, or vice versa.
+**
+** 2) The arguments xp and yp are the coordinates (in radians) of the
+** Celestial Intermediate Pole with respect to the International
+** Terrestrial Reference System (see IERS Conventions 2003),
+** measured along the meridians to 0 and 90 deg west respectively.
+**
+** 3) The matrix rc2t transforms from celestial to terrestrial
+** coordinates:
+**
+** [TRS] = RPOM * R_3(ERA) * RC2I * [CRS]
+**
+** = rc2t * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003), RC2I is the
+** celestial-to-intermediate matrix, ERA is the Earth rotation
+** angle and RPOM is the polar motion matrix.
+**
+** 4) The present function is faster, but slightly less accurate (about
+** 1 mas), than the iauC2t00a function.
+**
+** Called:
+** iauC2i00b celestial-to-intermediate matrix, IAU 2000B
+** iauEra00 Earth rotation angle, IAU 2000
+** iauPom00 polar motion matrix
+** iauC2tcio form CIO-based celestial-to-terrestrial matrix
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2009 April 1
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rc2i[3][3], era, rpom[3][3];
+
+
+/* Form the celestial-to-intermediate matrix for this TT (IAU 2000B). */
+ iauC2i00b(tta, ttb, rc2i);
+
+/* Predict the Earth rotation angle for this UT1. */
+ era = iauEra00(uta, utb);
+
+/* Form the polar motion matrix (neglecting s'). */
+ iauPom00(xp, yp, 0.0, rpom);
+
+/* Combine to form the celestial-to-terrestrial matrix. */
+ iauC2tcio(rc2i, era, rpom, rc2t);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2t06a.c b/sofa/c2t06a.c
new file mode 100644
index 0000000..2b60eae
--- /dev/null
+++ b/sofa/c2t06a.c
@@ -0,0 +1,202 @@
+#include "sofam.h"
+
+void iauC2t06a(double tta, double ttb, double uta, double utb,
+ double xp, double yp, double rc2t[3][3])
+/*
+** - - - - - - - - - -
+** i a u C 2 t 0 6 a
+** - - - - - - - - - -
+**
+** Form the celestial to terrestrial matrix given the date, the UT1 and
+** the polar motion, using the IAU 2006 precession and IAU 2000A
+** nutation models.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** tta,ttb double TT as a 2-part Julian Date (Note 1)
+** uta,utb double UT1 as a 2-part Julian Date (Note 1)
+** xp,yp double coordinates of the pole (radians, Note 2)
+**
+** Returned:
+** rc2t double[3][3] celestial-to-terrestrial matrix (Note 3)
+**
+** Notes:
+**
+** 1) The TT and UT1 dates tta+ttb and uta+utb are Julian Dates,
+** apportioned in any convenient way between the arguments uta and
+** utb. For example, JD(UT1)=2450123.7 could be expressed in any of
+** these ways, among others:
+**
+** uta utb
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution is
+** acceptable. The J2000 and MJD methods are good compromises
+** between resolution and convenience. In the case of uta,utb, the
+** date & time method is best matched to the Earth rotation angle
+** algorithm used: maximum precision is delivered when the uta
+** argument is for 0hrs UT1 on the day in question and the utb
+** argument lies in the range 0 to 1, or vice versa.
+**
+** 2) The arguments xp and yp are the coordinates (in radians) of the
+** Celestial Intermediate Pole with respect to the International
+** Terrestrial Reference System (see IERS Conventions 2003),
+** measured along the meridians to 0 and 90 deg west respectively.
+**
+** 3) The matrix rc2t transforms from celestial to terrestrial
+** coordinates:
+**
+** [TRS] = RPOM * R_3(ERA) * RC2I * [CRS]
+**
+** = rc2t * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003), RC2I is the
+** celestial-to-intermediate matrix, ERA is the Earth rotation
+** angle and RPOM is the polar motion matrix.
+**
+** Called:
+** iauC2i06a celestial-to-intermediate matrix, IAU 2006/2000A
+** iauEra00 Earth rotation angle, IAU 2000
+** iauSp00 the TIO locator s', IERS 2000
+** iauPom00 polar motion matrix
+** iauC2tcio form CIO-based celestial-to-terrestrial matrix
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), 2004, IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG
+**
+** This revision: 2009 April 1
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rc2i[3][3], era, sp, rpom[3][3];
+
+
+/* Form the celestial-to-intermediate matrix for this TT. */
+ iauC2i06a(tta, ttb, rc2i);
+
+/* Predict the Earth rotation angle for this UT1. */
+ era = iauEra00(uta, utb);
+
+/* Estimate s'. */
+ sp = iauSp00(tta, ttb);
+
+/* Form the polar motion matrix. */
+ iauPom00(xp, yp, sp, rpom);
+
+/* Combine to form the celestial-to-terrestrial matrix. */
+ iauC2tcio(rc2i, era, rpom, rc2t);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2tcio.c b/sofa/c2tcio.c
new file mode 100644
index 0000000..71320a0
--- /dev/null
+++ b/sofa/c2tcio.c
@@ -0,0 +1,172 @@
+#include "sofam.h"
+
+void iauC2tcio(double rc2i[3][3], double era, double rpom[3][3],
+ double rc2t[3][3])
+/*
+** - - - - - - - - - -
+** i a u C 2 t c i o
+** - - - - - - - - - -
+**
+** Assemble the celestial to terrestrial matrix from CIO-based
+** components (the celestial-to-intermediate matrix, the Earth Rotation
+** Angle and the polar motion matrix).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** rc2i double[3][3] celestial-to-intermediate matrix
+** era double Earth rotation angle
+** rpom double[3][3] polar-motion matrix
+**
+** Returned:
+** rc2t double[3][3] celestial-to-terrestrial matrix
+**
+** Notes:
+**
+** 1) This function constructs the rotation matrix that transforms
+** vectors in the celestial system into vectors in the terrestrial
+** system. It does so starting from precomputed components, namely
+** the matrix which rotates from celestial coordinates to the
+** intermediate frame, the Earth rotation angle and the polar motion
+** matrix. One use of the present function is when generating a
+** series of celestial-to-terrestrial matrices where only the Earth
+** Rotation Angle changes, avoiding the considerable overhead of
+** recomputing the precession-nutation more often than necessary to
+** achieve given accuracy objectives.
+**
+** 2) The relationship between the arguments is as follows:
+**
+** [TRS] = RPOM * R_3(ERA) * rc2i * [CRS]
+**
+** = rc2t * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003).
+**
+** Called:
+** iauCr copy r-matrix
+** iauRz rotate around Z-axis
+** iauRxr product of two r-matrices
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), 2004, IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double r[3][3];
+
+
+/* Construct the matrix. */
+ iauCr(rc2i, r);
+ iauRz(era, r);
+ iauRxr(rpom, r, rc2t);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2teqx.c b/sofa/c2teqx.c
new file mode 100644
index 0000000..9632ca4
--- /dev/null
+++ b/sofa/c2teqx.c
@@ -0,0 +1,172 @@
+#include "sofam.h"
+
+void iauC2teqx(double rbpn[3][3], double gst, double rpom[3][3],
+ double rc2t[3][3])
+/*
+** - - - - - - - - - -
+** i a u C 2 t e q x
+** - - - - - - - - - -
+**
+** Assemble the celestial to terrestrial matrix from equinox-based
+** components (the celestial-to-true matrix, the Greenwich Apparent
+** Sidereal Time and the polar motion matrix).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** rbpn double[3][3] celestial-to-true matrix
+** gst double Greenwich (apparent) Sidereal Time
+** rpom double[3][3] polar-motion matrix
+**
+** Returned:
+** rc2t double[3][3] celestial-to-terrestrial matrix (Note 2)
+**
+** Notes:
+**
+** 1) This function constructs the rotation matrix that transforms
+** vectors in the celestial system into vectors in the terrestrial
+** system. It does so starting from precomputed components, namely
+** the matrix which rotates from celestial coordinates to the
+** true equator and equinox of date, the Greenwich Apparent Sidereal
+** Time and the polar motion matrix. One use of the present function
+** is when generating a series of celestial-to-terrestrial matrices
+** where only the Sidereal Time changes, avoiding the considerable
+** overhead of recomputing the precession-nutation more often than
+** necessary to achieve given accuracy objectives.
+**
+** 2) The relationship between the arguments is as follows:
+**
+** [TRS] = rpom * R_3(gst) * rbpn * [CRS]
+**
+** = rc2t * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003).
+**
+** Called:
+** iauCr copy r-matrix
+** iauRz rotate around Z-axis
+** iauRxr product of two r-matrices
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double r[3][3];
+
+
+/* Construct the matrix. */
+ iauCr(rbpn, r);
+ iauRz(gst, r);
+ iauRxr(rpom, r, rc2t);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2tpe.c b/sofa/c2tpe.c
new file mode 100644
index 0000000..281cd93
--- /dev/null
+++ b/sofa/c2tpe.c
@@ -0,0 +1,217 @@
+#include "sofam.h"
+
+void iauC2tpe(double tta, double ttb, double uta, double utb,
+ double dpsi, double deps, double xp, double yp,
+ double rc2t[3][3])
+/*
+** - - - - - - - - -
+** i a u C 2 t p e
+** - - - - - - - - -
+**
+** Form the celestial to terrestrial matrix given the date, the UT1,
+** the nutation and the polar motion. IAU 2000.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** tta,ttb double TT as a 2-part Julian Date (Note 1)
+** uta,utb double UT1 as a 2-part Julian Date (Note 1)
+** dpsi,deps double nutation (Note 2)
+** xp,yp double coordinates of the pole (radians, Note 3)
+**
+** Returned:
+** rc2t double[3][3] celestial-to-terrestrial matrix (Note 4)
+**
+** Notes:
+**
+** 1) The TT and UT1 dates tta+ttb and uta+utb are Julian Dates,
+** apportioned in any convenient way between the arguments uta and
+** utb. For example, JD(UT1)=2450123.7 could be expressed in any of
+** these ways, among others:
+**
+** uta utb
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution is
+** acceptable. The J2000 and MJD methods are good compromises
+** between resolution and convenience. In the case of uta,utb, the
+** date & time method is best matched to the Earth rotation angle
+** algorithm used: maximum precision is delivered when the uta
+** argument is for 0hrs UT1 on the day in question and the utb
+** argument lies in the range 0 to 1, or vice versa.
+**
+** 2) The caller is responsible for providing the nutation components;
+** they are in longitude and obliquity, in radians and are with
+** respect to the equinox and ecliptic of date. For high-accuracy
+** applications, free core nutation should be included as well as
+** any other relevant corrections to the position of the CIP.
+**
+** 3) The arguments xp and yp are the coordinates (in radians) of the
+** Celestial Intermediate Pole with respect to the International
+** Terrestrial Reference System (see IERS Conventions 2003),
+** measured along the meridians to 0 and 90 deg west respectively.
+**
+** 4) The matrix rc2t transforms from celestial to terrestrial
+** coordinates:
+**
+** [TRS] = RPOM * R_3(GST) * RBPN * [CRS]
+**
+** = rc2t * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003), RBPN is the
+** bias-precession-nutation matrix, GST is the Greenwich (apparent)
+** Sidereal Time and RPOM is the polar motion matrix.
+**
+** 5) Although its name does not include "00", This function is in fact
+** specific to the IAU 2000 models.
+**
+** Called:
+** iauPn00 bias/precession/nutation results, IAU 2000
+** iauGmst00 Greenwich mean sidereal time, IAU 2000
+** iauSp00 the TIO locator s', IERS 2000
+** iauEe00 equation of the equinoxes, IAU 2000
+** iauPom00 polar motion matrix
+** iauC2teqx form equinox-based celestial-to-terrestrial matrix
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2009 April 1
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double epsa, rb[3][3], rp[3][3], rbp[3][3], rn[3][3],
+ rbpn[3][3], gmst, ee, sp, rpom[3][3];
+
+
+/* Form the celestial-to-true matrix for this TT. */
+ iauPn00(tta, ttb, dpsi, deps, &epsa, rb, rp, rbp, rn, rbpn);
+
+/* Predict the Greenwich Mean Sidereal Time for this UT1 and TT. */
+ gmst = iauGmst00(uta, utb, tta, ttb);
+
+/* Predict the equation of the equinoxes given TT and nutation. */
+ ee = iauEe00(tta, ttb, epsa, dpsi);
+
+/* Estimate s'. */
+ sp = iauSp00(tta, ttb);
+
+/* Form the polar motion matrix. */
+ iauPom00(xp, yp, sp, rpom);
+
+/* Combine to form the celestial-to-terrestrial matrix. */
+ iauC2teqx(rbpn, gmst + ee, rpom, rc2t);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/c2txy.c b/sofa/c2txy.c
new file mode 100644
index 0000000..5ee1280
--- /dev/null
+++ b/sofa/c2txy.c
@@ -0,0 +1,209 @@
+#include "sofam.h"
+
+void iauC2txy(double tta, double ttb, double uta, double utb,
+ double x, double y, double xp, double yp,
+ double rc2t[3][3])
+/*
+** - - - - - - - - -
+** i a u C 2 t x y
+** - - - - - - - - -
+**
+** Form the celestial to terrestrial matrix given the date, the UT1,
+** the CIP coordinates and the polar motion. IAU 2000.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** tta,ttb double TT as a 2-part Julian Date (Note 1)
+** uta,utb double UT1 as a 2-part Julian Date (Note 1)
+** x,y double Celestial Intermediate Pole (Note 2)
+** xp,yp double coordinates of the pole (radians, Note 3)
+**
+** Returned:
+** rc2t double[3][3] celestial-to-terrestrial matrix (Note 4)
+**
+** Notes:
+**
+** 1) The TT and UT1 dates tta+ttb and uta+utb are Julian Dates,
+** apportioned in any convenient way between the arguments uta and
+** utb. For example, JD(UT1)=2450123.7 could be expressed in any o
+** these ways, among others:
+**
+** uta utb
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution is
+** acceptable. The J2000 and MJD methods are good compromises
+** between resolution and convenience. In the case of uta,utb, the
+** date & time method is best matched to the Earth rotation angle
+** algorithm used: maximum precision is delivered when the uta
+** argument is for 0hrs UT1 on the day in question and the utb
+** argument lies in the range 0 to 1, or vice versa.
+**
+** 2) The Celestial Intermediate Pole coordinates are the x,y
+** components of the unit vector in the Geocentric Celestial
+** Reference System.
+**
+** 3) The arguments xp and yp are the coordinates (in radians) of the
+** Celestial Intermediate Pole with respect to the International
+** Terrestrial Reference System (see IERS Conventions 2003),
+** measured along the meridians to 0 and 90 deg west respectively.
+**
+** 4) The matrix rc2t transforms from celestial to terrestrial
+** coordinates:
+**
+** [TRS] = RPOM * R_3(ERA) * RC2I * [CRS]
+**
+** = rc2t * [CRS]
+**
+** where [CRS] is a vector in the Geocentric Celestial Reference
+** System and [TRS] is a vector in the International Terrestrial
+** Reference System (see IERS Conventions 2003), ERA is the Earth
+** Rotation Angle and RPOM is the polar motion matrix.
+**
+** 5) Although its name does not include "00", This function is in fact
+** specific to the IAU 2000 models.
+**
+** Called:
+** iauC2ixy celestial-to-intermediate matrix, given X,Y
+** iauEra00 Earth rotation angle, IAU 2000
+** iauSp00 the TIO locator s', IERS 2000
+** iauPom00 polar motion matrix
+** iauC2tcio form CIO-based celestial-to-terrestrial matrix
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2009 April 1
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rc2i[3][3], era, sp, rpom[3][3];
+
+
+/* Form the celestial-to-intermediate matrix for this TT. */
+ iauC2ixy(tta, ttb, x, y, rc2i);
+
+/* Predict the Earth rotation angle for this UT1. */
+ era = iauEra00(uta, utb);
+
+/* Estimate s'. */
+ sp = iauSp00(tta, ttb);
+
+/* Form the polar motion matrix. */
+ iauPom00(xp, yp, sp, rpom);
+
+/* Combine to form the celestial-to-terrestrial matrix. */
+ iauC2tcio(rc2i, era, rpom, rc2t);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/cal2jd.c b/sofa/cal2jd.c
new file mode 100644
index 0000000..0d6c154
--- /dev/null
+++ b/sofa/cal2jd.c
@@ -0,0 +1,189 @@
+#include "sofam.h"
+
+int iauCal2jd(int iy, int im, int id, double *djm0, double *djm)
+/*
+** - - - - - - - - - -
+** i a u C a l 2 j d
+** - - - - - - - - - -
+**
+** Gregorian Calendar to Julian Date.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** iy,im,id int year, month, day in Gregorian calendar (Note 1)
+**
+** Returned:
+** djm0 double MJD zero-point: always 2400000.5
+** djm double Modified Julian Date for 0 hrs
+**
+** Returned (function value):
+** int status:
+** 0 = OK
+** -1 = bad year (Note 3: JD not computed)
+** -2 = bad month (JD not computed)
+** -3 = bad day (JD computed)
+**
+** Notes:
+**
+** 1) The algorithm used is valid from -4800 March 1, but this
+** implementation rejects dates before -4799 January 1.
+**
+** 2) The Julian Date is returned in two pieces, in the usual SOFA
+** manner, which is designed to preserve time resolution. The
+** Julian Date is available as a single number by adding djm0 and
+** djm.
+**
+** 3) In early eras the conversion is from the "Proleptic Gregorian
+** Calendar"; no account is taken of the date(s) of adoption of
+** the Gregorian Calendar, nor is the AD/BC numbering convention
+** observed.
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992),
+** Section 12.92 (p604).
+**
+** This revision: 2009 October 19
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int j, ly, my;
+ long iypmy;
+
+/* Earliest year allowed (4800BC) */
+ const int IYMIN = -4799;
+
+/* Month lengths in days */
+ static const int mtab[]
+ = {31, 28, 31, 30, 31, 30, 31, 31, 30, 31, 30, 31};
+
+
+/* Preset status. */
+ j = 0;
+
+/* Validate year and month. */
+ if (iy < IYMIN) return -1;
+ if (im < 1 || im > 12) return -2;
+
+/* If February in a leap year, 1, otherwise 0. */
+ ly = ((im == 2) && !(iy%4) && (iy%100 || !(iy%400)));
+
+/* Validate day, taking into account leap years. */
+ if ( (id < 1) || (id > (mtab[im-1] + ly))) j = -3;
+
+/* Return result. */
+ my = (im - 14) / 12;
+ iypmy = (long) (iy + my);
+ *djm0 = 2400000.5;
+ *djm = (double)((1461L * (iypmy + 4800L)) / 4L
+ + (367L * (long) (im - 2 - 12 * my)) / 12L
+ - (3L * ((iypmy + 4900L) / 100L)) / 4L
+ + (long) id - 2432076L);
+
+/* Return status. */
+ return j;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/cp.c b/sofa/cp.c
new file mode 100644
index 0000000..1c13587
--- /dev/null
+++ b/sofa/cp.c
@@ -0,0 +1,130 @@
+#include "sofam.h"
+
+void iauCp(double p[3], double c[3])
+/*
+** - - - - - -
+** i a u C p
+** - - - - - -
+**
+** Copy a p-vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** p double[3] p-vector to be copied
+**
+** Returned:
+** c double[3] copy
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ c[0] = p[0];
+ c[1] = p[1];
+ c[2] = p[2];
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/cpv.c b/sofa/cpv.c
new file mode 100644
index 0000000..2f9698b
--- /dev/null
+++ b/sofa/cpv.c
@@ -0,0 +1,132 @@
+#include "sofam.h"
+
+void iauCpv(double pv[2][3], double c[2][3])
+/*
+** - - - - - - -
+** i a u C p v
+** - - - - - - -
+**
+** Copy a position/velocity vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** pv double[2][3] position/velocity vector to be copied
+**
+** Returned:
+** c double[2][3] copy
+**
+** Called:
+** iauCp copy p-vector
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauCp(pv[0], c[0]);
+ iauCp(pv[1], c[1]);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/cr.c b/sofa/cr.c
new file mode 100644
index 0000000..9c4ee7e
--- /dev/null
+++ b/sofa/cr.c
@@ -0,0 +1,133 @@
+#include "sofam.h"
+
+void iauCr(double r[3][3], double c[3][3])
+/*
+** - - - - - -
+** i a u C r
+** - - - - - -
+**
+** Copy an r-matrix.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** r double[3][3] r-matrix to be copied
+**
+** Returned:
+** char[] double[3][3] copy
+**
+** Called:
+** iauCp copy p-vector
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauCp(r[0], c[0]);
+ iauCp(r[1], c[1]);
+ iauCp(r[2], c[2]);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/d2dtf.c b/sofa/d2dtf.c
new file mode 100644
index 0000000..f84ac3f
--- /dev/null
+++ b/sofa/d2dtf.c
@@ -0,0 +1,256 @@
+#include "sofam.h"
+#include <string.h>
+
+int iauD2dtf(const char *scale, int ndp, double d1, double d2,
+ int *iy, int *im, int *id, int ihmsf[4])
+/*
+** - - - - - - - - -
+** i a u D 2 d t f
+** - - - - - - - - -
+**
+** Format for output a 2-part Julian Date (or in the case of UTC a
+** quasi-JD form that includes special provision for leap seconds).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** scale char[] time scale ID (Note 1)
+** ndp int resolution (Note 2)
+** d1,d2 double time as a 2-part Julian Date (Notes 3,4)
+**
+** Returned:
+** iy,im,id int year, month, day in Gregorian calendar (Note 5)
+** ihmsf int[4] hours, minutes, seconds, fraction (Note 1)
+**
+** Returned (function value):
+** int status: +1 = dubious year (Note 5)
+** 0 = OK
+** -1 = unacceptable date (Note 6)
+**
+** Notes:
+**
+** 1) scale identifies the time scale. Only the value "UTC" (in upper
+** case) is significant, and enables handling of leap seconds (see
+** Note 4).
+**
+** 2) ndp is the number of decimal places in the seconds field, and can
+** have negative as well as positive values, such as:
+**
+** ndp resolution
+** -4 1 00 00
+** -3 0 10 00
+** -2 0 01 00
+** -1 0 00 10
+** 0 0 00 01
+** 1 0 00 00.1
+** 2 0 00 00.01
+** 3 0 00 00.001
+**
+** The limits are platform dependent, but a safe range is -5 to +9.
+**
+** 3) d1+d2 is Julian Date, apportioned in any convenient way between
+** the two arguments, for example where d1 is the Julian Day Number
+** and d2 is the fraction of a day. In the case of UTC, where the
+** use of JD is problematical, special conventions apply: see the
+** next note.
+**
+** 4) JD cannot unambiguously represent UTC during a leap second unless
+** special measures are taken. The SOFA internal convention is that
+** the quasi-JD day represents UTC days whether the length is 86399,
+** 86400 or 86401 SI seconds.
+**
+** 5) The warning status "dubious year" flags UTCs that predate the
+** introduction of the time scale and that are too far in the future
+** to be trusted. See iauDat for further details.
+**
+** 6) For calendar conventions and limitations, see iauCal2jd.
+**
+** Called:
+** iauJd2cal JD to Gregorian calendar
+** iauD2tf decompose days to hms
+** iauDat delta(AT) = TAI-UTC
+**
+** This revision: 2012 February 12
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int leap;
+ char s;
+ int iy1, im1, id1, js, iy2, im2, id2, ihmsf1[4], i;
+ double a1, b1, fd, dat1, w, dat2, ddt;
+
+
+/* The two-part JD. */
+ a1 = d1;
+ b1 = d2;
+
+/* Provisional calendar date. */
+ js = iauJd2cal(a1, b1, &iy1, &im1, &id1, &fd);
+ if ( js ) return js < 0 ? -1 : js;
+
+/* Is this a leap second day? */
+ leap = 0;
+ if ( ! strcmp(scale,"UTC") ) {
+
+ /* TAI-UTC today. */
+ js = iauDat(iy1, im1, id1, fd, &dat1);
+ if ( js < 0 ) return -1;
+
+ /* TAI-UTC tomorrow (at noon, to avoid rounding effects). */
+ js = iauJd2cal(a1+1.5, b1-fd, &iy2, &im2, &id2, &w);
+ js = iauDat(iy2, im2, id2, 0.0, &dat2);
+ if ( js < 0 ) return -1;
+
+ /* The change in TAI-UTC (seconds). */
+ ddt = dat2 - dat1;
+
+ /* If leap second day, scale the fraction of a day into SI. */
+ leap = fabs(ddt) > 0.5;
+ if (leap) fd += fd * ddt/DAYSEC;
+ }
+
+/* Provisional time of day. */
+ iauD2tf ( ndp, fd, &s, ihmsf1 );
+
+/* Is this a leap second day? */
+ if ( ! leap ) {
+
+ /* No. Has the time rounded up to 24h? */
+ if ( ihmsf1[0] > 23 ) {
+
+ /* Yes. We will need tomorrow's calendar date. */
+ js = iauJd2cal(a1+1.5, b1-fd, &iy2, &im2, &id2, &w);
+
+ /* Use 0h tomorrow. */
+ iy1 = iy2;
+ im1 = im2;
+ id1 = id2;
+ for ( i = 0; i < 4; i++ ) {
+ ihmsf1[i] = 0;
+ }
+ }
+ } else {
+
+ /* This is a leap second day. Has the time reached or passed 24h? */
+ if ( ihmsf1[0] > 23 ) {
+
+ /* Yes. Use 23 59 60... */
+ ihmsf1[0] = 23;
+ ihmsf1[1] = 59;
+ ihmsf1[2] = 60;
+ }
+ }
+
+/* Results. */
+ *iy = iy1;
+ *im = im1;
+ *id = id1;
+ for ( i = 0; i < 4; i++ ) {
+ ihmsf[i] = ihmsf1[i];
+ }
+
+/* Status. */
+ return js < 0 ? -1 : js;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/d2tf.c b/sofa/d2tf.c
new file mode 100644
index 0000000..d887f34
--- /dev/null
+++ b/sofa/d2tf.c
@@ -0,0 +1,210 @@
+#include "sofam.h"
+
+void iauD2tf(int ndp, double days, char *sign, int ihmsf[4])
+/*
+** - - - - - - - -
+** i a u D 2 t f
+** - - - - - - - -
+**
+** Decompose days to hours, minutes, seconds, fraction.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** ndp int resolution (Note 1)
+** days double interval in days
+**
+** Returned:
+** sign char '+' or '-'
+** ihmsf int[4] hours, minutes, seconds, fraction
+**
+** Notes:
+**
+** 1) The argument ndp is interpreted as follows:
+**
+** ndp resolution
+** : ...0000 00 00
+** -7 1000 00 00
+** -6 100 00 00
+** -5 10 00 00
+** -4 1 00 00
+** -3 0 10 00
+** -2 0 01 00
+** -1 0 00 10
+** 0 0 00 01
+** 1 0 00 00.1
+** 2 0 00 00.01
+** 3 0 00 00.001
+** : 0 00 00.000...
+**
+** 2) The largest positive useful value for ndp is determined by the
+** size of days, the format of double on the target platform, and
+** the risk of overflowing ihmsf[3]. On a typical platform, for
+** days up to 1.0, the available floating-point precision might
+** correspond to ndp=12. However, the practical limit is typically
+** ndp=9, set by the capacity of a 32-bit int, or ndp=4 if int is
+** only 16 bits.
+**
+** 3) The absolute value of days may exceed 1.0. In cases where it
+** does not, it is up to the caller to test for and handle the
+** case where days is very nearly 1.0 and rounds up to 24 hours,
+** by testing for ihmsf[0]=24 and setting ihmsf[0-3] to zero.
+**
+** This revision: 2008 May 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int nrs, n;
+ double rs, rm, rh, a, w, ah, am, as, af;
+
+
+/* Handle sign. */
+ *sign = (char) ( ( days >= 0.0 ) ? '+' : '-' );
+
+/* Interval in seconds. */
+ a = DAYSEC * fabs(days);
+
+/* Pre-round if resolution coarser than 1s (then pretend ndp=1). */
+ if (ndp < 0) {
+ nrs = 1;
+ for (n = 1; n <= -ndp; n++) {
+ nrs *= (n == 2 || n == 4) ? 6 : 10;
+ }
+ rs = (double) nrs;
+ w = a / rs;
+ a = rs * dnint(w);
+ }
+
+/* Express the unit of each field in resolution units. */
+ nrs = 1;
+ for (n = 1; n <= ndp; n++) {
+ nrs *= 10;
+ }
+ rs = (double) nrs;
+ rm = rs * 60.0;
+ rh = rm * 60.0;
+
+/* Round the interval and express in resolution units. */
+ a = dnint(rs * a);
+
+/* Break into fields. */
+ ah = a / rh;
+ ah = dint(ah);
+ a -= ah * rh;
+ am = a / rm;
+ am = dint(am);
+ a -= am * rm;
+ as = a / rs;
+ as = dint(as);
+ af = a - as * rs;
+
+/* Return results. */
+ ihmsf[0] = (int) ah;
+ ihmsf[1] = (int) am;
+ ihmsf[2] = (int) as;
+ ihmsf[3] = (int) af;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/dat.c b/sofa/dat.c
new file mode 100644
index 0000000..4ca053b
--- /dev/null
+++ b/sofa/dat.c
@@ -0,0 +1,339 @@
+#include "sofam.h"
+
+int iauDat(int iy, int im, int id, double fd, double *deltat )
+/*
+** - - - - - - -
+** i a u D a t
+** - - - - - - -
+**
+** For a given UTC date, calculate delta(AT) = TAI-UTC.
+**
+** :------------------------------------------:
+** : :
+** : IMPORTANT :
+** : :
+** : A new version of this function must be :
+** : produced whenever a new leap second is :
+** : announced. There are four items to :
+** : change on each such occasion: :
+** : :
+** : 1) A new line must be added to the set :
+** : of statements that initialize the :
+** : array "changes". :
+** : :
+** : 2) The parameter IYV must be set to :
+** : the current year. :
+** : :
+** : 3) The "Latest leap second" comment :
+** : below must be set to the new leap :
+** : second date. :
+** : :
+** : 4) The "This revision" comment, later, :
+** : must be set to the current date. :
+** : :
+** : Change (2) must also be carried out :
+** : whenever the function is re-issued, :
+** : even if no leap seconds have been :
+** : added. :
+** : :
+** : Latest leap second: 2012 June 30 :
+** : :
+** :__________________________________________:
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** iy int UTC: year (Notes 1 and 2)
+** im int month (Note 2)
+** id int day (Notes 2 and 3)
+** fd double fraction of day (Note 4)
+**
+** Returned:
+** deltat double TAI minus UTC, seconds
+**
+** Returned (function value):
+** int status (Note 5):
+** 1 = dubious year (Note 1)
+** 0 = OK
+** -1 = bad year
+** -2 = bad month
+** -3 = bad day (Note 3)
+** -4 = bad fraction (Note 4)
+**
+** Notes:
+**
+** 1) UTC began at 1960 January 1.0 (JD 2436934.5) and it is improper
+** to call the function with an earlier date. If this is attempted,
+** zero is returned together with a warning status.
+**
+** Because leap seconds cannot, in principle, be predicted in
+** advance, a reliable check for dates beyond the valid range is
+** impossible. To guard against gross errors, a year five or more
+** after the release year of the present function (see parameter
+** IYV) is considered dubious. In this case a warning status is
+** returned but the result is computed in the normal way.
+**
+** For both too-early and too-late years, the warning status is
+** j=+1. This is distinct from the error status j=-1, which
+** signifies a year so early that JD could not be computed.
+**
+** 2) If the specified date is for a day which ends with a leap second,
+** the UTC-TAI value returned is for the period leading up to the
+** leap second. If the date is for a day which begins as a leap
+** second ends, the UTC-TAI returned is for the period following the
+** leap second.
+**
+** 3) The day number must be in the normal calendar range, for example
+** 1 through 30 for April. The "almanac" convention of allowing
+** such dates as January 0 and December 32 is not supported in this
+** function, in order to avoid confusion near leap seconds.
+**
+** 4) The fraction of day is used only for dates before the
+** introduction of leap seconds, the first of which occurred at the
+** end of 1971. It is tested for validity (zero to less than 1 is
+** the valid range) even if not used; if invalid, zero is used and
+** status j=-4 is returned. For many applications, setting fd to
+** zero is acceptable; the resulting error is always less than 3 ms
+** (and occurs only pre-1972).
+**
+** 5) The status value returned in the case where there are multiple
+** errors refers to the first error detected. For example, if the
+** month and day are 13 and 32 respectively, j=-2 (bad month)
+** will be returned.
+**
+** 6) In cases where a valid result is not available, zero is returned.
+**
+** References:
+**
+** 1) For dates from 1961 January 1 onwards, the expressions from the
+** file ftp://maia.usno.navy.mil/ser7/tai-utc.dat are used.
+**
+** 2) The 5ms timestep at 1961 January 1 is taken from 2.58.1 (p87) of
+** the 1992 Explanatory Supplement.
+**
+** Called:
+** iauCal2jd Gregorian calendar to Julian Day number
+**
+** This revision: 2012 January 5
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Release year for this version of iauDat */
+#define IYV (2012)
+
+/* Reference dates (MJD) and drift rates (s/day), pre leap seconds */
+ static const double drift[][2] = {
+ { 37300.0, 0.0012960 },
+ { 37300.0, 0.0012960 },
+ { 37300.0, 0.0012960 },
+ { 37665.0, 0.0011232 },
+ { 37665.0, 0.0011232 },
+ { 38761.0, 0.0012960 },
+ { 38761.0, 0.0012960 },
+ { 38761.0, 0.0012960 },
+ { 38761.0, 0.0012960 },
+ { 38761.0, 0.0012960 },
+ { 38761.0, 0.0012960 },
+ { 38761.0, 0.0012960 },
+ { 39126.0, 0.0025920 },
+ { 39126.0, 0.0025920 }
+ };
+
+/* Number of Delta(AT) expressions before leap seconds were introduced */
+#define NERA1 ((int) (sizeof drift / sizeof (double) / 2))
+
+/* Dates and Delta(AT)s */
+ static const struct {
+ int iyear, month;
+ double delat;
+ } changes[] = {
+ { 1960, 1, 1.4178180 },
+ { 1961, 1, 1.4228180 },
+ { 1961, 8, 1.3728180 },
+ { 1962, 1, 1.8458580 },
+ { 1963, 11, 1.9458580 },
+ { 1964, 1, 3.2401300 },
+ { 1964, 4, 3.3401300 },
+ { 1964, 9, 3.4401300 },
+ { 1965, 1, 3.5401300 },
+ { 1965, 3, 3.6401300 },
+ { 1965, 7, 3.7401300 },
+ { 1965, 9, 3.8401300 },
+ { 1966, 1, 4.3131700 },
+ { 1968, 2, 4.2131700 },
+ { 1972, 1, 10.0 },
+ { 1972, 7, 11.0 },
+ { 1973, 1, 12.0 },
+ { 1974, 1, 13.0 },
+ { 1975, 1, 14.0 },
+ { 1976, 1, 15.0 },
+ { 1977, 1, 16.0 },
+ { 1978, 1, 17.0 },
+ { 1979, 1, 18.0 },
+ { 1980, 1, 19.0 },
+ { 1981, 7, 20.0 },
+ { 1982, 7, 21.0 },
+ { 1983, 7, 22.0 },
+ { 1985, 7, 23.0 },
+ { 1988, 1, 24.0 },
+ { 1990, 1, 25.0 },
+ { 1991, 1, 26.0 },
+ { 1992, 7, 27.0 },
+ { 1993, 7, 28.0 },
+ { 1994, 7, 29.0 },
+ { 1996, 1, 30.0 },
+ { 1997, 7, 31.0 },
+ { 1999, 1, 32.0 },
+ { 2006, 1, 33.0 },
+ { 2009, 1, 34.0 },
+ { 2012, 7, 35.0 }
+ };
+
+/* Number of Delta(AT) changes */
+ const int NDAT = sizeof changes / sizeof changes[0];
+
+/* Miscellaneous local variables */
+ int j, i, m;
+ double da, djm0, djm;
+
+
+/* Initialize the result to zero. */
+ *deltat = da = 0.0;
+
+/* If invalid fraction of a day, set error status and give up. */
+ if (fd < 0.0 || fd >= 1.0) return -4;
+
+/* Convert the date into an MJD. */
+ j = iauCal2jd(iy, im, id, &djm0, &djm);
+
+/* If invalid year, month, or day, give up. */
+ if (j < 0) return j;
+
+/* If pre-UTC year, set warning status and give up. */
+ if (iy < changes[0].iyear) return 1;
+
+/* If suspiciously late year, set warning status but proceed. */
+ if (iy > IYV + 5) j = 1;
+
+/* Combine year and month to form a date-ordered integer... */
+ m = 12*iy + im;
+
+/* ...and use it to find the preceding table entry. */
+ for (i = NDAT-1; i >=0; i--) {
+ if (m >= (12 * changes[i].iyear + changes[i].month)) break;
+ }
+
+/* Get the Delta(AT). */
+ da = changes[i].delat;
+
+/* If pre-1972, adjust for drift. */
+ if (i < NERA1) da += (djm + fd - drift[i][0]) * drift[i][1];
+
+/* Return the Delta(AT) value. */
+ *deltat = da;
+
+/* Return the status. */
+ return j;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/dtdb.c b/sofa/dtdb.c
new file mode 100644
index 0000000..0048dbe
--- /dev/null
+++ b/sofa/dtdb.c
@@ -0,0 +1,1263 @@
+#include "sofam.h"
+
+double iauDtdb(double date1, double date2,
+ double ut, double elong, double u, double v)
+/*
+** - - - - - - - -
+** i a u D t d b
+** - - - - - - - -
+**
+** An approximation to TDB-TT, the difference between barycentric
+** dynamical time and terrestrial time, for an observer on the Earth.
+**
+** The different time scales - proper, coordinate and realized - are
+** related to each other:
+**
+** TAI <- physically realized
+** :
+** offset <- observed (nominally +32.184s)
+** :
+** TT <- terrestrial time
+** :
+** rate adjustment (L_G) <- definition of TT
+** :
+** TCG <- time scale for GCRS
+** :
+** "periodic" terms <- iauDtdb is an implementation
+** :
+** rate adjustment (L_C) <- function of solar-system ephemeris
+** :
+** TCB <- time scale for BCRS
+** :
+** rate adjustment (-L_B) <- definition of TDB
+** :
+** TDB <- TCB scaled to track TT
+** :
+** "periodic" terms <- -iauDtdb is an approximation
+** :
+** TT <- terrestrial time
+**
+** Adopted values for the various constants can be found in the IERS
+** Conventions (McCarthy & Petit 2003).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support routine.
+**
+** Given:
+** date1,date2 double date, TDB (Notes 1-3)
+** ut double universal time (UT1, fraction of one day)
+** elong double longitude (east positive, radians)
+** u double distance from Earth spin axis (km)
+** v double distance north of equatorial plane (km)
+**
+** Returned (function value):
+** double TDB-TT (seconds)
+**
+** Notes:
+**
+** 1) The date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** Although the date is, formally, barycentric dynamical time (TDB),
+** the terrestrial dynamical time (TT) can be used with no practical
+** effect on the accuracy of the prediction.
+**
+** 2) TT can be regarded as a coordinate time that is realized as an
+** offset of 32.184s from International Atomic Time, TAI. TT is a
+** specific linear transformation of geocentric coordinate time TCG,
+** which is the time scale for the Geocentric Celestial Reference
+** System, GCRS.
+**
+** 3) TDB is a coordinate time, and is a specific linear transformation
+** of barycentric coordinate time TCB, which is the time scale for
+** the Barycentric Celestial Reference System, BCRS.
+**
+** 4) The difference TCG-TCB depends on the masses and positions of the
+** bodies of the solar system and the velocity of the Earth. It is
+** dominated by a rate difference, the residual being of a periodic
+** character. The latter, which is modeled by the present function,
+** comprises a main (annual) sinusoidal term of amplitude
+** approximately 0.00166 seconds, plus planetary terms up to about
+** 20 microseconds, and lunar and diurnal terms up to 2 microseconds.
+** These effects come from the changing transverse Doppler effect
+** and gravitational red-shift as the observer (on the Earth's
+** surface) experiences variations in speed (with respect to the
+** BCRS) and gravitational potential.
+**
+** 5) TDB can be regarded as the same as TCB but with a rate adjustment
+** to keep it close to TT, which is convenient for many applications.
+** The history of successive attempts to define TDB is set out in
+** Resolution 3 adopted by the IAU General Assembly in 2006, which
+** defines a fixed TDB(TCB) transformation that is consistent with
+** contemporary solar-system ephemerides. Future ephemerides will
+** imply slightly changed transformations between TCG and TCB, which
+** could introduce a linear drift between TDB and TT; however, any
+** such drift is unlikely to exceed 1 nanosecond per century.
+**
+** 6) The geocentric TDB-TT model used in the present function is that of
+** Fairhead & Bretagnon (1990), in its full form. It was originally
+** supplied by Fairhead (private communications with P.T.Wallace,
+** 1990) as a Fortran subroutine. The present C function contains an
+** adaptation of the Fairhead code. The numerical results are
+** essentially unaffected by the changes, the differences with
+** respect to the Fairhead & Bretagnon original being at the 1e-20 s
+** level.
+**
+** The topocentric part of the model is from Moyer (1981) and
+** Murray (1983), with fundamental arguments adapted from
+** Simon et al. 1994. It is an approximation to the expression
+** ( v / c ) . ( r / c ), where v is the barycentric velocity of
+** the Earth, r is the geocentric position of the observer and
+** c is the speed of light.
+**
+** By supplying zeroes for u and v, the topocentric part of the
+** model can be nullified, and the function will return the Fairhead
+** & Bretagnon result alone.
+**
+** 7) During the interval 1950-2050, the absolute accuracy is better
+** than +/- 3 nanoseconds relative to time ephemerides obtained by
+** direct numerical integrations based on the JPL DE405 solar system
+** ephemeris.
+**
+** 8) It must be stressed that the present function is merely a model,
+** and that numerical integration of solar-system ephemerides is the
+** definitive method for predicting the relationship between TCG and
+** TCB and hence between TT and TDB.
+**
+** References:
+**
+** Fairhead, L., & Bretagnon, P., Astron.Astrophys., 229, 240-247
+** (1990).
+**
+** IAU 2006 Resolution 3.
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Moyer, T.D., Cel.Mech., 23, 33 (1981).
+**
+** Murray, C.A., Vectorial Astrometry, Adam Hilger (1983).
+**
+** Seidelmann, P.K. et al., Explanatory Supplement to the
+** Astronomical Almanac, Chapter 2, University Science Books (1992).
+**
+** Simon, J.L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G. & Laskar, J., Astron.Astrophys., 282, 663-683 (1994).
+**
+** This revision: 2012 February 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t, tsol, w, elsun, emsun, d, elj, els, wt, w0, w1, w2, w3, w4,
+ wf, wj;
+ int j;
+
+/*
+** =====================
+** Fairhead et al. model
+** =====================
+**
+** 787 sets of three coefficients.
+**
+** Each set is
+** amplitude (microseconds)
+** frequency (radians per Julian millennium since J2000.0)
+** phase (radians)
+**
+** Sets 1-474 are the T**0 terms
+** " 475-679 " " T**1
+** " 680-764 " " T**2
+** " 765-784 " " T**3
+** " 785-787 " " T**4
+*/
+
+ static const double fairhd[787][3] = {
+ /* 1, 10 */
+ { 1656.674564e-6, 6283.075849991, 6.240054195 },
+ { 22.417471e-6, 5753.384884897, 4.296977442 },
+ { 13.839792e-6, 12566.151699983, 6.196904410 },
+ { 4.770086e-6, 529.690965095, 0.444401603 },
+ { 4.676740e-6, 6069.776754553, 4.021195093 },
+ { 2.256707e-6, 213.299095438, 5.543113262 },
+ { 1.694205e-6, -3.523118349, 5.025132748 },
+ { 1.554905e-6, 77713.771467920, 5.198467090 },
+ { 1.276839e-6, 7860.419392439, 5.988822341 },
+ { 1.193379e-6, 5223.693919802, 3.649823730 },
+ /* 11, 20 */
+ { 1.115322e-6, 3930.209696220, 1.422745069 },
+ { 0.794185e-6, 11506.769769794, 2.322313077 },
+ { 0.447061e-6, 26.298319800, 3.615796498 },
+ { 0.435206e-6, -398.149003408, 4.349338347 },
+ { 0.600309e-6, 1577.343542448, 2.678271909 },
+ { 0.496817e-6, 6208.294251424, 5.696701824 },
+ { 0.486306e-6, 5884.926846583, 0.520007179 },
+ { 0.432392e-6, 74.781598567, 2.435898309 },
+ { 0.468597e-6, 6244.942814354, 5.866398759 },
+ { 0.375510e-6, 5507.553238667, 4.103476804 },
+ /* 21, 30 */
+ { 0.243085e-6, -775.522611324, 3.651837925 },
+ { 0.173435e-6, 18849.227549974, 6.153743485 },
+ { 0.230685e-6, 5856.477659115, 4.773852582 },
+ { 0.203747e-6, 12036.460734888, 4.333987818 },
+ { 0.143935e-6, -796.298006816, 5.957517795 },
+ { 0.159080e-6, 10977.078804699, 1.890075226 },
+ { 0.119979e-6, 38.133035638, 4.551585768 },
+ { 0.118971e-6, 5486.777843175, 1.914547226 },
+ { 0.116120e-6, 1059.381930189, 0.873504123 },
+ { 0.137927e-6, 11790.629088659, 1.135934669 },
+ /* 31, 40 */
+ { 0.098358e-6, 2544.314419883, 0.092793886 },
+ { 0.101868e-6, -5573.142801634, 5.984503847 },
+ { 0.080164e-6, 206.185548437, 2.095377709 },
+ { 0.079645e-6, 4694.002954708, 2.949233637 },
+ { 0.062617e-6, 20.775395492, 2.654394814 },
+ { 0.075019e-6, 2942.463423292, 4.980931759 },
+ { 0.064397e-6, 5746.271337896, 1.280308748 },
+ { 0.063814e-6, 5760.498431898, 4.167901731 },
+ { 0.048042e-6, 2146.165416475, 1.495846011 },
+ { 0.048373e-6, 155.420399434, 2.251573730 },
+ /* 41, 50 */
+ { 0.058844e-6, 426.598190876, 4.839650148 },
+ { 0.046551e-6, -0.980321068, 0.921573539 },
+ { 0.054139e-6, 17260.154654690, 3.411091093 },
+ { 0.042411e-6, 6275.962302991, 2.869567043 },
+ { 0.040184e-6, -7.113547001, 3.565975565 },
+ { 0.036564e-6, 5088.628839767, 3.324679049 },
+ { 0.040759e-6, 12352.852604545, 3.981496998 },
+ { 0.036507e-6, 801.820931124, 6.248866009 },
+ { 0.036955e-6, 3154.687084896, 5.071801441 },
+ { 0.042732e-6, 632.783739313, 5.720622217 },
+ /* 51, 60 */
+ { 0.042560e-6, 161000.685737473, 1.270837679 },
+ { 0.040480e-6, 15720.838784878, 2.546610123 },
+ { 0.028244e-6, -6286.598968340, 5.069663519 },
+ { 0.033477e-6, 6062.663207553, 4.144987272 },
+ { 0.034867e-6, 522.577418094, 5.210064075 },
+ { 0.032438e-6, 6076.890301554, 0.749317412 },
+ { 0.030215e-6, 7084.896781115, 3.389610345 },
+ { 0.029247e-6, -71430.695617928, 4.183178762 },
+ { 0.033529e-6, 9437.762934887, 2.404714239 },
+ { 0.032423e-6, 8827.390269875, 5.541473556 },
+ /* 61, 70 */
+ { 0.027567e-6, 6279.552731642, 5.040846034 },
+ { 0.029862e-6, 12139.553509107, 1.770181024 },
+ { 0.022509e-6, 10447.387839604, 1.460726241 },
+ { 0.020937e-6, 8429.241266467, 0.652303414 },
+ { 0.020322e-6, 419.484643875, 3.735430632 },
+ { 0.024816e-6, -1194.447010225, 1.087136918 },
+ { 0.025196e-6, 1748.016413067, 2.901883301 },
+ { 0.021691e-6, 14143.495242431, 5.952658009 },
+ { 0.017673e-6, 6812.766815086, 3.186129845 },
+ { 0.022567e-6, 6133.512652857, 3.307984806 },
+ /* 71, 80 */
+ { 0.016155e-6, 10213.285546211, 1.331103168 },
+ { 0.014751e-6, 1349.867409659, 4.308933301 },
+ { 0.015949e-6, -220.412642439, 4.005298270 },
+ { 0.015974e-6, -2352.866153772, 6.145309371 },
+ { 0.014223e-6, 17789.845619785, 2.104551349 },
+ { 0.017806e-6, 73.297125859, 3.475975097 },
+ { 0.013671e-6, -536.804512095, 5.971672571 },
+ { 0.011942e-6, 8031.092263058, 2.053414715 },
+ { 0.014318e-6, 16730.463689596, 3.016058075 },
+ { 0.012462e-6, 103.092774219, 1.737438797 },
+ /* 81, 90 */
+ { 0.010962e-6, 3.590428652, 2.196567739 },
+ { 0.015078e-6, 19651.048481098, 3.969480770 },
+ { 0.010396e-6, 951.718406251, 5.717799605 },
+ { 0.011707e-6, -4705.732307544, 2.654125618 },
+ { 0.010453e-6, 5863.591206116, 1.913704550 },
+ { 0.012420e-6, 4690.479836359, 4.734090399 },
+ { 0.011847e-6, 5643.178563677, 5.489005403 },
+ { 0.008610e-6, 3340.612426700, 3.661698944 },
+ { 0.011622e-6, 5120.601145584, 4.863931876 },
+ { 0.010825e-6, 553.569402842, 0.842715011 },
+ /* 91, 100 */
+ { 0.008666e-6, -135.065080035, 3.293406547 },
+ { 0.009963e-6, 149.563197135, 4.870690598 },
+ { 0.009858e-6, 6309.374169791, 1.061816410 },
+ { 0.007959e-6, 316.391869657, 2.465042647 },
+ { 0.010099e-6, 283.859318865, 1.942176992 },
+ { 0.007147e-6, -242.728603974, 3.661486981 },
+ { 0.007505e-6, 5230.807466803, 4.920937029 },
+ { 0.008323e-6, 11769.853693166, 1.229392026 },
+ { 0.007490e-6, -6256.777530192, 3.658444681 },
+ { 0.009370e-6, 149854.400134205, 0.673880395 },
+ /* 101, 110 */
+ { 0.007117e-6, 38.027672636, 5.294249518 },
+ { 0.007857e-6, 12168.002696575, 0.525733528 },
+ { 0.007019e-6, 6206.809778716, 0.837688810 },
+ { 0.006056e-6, 955.599741609, 4.194535082 },
+ { 0.008107e-6, 13367.972631107, 3.793235253 },
+ { 0.006731e-6, 5650.292110678, 5.639906583 },
+ { 0.007332e-6, 36.648562930, 0.114858677 },
+ { 0.006366e-6, 4164.311989613, 2.262081818 },
+ { 0.006858e-6, 5216.580372801, 0.642063318 },
+ { 0.006919e-6, 6681.224853400, 6.018501522 },
+ /* 111, 120 */
+ { 0.006826e-6, 7632.943259650, 3.458654112 },
+ { 0.005308e-6, -1592.596013633, 2.500382359 },
+ { 0.005096e-6, 11371.704689758, 2.547107806 },
+ { 0.004841e-6, 5333.900241022, 0.437078094 },
+ { 0.005582e-6, 5966.683980335, 2.246174308 },
+ { 0.006304e-6, 11926.254413669, 2.512929171 },
+ { 0.006603e-6, 23581.258177318, 5.393136889 },
+ { 0.005123e-6, -1.484472708, 2.999641028 },
+ { 0.004648e-6, 1589.072895284, 1.275847090 },
+ { 0.005119e-6, 6438.496249426, 1.486539246 },
+ /* 121, 130 */
+ { 0.004521e-6, 4292.330832950, 6.140635794 },
+ { 0.005680e-6, 23013.539539587, 4.557814849 },
+ { 0.005488e-6, -3.455808046, 0.090675389 },
+ { 0.004193e-6, 7234.794256242, 4.869091389 },
+ { 0.003742e-6, 7238.675591600, 4.691976180 },
+ { 0.004148e-6, -110.206321219, 3.016173439 },
+ { 0.004553e-6, 11499.656222793, 5.554998314 },
+ { 0.004892e-6, 5436.993015240, 1.475415597 },
+ { 0.004044e-6, 4732.030627343, 1.398784824 },
+ { 0.004164e-6, 12491.370101415, 5.650931916 },
+ /* 131, 140 */
+ { 0.004349e-6, 11513.883316794, 2.181745369 },
+ { 0.003919e-6, 12528.018664345, 5.823319737 },
+ { 0.003129e-6, 6836.645252834, 0.003844094 },
+ { 0.004080e-6, -7058.598461315, 3.690360123 },
+ { 0.003270e-6, 76.266071276, 1.517189902 },
+ { 0.002954e-6, 6283.143160294, 4.447203799 },
+ { 0.002872e-6, 28.449187468, 1.158692983 },
+ { 0.002881e-6, 735.876513532, 0.349250250 },
+ { 0.003279e-6, 5849.364112115, 4.893384368 },
+ { 0.003625e-6, 6209.778724132, 1.473760578 },
+ /* 141, 150 */
+ { 0.003074e-6, 949.175608970, 5.185878737 },
+ { 0.002775e-6, 9917.696874510, 1.030026325 },
+ { 0.002646e-6, 10973.555686350, 3.918259169 },
+ { 0.002575e-6, 25132.303399966, 6.109659023 },
+ { 0.003500e-6, 263.083923373, 1.892100742 },
+ { 0.002740e-6, 18319.536584880, 4.320519510 },
+ { 0.002464e-6, 202.253395174, 4.698203059 },
+ { 0.002409e-6, 2.542797281, 5.325009315 },
+ { 0.003354e-6, -90955.551694697, 1.942656623 },
+ { 0.002296e-6, 6496.374945429, 5.061810696 },
+ /* 151, 160 */
+ { 0.003002e-6, 6172.869528772, 2.797822767 },
+ { 0.003202e-6, 27511.467873537, 0.531673101 },
+ { 0.002954e-6, -6283.008539689, 4.533471191 },
+ { 0.002353e-6, 639.897286314, 3.734548088 },
+ { 0.002401e-6, 16200.772724501, 2.605547070 },
+ { 0.003053e-6, 233141.314403759, 3.029030662 },
+ { 0.003024e-6, 83286.914269554, 2.355556099 },
+ { 0.002863e-6, 17298.182327326, 5.240963796 },
+ { 0.002103e-6, -7079.373856808, 5.756641637 },
+ { 0.002303e-6, 83996.847317911, 2.013686814 },
+ /* 161, 170 */
+ { 0.002303e-6, 18073.704938650, 1.089100410 },
+ { 0.002381e-6, 63.735898303, 0.759188178 },
+ { 0.002493e-6, 6386.168624210, 0.645026535 },
+ { 0.002366e-6, 3.932153263, 6.215885448 },
+ { 0.002169e-6, 11015.106477335, 4.845297676 },
+ { 0.002397e-6, 6243.458341645, 3.809290043 },
+ { 0.002183e-6, 1162.474704408, 6.179611691 },
+ { 0.002353e-6, 6246.427287062, 4.781719760 },
+ { 0.002199e-6, -245.831646229, 5.956152284 },
+ { 0.001729e-6, 3894.181829542, 1.264976635 },
+ /* 171, 180 */
+ { 0.001896e-6, -3128.388765096, 4.914231596 },
+ { 0.002085e-6, 35.164090221, 1.405158503 },
+ { 0.002024e-6, 14712.317116458, 2.752035928 },
+ { 0.001737e-6, 6290.189396992, 5.280820144 },
+ { 0.002229e-6, 491.557929457, 1.571007057 },
+ { 0.001602e-6, 14314.168113050, 4.203664806 },
+ { 0.002186e-6, 454.909366527, 1.402101526 },
+ { 0.001897e-6, 22483.848574493, 4.167932508 },
+ { 0.001825e-6, -3738.761430108, 0.545828785 },
+ { 0.001894e-6, 1052.268383188, 5.817167450 },
+ /* 181, 190 */
+ { 0.001421e-6, 20.355319399, 2.419886601 },
+ { 0.001408e-6, 10984.192351700, 2.732084787 },
+ { 0.001847e-6, 10873.986030480, 2.903477885 },
+ { 0.001391e-6, -8635.942003763, 0.593891500 },
+ { 0.001388e-6, -7.046236698, 1.166145902 },
+ { 0.001810e-6, -88860.057071188, 0.487355242 },
+ { 0.001288e-6, -1990.745017041, 3.913022880 },
+ { 0.001297e-6, 23543.230504682, 3.063805171 },
+ { 0.001335e-6, -266.607041722, 3.995764039 },
+ { 0.001376e-6, 10969.965257698, 5.152914309 },
+ /* 191, 200 */
+ { 0.001745e-6, 244287.600007027, 3.626395673 },
+ { 0.001649e-6, 31441.677569757, 1.952049260 },
+ { 0.001416e-6, 9225.539273283, 4.996408389 },
+ { 0.001238e-6, 4804.209275927, 5.503379738 },
+ { 0.001472e-6, 4590.910180489, 4.164913291 },
+ { 0.001169e-6, 6040.347246017, 5.841719038 },
+ { 0.001039e-6, 5540.085789459, 2.769753519 },
+ { 0.001004e-6, -170.672870619, 0.755008103 },
+ { 0.001284e-6, 10575.406682942, 5.306538209 },
+ { 0.001278e-6, 71.812653151, 4.713486491 },
+ /* 201, 210 */
+ { 0.001321e-6, 18209.330263660, 2.624866359 },
+ { 0.001297e-6, 21228.392023546, 0.382603541 },
+ { 0.000954e-6, 6282.095528923, 0.882213514 },
+ { 0.001145e-6, 6058.731054289, 1.169483931 },
+ { 0.000979e-6, 5547.199336460, 5.448375984 },
+ { 0.000987e-6, -6262.300454499, 2.656486959 },
+ { 0.001070e-6, -154717.609887482, 1.827624012 },
+ { 0.000991e-6, 4701.116501708, 4.387001801 },
+ { 0.001155e-6, -14.227094002, 3.042700750 },
+ { 0.001176e-6, 277.034993741, 3.335519004 },
+ /* 211, 220 */
+ { 0.000890e-6, 13916.019109642, 5.601498297 },
+ { 0.000884e-6, -1551.045222648, 1.088831705 },
+ { 0.000876e-6, 5017.508371365, 3.969902609 },
+ { 0.000806e-6, 15110.466119866, 5.142876744 },
+ { 0.000773e-6, -4136.910433516, 0.022067765 },
+ { 0.001077e-6, 175.166059800, 1.844913056 },
+ { 0.000954e-6, -6284.056171060, 0.968480906 },
+ { 0.000737e-6, 5326.786694021, 4.923831588 },
+ { 0.000845e-6, -433.711737877, 4.749245231 },
+ { 0.000819e-6, 8662.240323563, 5.991247817 },
+ /* 221, 230 */
+ { 0.000852e-6, 199.072001436, 2.189604979 },
+ { 0.000723e-6, 17256.631536341, 6.068719637 },
+ { 0.000940e-6, 6037.244203762, 6.197428148 },
+ { 0.000885e-6, 11712.955318231, 3.280414875 },
+ { 0.000706e-6, 12559.038152982, 2.824848947 },
+ { 0.000732e-6, 2379.164473572, 2.501813417 },
+ { 0.000764e-6, -6127.655450557, 2.236346329 },
+ { 0.000908e-6, 131.541961686, 2.521257490 },
+ { 0.000907e-6, 35371.887265976, 3.370195967 },
+ { 0.000673e-6, 1066.495477190, 3.876512374 },
+ /* 231, 240 */
+ { 0.000814e-6, 17654.780539750, 4.627122566 },
+ { 0.000630e-6, 36.027866677, 0.156368499 },
+ { 0.000798e-6, 515.463871093, 5.151962502 },
+ { 0.000798e-6, 148.078724426, 5.909225055 },
+ { 0.000806e-6, 309.278322656, 6.054064447 },
+ { 0.000607e-6, -39.617508346, 2.839021623 },
+ { 0.000601e-6, 412.371096874, 3.984225404 },
+ { 0.000646e-6, 11403.676995575, 3.852959484 },
+ { 0.000704e-6, 13521.751441591, 2.300991267 },
+ { 0.000603e-6, -65147.619767937, 4.140083146 },
+ /* 241, 250 */
+ { 0.000609e-6, 10177.257679534, 0.437122327 },
+ { 0.000631e-6, 5767.611978898, 4.026532329 },
+ { 0.000576e-6, 11087.285125918, 4.760293101 },
+ { 0.000674e-6, 14945.316173554, 6.270510511 },
+ { 0.000726e-6, 5429.879468239, 6.039606892 },
+ { 0.000710e-6, 28766.924424484, 5.672617711 },
+ { 0.000647e-6, 11856.218651625, 3.397132627 },
+ { 0.000678e-6, -5481.254918868, 6.249666675 },
+ { 0.000618e-6, 22003.914634870, 2.466427018 },
+ { 0.000738e-6, 6134.997125565, 2.242668890 },
+ /* 251, 260 */
+ { 0.000660e-6, 625.670192312, 5.864091907 },
+ { 0.000694e-6, 3496.032826134, 2.668309141 },
+ { 0.000531e-6, 6489.261398429, 1.681888780 },
+ { 0.000611e-6, -143571.324284214, 2.424978312 },
+ { 0.000575e-6, 12043.574281889, 4.216492400 },
+ { 0.000553e-6, 12416.588502848, 4.772158039 },
+ { 0.000689e-6, 4686.889407707, 6.224271088 },
+ { 0.000495e-6, 7342.457780181, 3.817285811 },
+ { 0.000567e-6, 3634.621024518, 1.649264690 },
+ { 0.000515e-6, 18635.928454536, 3.945345892 },
+ /* 261, 270 */
+ { 0.000486e-6, -323.505416657, 4.061673868 },
+ { 0.000662e-6, 25158.601719765, 1.794058369 },
+ { 0.000509e-6, 846.082834751, 3.053874588 },
+ { 0.000472e-6, -12569.674818332, 5.112133338 },
+ { 0.000461e-6, 6179.983075773, 0.513669325 },
+ { 0.000641e-6, 83467.156352816, 3.210727723 },
+ { 0.000520e-6, 10344.295065386, 2.445597761 },
+ { 0.000493e-6, 18422.629359098, 1.676939306 },
+ { 0.000478e-6, 1265.567478626, 5.487314569 },
+ { 0.000472e-6, -18.159247265, 1.999707589 },
+ /* 271, 280 */
+ { 0.000559e-6, 11190.377900137, 5.783236356 },
+ { 0.000494e-6, 9623.688276691, 3.022645053 },
+ { 0.000463e-6, 5739.157790895, 1.411223013 },
+ { 0.000432e-6, 16858.482532933, 1.179256434 },
+ { 0.000574e-6, 72140.628666286, 1.758191830 },
+ { 0.000484e-6, 17267.268201691, 3.290589143 },
+ { 0.000550e-6, 4907.302050146, 0.864024298 },
+ { 0.000399e-6, 14.977853527, 2.094441910 },
+ { 0.000491e-6, 224.344795702, 0.878372791 },
+ { 0.000432e-6, 20426.571092422, 6.003829241 },
+ /* 281, 290 */
+ { 0.000481e-6, 5749.452731634, 4.309591964 },
+ { 0.000480e-6, 5757.317038160, 1.142348571 },
+ { 0.000485e-6, 6702.560493867, 0.210580917 },
+ { 0.000426e-6, 6055.549660552, 4.274476529 },
+ { 0.000480e-6, 5959.570433334, 5.031351030 },
+ { 0.000466e-6, 12562.628581634, 4.959581597 },
+ { 0.000520e-6, 39302.096962196, 4.788002889 },
+ { 0.000458e-6, 12132.439962106, 1.880103788 },
+ { 0.000470e-6, 12029.347187887, 1.405611197 },
+ { 0.000416e-6, -7477.522860216, 1.082356330 },
+ /* 291, 300 */
+ { 0.000449e-6, 11609.862544012, 4.179989585 },
+ { 0.000465e-6, 17253.041107690, 0.353496295 },
+ { 0.000362e-6, -4535.059436924, 1.583849576 },
+ { 0.000383e-6, 21954.157609398, 3.747376371 },
+ { 0.000389e-6, 17.252277143, 1.395753179 },
+ { 0.000331e-6, 18052.929543158, 0.566790582 },
+ { 0.000430e-6, 13517.870106233, 0.685827538 },
+ { 0.000368e-6, -5756.908003246, 0.731374317 },
+ { 0.000330e-6, 10557.594160824, 3.710043680 },
+ { 0.000332e-6, 20199.094959633, 1.652901407 },
+ /* 301, 310 */
+ { 0.000384e-6, 11933.367960670, 5.827781531 },
+ { 0.000387e-6, 10454.501386605, 2.541182564 },
+ { 0.000325e-6, 15671.081759407, 2.178850542 },
+ { 0.000318e-6, 138.517496871, 2.253253037 },
+ { 0.000305e-6, 9388.005909415, 0.578340206 },
+ { 0.000352e-6, 5749.861766548, 3.000297967 },
+ { 0.000311e-6, 6915.859589305, 1.693574249 },
+ { 0.000297e-6, 24072.921469776, 1.997249392 },
+ { 0.000363e-6, -640.877607382, 5.071820966 },
+ { 0.000323e-6, 12592.450019783, 1.072262823 },
+ /* 311, 320 */
+ { 0.000341e-6, 12146.667056108, 4.700657997 },
+ { 0.000290e-6, 9779.108676125, 1.812320441 },
+ { 0.000342e-6, 6132.028180148, 4.322238614 },
+ { 0.000329e-6, 6268.848755990, 3.033827743 },
+ { 0.000374e-6, 17996.031168222, 3.388716544 },
+ { 0.000285e-6, -533.214083444, 4.687313233 },
+ { 0.000338e-6, 6065.844601290, 0.877776108 },
+ { 0.000276e-6, 24.298513841, 0.770299429 },
+ { 0.000336e-6, -2388.894020449, 5.353796034 },
+ { 0.000290e-6, 3097.883822726, 4.075291557 },
+ /* 321, 330 */
+ { 0.000318e-6, 709.933048357, 5.941207518 },
+ { 0.000271e-6, 13095.842665077, 3.208912203 },
+ { 0.000331e-6, 6073.708907816, 4.007881169 },
+ { 0.000292e-6, 742.990060533, 2.714333592 },
+ { 0.000362e-6, 29088.811415985, 3.215977013 },
+ { 0.000280e-6, 12359.966151546, 0.710872502 },
+ { 0.000267e-6, 10440.274292604, 4.730108488 },
+ { 0.000262e-6, 838.969287750, 1.327720272 },
+ { 0.000250e-6, 16496.361396202, 0.898769761 },
+ { 0.000325e-6, 20597.243963041, 0.180044365 },
+ /* 331, 340 */
+ { 0.000268e-6, 6148.010769956, 5.152666276 },
+ { 0.000284e-6, 5636.065016677, 5.655385808 },
+ { 0.000301e-6, 6080.822454817, 2.135396205 },
+ { 0.000294e-6, -377.373607916, 3.708784168 },
+ { 0.000236e-6, 2118.763860378, 1.733578756 },
+ { 0.000234e-6, 5867.523359379, 5.575209112 },
+ { 0.000268e-6, -226858.238553767, 0.069432392 },
+ { 0.000265e-6, 167283.761587465, 4.369302826 },
+ { 0.000280e-6, 28237.233459389, 5.304829118 },
+ { 0.000292e-6, 12345.739057544, 4.096094132 },
+ /* 341, 350 */
+ { 0.000223e-6, 19800.945956225, 3.069327406 },
+ { 0.000301e-6, 43232.306658416, 6.205311188 },
+ { 0.000264e-6, 18875.525869774, 1.417263408 },
+ { 0.000304e-6, -1823.175188677, 3.409035232 },
+ { 0.000301e-6, 109.945688789, 0.510922054 },
+ { 0.000260e-6, 813.550283960, 2.389438934 },
+ { 0.000299e-6, 316428.228673312, 5.384595078 },
+ { 0.000211e-6, 5756.566278634, 3.789392838 },
+ { 0.000209e-6, 5750.203491159, 1.661943545 },
+ { 0.000240e-6, 12489.885628707, 5.684549045 },
+ /* 351, 360 */
+ { 0.000216e-6, 6303.851245484, 3.862942261 },
+ { 0.000203e-6, 1581.959348283, 5.549853589 },
+ { 0.000200e-6, 5642.198242609, 1.016115785 },
+ { 0.000197e-6, -70.849445304, 4.690702525 },
+ { 0.000227e-6, 6287.008003254, 2.911891613 },
+ { 0.000197e-6, 533.623118358, 1.048982898 },
+ { 0.000205e-6, -6279.485421340, 1.829362730 },
+ { 0.000209e-6, -10988.808157535, 2.636140084 },
+ { 0.000208e-6, -227.526189440, 4.127883842 },
+ { 0.000191e-6, 415.552490612, 4.401165650 },
+ /* 361, 370 */
+ { 0.000190e-6, 29296.615389579, 4.175658539 },
+ { 0.000264e-6, 66567.485864652, 4.601102551 },
+ { 0.000256e-6, -3646.350377354, 0.506364778 },
+ { 0.000188e-6, 13119.721102825, 2.032195842 },
+ { 0.000185e-6, -209.366942175, 4.694756586 },
+ { 0.000198e-6, 25934.124331089, 3.832703118 },
+ { 0.000195e-6, 4061.219215394, 3.308463427 },
+ { 0.000234e-6, 5113.487598583, 1.716090661 },
+ { 0.000188e-6, 1478.866574064, 5.686865780 },
+ { 0.000222e-6, 11823.161639450, 1.942386641 },
+ /* 371, 380 */
+ { 0.000181e-6, 10770.893256262, 1.999482059 },
+ { 0.000171e-6, 6546.159773364, 1.182807992 },
+ { 0.000206e-6, 70.328180442, 5.934076062 },
+ { 0.000169e-6, 20995.392966449, 2.169080622 },
+ { 0.000191e-6, 10660.686935042, 5.405515999 },
+ { 0.000228e-6, 33019.021112205, 4.656985514 },
+ { 0.000184e-6, -4933.208440333, 3.327476868 },
+ { 0.000220e-6, -135.625325010, 1.765430262 },
+ { 0.000166e-6, 23141.558382925, 3.454132746 },
+ { 0.000191e-6, 6144.558353121, 5.020393445 },
+ /* 381, 390 */
+ { 0.000180e-6, 6084.003848555, 0.602182191 },
+ { 0.000163e-6, 17782.732072784, 4.960593133 },
+ { 0.000225e-6, 16460.333529525, 2.596451817 },
+ { 0.000222e-6, 5905.702242076, 3.731990323 },
+ { 0.000204e-6, 227.476132789, 5.636192701 },
+ { 0.000159e-6, 16737.577236597, 3.600691544 },
+ { 0.000200e-6, 6805.653268085, 0.868220961 },
+ { 0.000187e-6, 11919.140866668, 2.629456641 },
+ { 0.000161e-6, 127.471796607, 2.862574720 },
+ { 0.000205e-6, 6286.666278643, 1.742882331 },
+ /* 391, 400 */
+ { 0.000189e-6, 153.778810485, 4.812372643 },
+ { 0.000168e-6, 16723.350142595, 0.027860588 },
+ { 0.000149e-6, 11720.068865232, 0.659721876 },
+ { 0.000189e-6, 5237.921013804, 5.245313000 },
+ { 0.000143e-6, 6709.674040867, 4.317625647 },
+ { 0.000146e-6, 4487.817406270, 4.815297007 },
+ { 0.000144e-6, -664.756045130, 5.381366880 },
+ { 0.000175e-6, 5127.714692584, 4.728443327 },
+ { 0.000162e-6, 6254.626662524, 1.435132069 },
+ { 0.000187e-6, 47162.516354635, 1.354371923 },
+ /* 401, 410 */
+ { 0.000146e-6, 11080.171578918, 3.369695406 },
+ { 0.000180e-6, -348.924420448, 2.490902145 },
+ { 0.000148e-6, 151.047669843, 3.799109588 },
+ { 0.000157e-6, 6197.248551160, 1.284375887 },
+ { 0.000167e-6, 146.594251718, 0.759969109 },
+ { 0.000133e-6, -5331.357443741, 5.409701889 },
+ { 0.000154e-6, 95.979227218, 3.366890614 },
+ { 0.000148e-6, -6418.140930027, 3.384104996 },
+ { 0.000128e-6, -6525.804453965, 3.803419985 },
+ { 0.000130e-6, 11293.470674356, 0.939039445 },
+ /* 411, 420 */
+ { 0.000152e-6, -5729.506447149, 0.734117523 },
+ { 0.000138e-6, 210.117701700, 2.564216078 },
+ { 0.000123e-6, 6066.595360816, 4.517099537 },
+ { 0.000140e-6, 18451.078546566, 0.642049130 },
+ { 0.000126e-6, 11300.584221356, 3.485280663 },
+ { 0.000119e-6, 10027.903195729, 3.217431161 },
+ { 0.000151e-6, 4274.518310832, 4.404359108 },
+ { 0.000117e-6, 6072.958148291, 0.366324650 },
+ { 0.000165e-6, -7668.637425143, 4.298212528 },
+ { 0.000117e-6, -6245.048177356, 5.379518958 },
+ /* 421, 430 */
+ { 0.000130e-6, -5888.449964932, 4.527681115 },
+ { 0.000121e-6, -543.918059096, 6.109429504 },
+ { 0.000162e-6, 9683.594581116, 5.720092446 },
+ { 0.000141e-6, 6219.339951688, 0.679068671 },
+ { 0.000118e-6, 22743.409379516, 4.881123092 },
+ { 0.000129e-6, 1692.165669502, 0.351407289 },
+ { 0.000126e-6, 5657.405657679, 5.146592349 },
+ { 0.000114e-6, 728.762966531, 0.520791814 },
+ { 0.000120e-6, 52.596639600, 0.948516300 },
+ { 0.000115e-6, 65.220371012, 3.504914846 },
+ /* 431, 440 */
+ { 0.000126e-6, 5881.403728234, 5.577502482 },
+ { 0.000158e-6, 163096.180360983, 2.957128968 },
+ { 0.000134e-6, 12341.806904281, 2.598576764 },
+ { 0.000151e-6, 16627.370915377, 3.985702050 },
+ { 0.000109e-6, 1368.660252845, 0.014730471 },
+ { 0.000131e-6, 6211.263196841, 0.085077024 },
+ { 0.000146e-6, 5792.741760812, 0.708426604 },
+ { 0.000146e-6, -77.750543984, 3.121576600 },
+ { 0.000107e-6, 5341.013788022, 0.288231904 },
+ { 0.000138e-6, 6281.591377283, 2.797450317 },
+ /* 441, 450 */
+ { 0.000113e-6, -6277.552925684, 2.788904128 },
+ { 0.000115e-6, -525.758811831, 5.895222200 },
+ { 0.000138e-6, 6016.468808270, 6.096188999 },
+ { 0.000139e-6, 23539.707386333, 2.028195445 },
+ { 0.000146e-6, -4176.041342449, 4.660008502 },
+ { 0.000107e-6, 16062.184526117, 4.066520001 },
+ { 0.000142e-6, 83783.548222473, 2.936315115 },
+ { 0.000128e-6, 9380.959672717, 3.223844306 },
+ { 0.000135e-6, 6205.325306007, 1.638054048 },
+ { 0.000101e-6, 2699.734819318, 5.481603249 },
+ /* 451, 460 */
+ { 0.000104e-6, -568.821874027, 2.205734493 },
+ { 0.000103e-6, 6321.103522627, 2.440421099 },
+ { 0.000119e-6, 6321.208885629, 2.547496264 },
+ { 0.000138e-6, 1975.492545856, 2.314608466 },
+ { 0.000121e-6, 137.033024162, 4.539108237 },
+ { 0.000123e-6, 19402.796952817, 4.538074405 },
+ { 0.000119e-6, 22805.735565994, 2.869040566 },
+ { 0.000133e-6, 64471.991241142, 6.056405489 },
+ { 0.000129e-6, -85.827298831, 2.540635083 },
+ { 0.000131e-6, 13613.804277336, 4.005732868 },
+ /* 461, 470 */
+ { 0.000104e-6, 9814.604100291, 1.959967212 },
+ { 0.000112e-6, 16097.679950283, 3.589026260 },
+ { 0.000123e-6, 2107.034507542, 1.728627253 },
+ { 0.000121e-6, 36949.230808424, 6.072332087 },
+ { 0.000108e-6, -12539.853380183, 3.716133846 },
+ { 0.000113e-6, -7875.671863624, 2.725771122 },
+ { 0.000109e-6, 4171.425536614, 4.033338079 },
+ { 0.000101e-6, 6247.911759770, 3.441347021 },
+ { 0.000113e-6, 7330.728427345, 0.656372122 },
+ { 0.000113e-6, 51092.726050855, 2.791483066 },
+ /* 471, 480 */
+ { 0.000106e-6, 5621.842923210, 1.815323326 },
+ { 0.000101e-6, 111.430161497, 5.711033677 },
+ { 0.000103e-6, 909.818733055, 2.812745443 },
+ { 0.000101e-6, 1790.642637886, 1.965746028 },
+
+ /* T */
+ { 102.156724e-6, 6283.075849991, 4.249032005 },
+ { 1.706807e-6, 12566.151699983, 4.205904248 },
+ { 0.269668e-6, 213.299095438, 3.400290479 },
+ { 0.265919e-6, 529.690965095, 5.836047367 },
+ { 0.210568e-6, -3.523118349, 6.262738348 },
+ { 0.077996e-6, 5223.693919802, 4.670344204 },
+ /* 481, 490 */
+ { 0.054764e-6, 1577.343542448, 4.534800170 },
+ { 0.059146e-6, 26.298319800, 1.083044735 },
+ { 0.034420e-6, -398.149003408, 5.980077351 },
+ { 0.032088e-6, 18849.227549974, 4.162913471 },
+ { 0.033595e-6, 5507.553238667, 5.980162321 },
+ { 0.029198e-6, 5856.477659115, 0.623811863 },
+ { 0.027764e-6, 155.420399434, 3.745318113 },
+ { 0.025190e-6, 5746.271337896, 2.980330535 },
+ { 0.022997e-6, -796.298006816, 1.174411803 },
+ { 0.024976e-6, 5760.498431898, 2.467913690 },
+ /* 491, 500 */
+ { 0.021774e-6, 206.185548437, 3.854787540 },
+ { 0.017925e-6, -775.522611324, 1.092065955 },
+ { 0.013794e-6, 426.598190876, 2.699831988 },
+ { 0.013276e-6, 6062.663207553, 5.845801920 },
+ { 0.011774e-6, 12036.460734888, 2.292832062 },
+ { 0.012869e-6, 6076.890301554, 5.333425680 },
+ { 0.012152e-6, 1059.381930189, 6.222874454 },
+ { 0.011081e-6, -7.113547001, 5.154724984 },
+ { 0.010143e-6, 4694.002954708, 4.044013795 },
+ { 0.009357e-6, 5486.777843175, 3.416081409 },
+ /* 501, 510 */
+ { 0.010084e-6, 522.577418094, 0.749320262 },
+ { 0.008587e-6, 10977.078804699, 2.777152598 },
+ { 0.008628e-6, 6275.962302991, 4.562060226 },
+ { 0.008158e-6, -220.412642439, 5.806891533 },
+ { 0.007746e-6, 2544.314419883, 1.603197066 },
+ { 0.007670e-6, 2146.165416475, 3.000200440 },
+ { 0.007098e-6, 74.781598567, 0.443725817 },
+ { 0.006180e-6, -536.804512095, 1.302642751 },
+ { 0.005818e-6, 5088.628839767, 4.827723531 },
+ { 0.004945e-6, -6286.598968340, 0.268305170 },
+ /* 511, 520 */
+ { 0.004774e-6, 1349.867409659, 5.808636673 },
+ { 0.004687e-6, -242.728603974, 5.154890570 },
+ { 0.006089e-6, 1748.016413067, 4.403765209 },
+ { 0.005975e-6, -1194.447010225, 2.583472591 },
+ { 0.004229e-6, 951.718406251, 0.931172179 },
+ { 0.005264e-6, 553.569402842, 2.336107252 },
+ { 0.003049e-6, 5643.178563677, 1.362634430 },
+ { 0.002974e-6, 6812.766815086, 1.583012668 },
+ { 0.003403e-6, -2352.866153772, 2.552189886 },
+ { 0.003030e-6, 419.484643875, 5.286473844 },
+ /* 521, 530 */
+ { 0.003210e-6, -7.046236698, 1.863796539 },
+ { 0.003058e-6, 9437.762934887, 4.226420633 },
+ { 0.002589e-6, 12352.852604545, 1.991935820 },
+ { 0.002927e-6, 5216.580372801, 2.319951253 },
+ { 0.002425e-6, 5230.807466803, 3.084752833 },
+ { 0.002656e-6, 3154.687084896, 2.487447866 },
+ { 0.002445e-6, 10447.387839604, 2.347139160 },
+ { 0.002990e-6, 4690.479836359, 6.235872050 },
+ { 0.002890e-6, 5863.591206116, 0.095197563 },
+ { 0.002498e-6, 6438.496249426, 2.994779800 },
+ /* 531, 540 */
+ { 0.001889e-6, 8031.092263058, 3.569003717 },
+ { 0.002567e-6, 801.820931124, 3.425611498 },
+ { 0.001803e-6, -71430.695617928, 2.192295512 },
+ { 0.001782e-6, 3.932153263, 5.180433689 },
+ { 0.001694e-6, -4705.732307544, 4.641779174 },
+ { 0.001704e-6, -1592.596013633, 3.997097652 },
+ { 0.001735e-6, 5849.364112115, 0.417558428 },
+ { 0.001643e-6, 8429.241266467, 2.180619584 },
+ { 0.001680e-6, 38.133035638, 4.164529426 },
+ { 0.002045e-6, 7084.896781115, 0.526323854 },
+ /* 541, 550 */
+ { 0.001458e-6, 4292.330832950, 1.356098141 },
+ { 0.001437e-6, 20.355319399, 3.895439360 },
+ { 0.001738e-6, 6279.552731642, 0.087484036 },
+ { 0.001367e-6, 14143.495242431, 3.987576591 },
+ { 0.001344e-6, 7234.794256242, 0.090454338 },
+ { 0.001438e-6, 11499.656222793, 0.974387904 },
+ { 0.001257e-6, 6836.645252834, 1.509069366 },
+ { 0.001358e-6, 11513.883316794, 0.495572260 },
+ { 0.001628e-6, 7632.943259650, 4.968445721 },
+ { 0.001169e-6, 103.092774219, 2.838496795 },
+ /* 551, 560 */
+ { 0.001162e-6, 4164.311989613, 3.408387778 },
+ { 0.001092e-6, 6069.776754553, 3.617942651 },
+ { 0.001008e-6, 17789.845619785, 0.286350174 },
+ { 0.001008e-6, 639.897286314, 1.610762073 },
+ { 0.000918e-6, 10213.285546211, 5.532798067 },
+ { 0.001011e-6, -6256.777530192, 0.661826484 },
+ { 0.000753e-6, 16730.463689596, 3.905030235 },
+ { 0.000737e-6, 11926.254413669, 4.641956361 },
+ { 0.000694e-6, 3340.612426700, 2.111120332 },
+ { 0.000701e-6, 3894.181829542, 2.760823491 },
+ /* 561, 570 */
+ { 0.000689e-6, -135.065080035, 4.768800780 },
+ { 0.000700e-6, 13367.972631107, 5.760439898 },
+ { 0.000664e-6, 6040.347246017, 1.051215840 },
+ { 0.000654e-6, 5650.292110678, 4.911332503 },
+ { 0.000788e-6, 6681.224853400, 4.699648011 },
+ { 0.000628e-6, 5333.900241022, 5.024608847 },
+ { 0.000755e-6, -110.206321219, 4.370971253 },
+ { 0.000628e-6, 6290.189396992, 3.660478857 },
+ { 0.000635e-6, 25132.303399966, 4.121051532 },
+ { 0.000534e-6, 5966.683980335, 1.173284524 },
+ /* 571, 580 */
+ { 0.000543e-6, -433.711737877, 0.345585464 },
+ { 0.000517e-6, -1990.745017041, 5.414571768 },
+ { 0.000504e-6, 5767.611978898, 2.328281115 },
+ { 0.000485e-6, 5753.384884897, 1.685874771 },
+ { 0.000463e-6, 7860.419392439, 5.297703006 },
+ { 0.000604e-6, 515.463871093, 0.591998446 },
+ { 0.000443e-6, 12168.002696575, 4.830881244 },
+ { 0.000570e-6, 199.072001436, 3.899190272 },
+ { 0.000465e-6, 10969.965257698, 0.476681802 },
+ { 0.000424e-6, -7079.373856808, 1.112242763 },
+ /* 581, 590 */
+ { 0.000427e-6, 735.876513532, 1.994214480 },
+ { 0.000478e-6, -6127.655450557, 3.778025483 },
+ { 0.000414e-6, 10973.555686350, 5.441088327 },
+ { 0.000512e-6, 1589.072895284, 0.107123853 },
+ { 0.000378e-6, 10984.192351700, 0.915087231 },
+ { 0.000402e-6, 11371.704689758, 4.107281715 },
+ { 0.000453e-6, 9917.696874510, 1.917490952 },
+ { 0.000395e-6, 149.563197135, 2.763124165 },
+ { 0.000371e-6, 5739.157790895, 3.112111866 },
+ { 0.000350e-6, 11790.629088659, 0.440639857 },
+ /* 591, 600 */
+ { 0.000356e-6, 6133.512652857, 5.444568842 },
+ { 0.000344e-6, 412.371096874, 5.676832684 },
+ { 0.000383e-6, 955.599741609, 5.559734846 },
+ { 0.000333e-6, 6496.374945429, 0.261537984 },
+ { 0.000340e-6, 6055.549660552, 5.975534987 },
+ { 0.000334e-6, 1066.495477190, 2.335063907 },
+ { 0.000399e-6, 11506.769769794, 5.321230910 },
+ { 0.000314e-6, 18319.536584880, 2.313312404 },
+ { 0.000424e-6, 1052.268383188, 1.211961766 },
+ { 0.000307e-6, 63.735898303, 3.169551388 },
+ /* 601, 610 */
+ { 0.000329e-6, 29.821438149, 6.106912080 },
+ { 0.000357e-6, 6309.374169791, 4.223760346 },
+ { 0.000312e-6, -3738.761430108, 2.180556645 },
+ { 0.000301e-6, 309.278322656, 1.499984572 },
+ { 0.000268e-6, 12043.574281889, 2.447520648 },
+ { 0.000257e-6, 12491.370101415, 3.662331761 },
+ { 0.000290e-6, 625.670192312, 1.272834584 },
+ { 0.000256e-6, 5429.879468239, 1.913426912 },
+ { 0.000339e-6, 3496.032826134, 4.165930011 },
+ { 0.000283e-6, 3930.209696220, 4.325565754 },
+ /* 611, 620 */
+ { 0.000241e-6, 12528.018664345, 3.832324536 },
+ { 0.000304e-6, 4686.889407707, 1.612348468 },
+ { 0.000259e-6, 16200.772724501, 3.470173146 },
+ { 0.000238e-6, 12139.553509107, 1.147977842 },
+ { 0.000236e-6, 6172.869528772, 3.776271728 },
+ { 0.000296e-6, -7058.598461315, 0.460368852 },
+ { 0.000306e-6, 10575.406682942, 0.554749016 },
+ { 0.000251e-6, 17298.182327326, 0.834332510 },
+ { 0.000290e-6, 4732.030627343, 4.759564091 },
+ { 0.000261e-6, 5884.926846583, 0.298259862 },
+ /* 621, 630 */
+ { 0.000249e-6, 5547.199336460, 3.749366406 },
+ { 0.000213e-6, 11712.955318231, 5.415666119 },
+ { 0.000223e-6, 4701.116501708, 2.703203558 },
+ { 0.000268e-6, -640.877607382, 0.283670793 },
+ { 0.000209e-6, 5636.065016677, 1.238477199 },
+ { 0.000193e-6, 10177.257679534, 1.943251340 },
+ { 0.000182e-6, 6283.143160294, 2.456157599 },
+ { 0.000184e-6, -227.526189440, 5.888038582 },
+ { 0.000182e-6, -6283.008539689, 0.241332086 },
+ { 0.000228e-6, -6284.056171060, 2.657323816 },
+ /* 631, 640 */
+ { 0.000166e-6, 7238.675591600, 5.930629110 },
+ { 0.000167e-6, 3097.883822726, 5.570955333 },
+ { 0.000159e-6, -323.505416657, 5.786670700 },
+ { 0.000154e-6, -4136.910433516, 1.517805532 },
+ { 0.000176e-6, 12029.347187887, 3.139266834 },
+ { 0.000167e-6, 12132.439962106, 3.556352289 },
+ { 0.000153e-6, 202.253395174, 1.463313961 },
+ { 0.000157e-6, 17267.268201691, 1.586837396 },
+ { 0.000142e-6, 83996.847317911, 0.022670115 },
+ { 0.000152e-6, 17260.154654690, 0.708528947 },
+ /* 641, 650 */
+ { 0.000144e-6, 6084.003848555, 5.187075177 },
+ { 0.000135e-6, 5756.566278634, 1.993229262 },
+ { 0.000134e-6, 5750.203491159, 3.457197134 },
+ { 0.000144e-6, 5326.786694021, 6.066193291 },
+ { 0.000160e-6, 11015.106477335, 1.710431974 },
+ { 0.000133e-6, 3634.621024518, 2.836451652 },
+ { 0.000134e-6, 18073.704938650, 5.453106665 },
+ { 0.000134e-6, 1162.474704408, 5.326898811 },
+ { 0.000128e-6, 5642.198242609, 2.511652591 },
+ { 0.000160e-6, 632.783739313, 5.628785365 },
+ /* 651, 660 */
+ { 0.000132e-6, 13916.019109642, 0.819294053 },
+ { 0.000122e-6, 14314.168113050, 5.677408071 },
+ { 0.000125e-6, 12359.966151546, 5.251984735 },
+ { 0.000121e-6, 5749.452731634, 2.210924603 },
+ { 0.000136e-6, -245.831646229, 1.646502367 },
+ { 0.000120e-6, 5757.317038160, 3.240883049 },
+ { 0.000134e-6, 12146.667056108, 3.059480037 },
+ { 0.000137e-6, 6206.809778716, 1.867105418 },
+ { 0.000141e-6, 17253.041107690, 2.069217456 },
+ { 0.000129e-6, -7477.522860216, 2.781469314 },
+ /* 661, 670 */
+ { 0.000116e-6, 5540.085789459, 4.281176991 },
+ { 0.000116e-6, 9779.108676125, 3.320925381 },
+ { 0.000129e-6, 5237.921013804, 3.497704076 },
+ { 0.000113e-6, 5959.570433334, 0.983210840 },
+ { 0.000122e-6, 6282.095528923, 2.674938860 },
+ { 0.000140e-6, -11.045700264, 4.957936982 },
+ { 0.000108e-6, 23543.230504682, 1.390113589 },
+ { 0.000106e-6, -12569.674818332, 0.429631317 },
+ { 0.000110e-6, -266.607041722, 5.501340197 },
+ { 0.000115e-6, 12559.038152982, 4.691456618 },
+ /* 671, 680 */
+ { 0.000134e-6, -2388.894020449, 0.577313584 },
+ { 0.000109e-6, 10440.274292604, 6.218148717 },
+ { 0.000102e-6, -543.918059096, 1.477842615 },
+ { 0.000108e-6, 21228.392023546, 2.237753948 },
+ { 0.000101e-6, -4535.059436924, 3.100492232 },
+ { 0.000103e-6, 76.266071276, 5.594294322 },
+ { 0.000104e-6, 949.175608970, 5.674287810 },
+ { 0.000101e-6, 13517.870106233, 2.196632348 },
+ { 0.000100e-6, 11933.367960670, 4.056084160 },
+
+ /* T^2 */
+ { 4.322990e-6, 6283.075849991, 2.642893748 },
+ /* 681, 690 */
+ { 0.406495e-6, 0.000000000, 4.712388980 },
+ { 0.122605e-6, 12566.151699983, 2.438140634 },
+ { 0.019476e-6, 213.299095438, 1.642186981 },
+ { 0.016916e-6, 529.690965095, 4.510959344 },
+ { 0.013374e-6, -3.523118349, 1.502210314 },
+ { 0.008042e-6, 26.298319800, 0.478549024 },
+ { 0.007824e-6, 155.420399434, 5.254710405 },
+ { 0.004894e-6, 5746.271337896, 4.683210850 },
+ { 0.004875e-6, 5760.498431898, 0.759507698 },
+ { 0.004416e-6, 5223.693919802, 6.028853166 },
+ /* 691, 700 */
+ { 0.004088e-6, -7.113547001, 0.060926389 },
+ { 0.004433e-6, 77713.771467920, 3.627734103 },
+ { 0.003277e-6, 18849.227549974, 2.327912542 },
+ { 0.002703e-6, 6062.663207553, 1.271941729 },
+ { 0.003435e-6, -775.522611324, 0.747446224 },
+ { 0.002618e-6, 6076.890301554, 3.633715689 },
+ { 0.003146e-6, 206.185548437, 5.647874613 },
+ { 0.002544e-6, 1577.343542448, 6.232904270 },
+ { 0.002218e-6, -220.412642439, 1.309509946 },
+ { 0.002197e-6, 5856.477659115, 2.407212349 },
+ /* 701, 710 */
+ { 0.002897e-6, 5753.384884897, 5.863842246 },
+ { 0.001766e-6, 426.598190876, 0.754113147 },
+ { 0.001738e-6, -796.298006816, 2.714942671 },
+ { 0.001695e-6, 522.577418094, 2.629369842 },
+ { 0.001584e-6, 5507.553238667, 1.341138229 },
+ { 0.001503e-6, -242.728603974, 0.377699736 },
+ { 0.001552e-6, -536.804512095, 2.904684667 },
+ { 0.001370e-6, -398.149003408, 1.265599125 },
+ { 0.001889e-6, -5573.142801634, 4.413514859 },
+ { 0.001722e-6, 6069.776754553, 2.445966339 },
+ /* 711, 720 */
+ { 0.001124e-6, 1059.381930189, 5.041799657 },
+ { 0.001258e-6, 553.569402842, 3.849557278 },
+ { 0.000831e-6, 951.718406251, 2.471094709 },
+ { 0.000767e-6, 4694.002954708, 5.363125422 },
+ { 0.000756e-6, 1349.867409659, 1.046195744 },
+ { 0.000775e-6, -11.045700264, 0.245548001 },
+ { 0.000597e-6, 2146.165416475, 4.543268798 },
+ { 0.000568e-6, 5216.580372801, 4.178853144 },
+ { 0.000711e-6, 1748.016413067, 5.934271972 },
+ { 0.000499e-6, 12036.460734888, 0.624434410 },
+ /* 721, 730 */
+ { 0.000671e-6, -1194.447010225, 4.136047594 },
+ { 0.000488e-6, 5849.364112115, 2.209679987 },
+ { 0.000621e-6, 6438.496249426, 4.518860804 },
+ { 0.000495e-6, -6286.598968340, 1.868201275 },
+ { 0.000456e-6, 5230.807466803, 1.271231591 },
+ { 0.000451e-6, 5088.628839767, 0.084060889 },
+ { 0.000435e-6, 5643.178563677, 3.324456609 },
+ { 0.000387e-6, 10977.078804699, 4.052488477 },
+ { 0.000547e-6, 161000.685737473, 2.841633844 },
+ { 0.000522e-6, 3154.687084896, 2.171979966 },
+ /* 731, 740 */
+ { 0.000375e-6, 5486.777843175, 4.983027306 },
+ { 0.000421e-6, 5863.591206116, 4.546432249 },
+ { 0.000439e-6, 7084.896781115, 0.522967921 },
+ { 0.000309e-6, 2544.314419883, 3.172606705 },
+ { 0.000347e-6, 4690.479836359, 1.479586566 },
+ { 0.000317e-6, 801.820931124, 3.553088096 },
+ { 0.000262e-6, 419.484643875, 0.606635550 },
+ { 0.000248e-6, 6836.645252834, 3.014082064 },
+ { 0.000245e-6, -1592.596013633, 5.519526220 },
+ { 0.000225e-6, 4292.330832950, 2.877956536 },
+ /* 741, 750 */
+ { 0.000214e-6, 7234.794256242, 1.605227587 },
+ { 0.000205e-6, 5767.611978898, 0.625804796 },
+ { 0.000180e-6, 10447.387839604, 3.499954526 },
+ { 0.000229e-6, 199.072001436, 5.632304604 },
+ { 0.000214e-6, 639.897286314, 5.960227667 },
+ { 0.000175e-6, -433.711737877, 2.162417992 },
+ { 0.000209e-6, 515.463871093, 2.322150893 },
+ { 0.000173e-6, 6040.347246017, 2.556183691 },
+ { 0.000184e-6, 6309.374169791, 4.732296790 },
+ { 0.000227e-6, 149854.400134205, 5.385812217 },
+ /* 751, 760 */
+ { 0.000154e-6, 8031.092263058, 5.120720920 },
+ { 0.000151e-6, 5739.157790895, 4.815000443 },
+ { 0.000197e-6, 7632.943259650, 0.222827271 },
+ { 0.000197e-6, 74.781598567, 3.910456770 },
+ { 0.000138e-6, 6055.549660552, 1.397484253 },
+ { 0.000149e-6, -6127.655450557, 5.333727496 },
+ { 0.000137e-6, 3894.181829542, 4.281749907 },
+ { 0.000135e-6, 9437.762934887, 5.979971885 },
+ { 0.000139e-6, -2352.866153772, 4.715630782 },
+ { 0.000142e-6, 6812.766815086, 0.513330157 },
+ /* 761, 770 */
+ { 0.000120e-6, -4705.732307544, 0.194160689 },
+ { 0.000131e-6, -71430.695617928, 0.000379226 },
+ { 0.000124e-6, 6279.552731642, 2.122264908 },
+ { 0.000108e-6, -6256.777530192, 0.883445696 },
+
+ /* T^3 */
+ { 0.143388e-6, 6283.075849991, 1.131453581 },
+ { 0.006671e-6, 12566.151699983, 0.775148887 },
+ { 0.001480e-6, 155.420399434, 0.480016880 },
+ { 0.000934e-6, 213.299095438, 6.144453084 },
+ { 0.000795e-6, 529.690965095, 2.941595619 },
+ { 0.000673e-6, 5746.271337896, 0.120415406 },
+ /* 771, 780 */
+ { 0.000672e-6, 5760.498431898, 5.317009738 },
+ { 0.000389e-6, -220.412642439, 3.090323467 },
+ { 0.000373e-6, 6062.663207553, 3.003551964 },
+ { 0.000360e-6, 6076.890301554, 1.918913041 },
+ { 0.000316e-6, -21.340641002, 5.545798121 },
+ { 0.000315e-6, -242.728603974, 1.884932563 },
+ { 0.000278e-6, 206.185548437, 1.266254859 },
+ { 0.000238e-6, -536.804512095, 4.532664830 },
+ { 0.000185e-6, 522.577418094, 4.578313856 },
+ { 0.000245e-6, 18849.227549974, 0.587467082 },
+ /* 781, 787 */
+ { 0.000180e-6, 426.598190876, 5.151178553 },
+ { 0.000200e-6, 553.569402842, 5.355983739 },
+ { 0.000141e-6, 5223.693919802, 1.336556009 },
+ { 0.000104e-6, 5856.477659115, 4.239842759 },
+
+ /* T^4 */
+ { 0.003826e-6, 6283.075849991, 5.705257275 },
+ { 0.000303e-6, 12566.151699983, 5.407132842 },
+ { 0.000209e-6, 155.420399434, 1.989815753 }
+ };
+
+
+/* Time since J2000.0 in Julian millennia. */
+ t = ((date1 - DJ00) + date2) / DJM;
+
+/* ================= */
+/* Topocentric terms */
+/* ================= */
+
+/* Convert UT to local solar time in radians. */
+ tsol = fmod(ut, 1.0) * D2PI + elong;
+
+/* FUNDAMENTAL ARGUMENTS: Simon et al. 1994. */
+
+/* Combine time argument (millennia) with deg/arcsec factor. */
+ w = t / 3600.0;
+
+/* Sun Mean Longitude. */
+ elsun = fmod(280.46645683 + 1296027711.03429 * w, 360.0) * DD2R;
+
+/* Sun Mean Anomaly. */
+ emsun = fmod(357.52910918 + 1295965810.481 * w, 360.0) * DD2R;
+
+/* Mean Elongation of Moon from Sun. */
+ d = fmod(297.85019547 + 16029616012.090 * w, 360.0) * DD2R;
+
+/* Mean Longitude of Jupiter. */
+ elj = fmod(34.35151874 + 109306899.89453 * w, 360.0) * DD2R;
+
+/* Mean Longitude of Saturn. */
+ els = fmod(50.07744430 + 44046398.47038 * w, 360.0) * DD2R;
+
+/* TOPOCENTRIC TERMS: Moyer 1981 and Murray 1983. */
+ wt = + 0.00029e-10 * u * sin(tsol + elsun - els)
+ + 0.00100e-10 * u * sin(tsol - 2.0 * emsun)
+ + 0.00133e-10 * u * sin(tsol - d)
+ + 0.00133e-10 * u * sin(tsol + elsun - elj)
+ - 0.00229e-10 * u * sin(tsol + 2.0 * elsun + emsun)
+ - 0.02200e-10 * v * cos(elsun + emsun)
+ + 0.05312e-10 * u * sin(tsol - emsun)
+ - 0.13677e-10 * u * sin(tsol + 2.0 * elsun)
+ - 1.31840e-10 * v * cos(elsun)
+ + 3.17679e-10 * u * sin(tsol);
+
+/* ===================== */
+/* Fairhead et al. model */
+/* ===================== */
+
+/* T**0 */
+ w0 = 0;
+ for (j = 473; j >= 0; j--) {
+ w0 += fairhd[j][0] * sin(fairhd[j][1] * t + fairhd[j][2]);
+ }
+
+/* T**1 */
+ w1 = 0;
+ for (j = 678; j >= 474; j--) {
+ w1 += fairhd[j][0] * sin(fairhd[j][1] * t + fairhd[j][2]);
+ }
+
+/* T**2 */
+ w2 = 0;
+ for (j = 763; j >= 679; j--) {
+ w2 += fairhd[j][0] * sin(fairhd[j][1] * t + fairhd[j][2]);
+ }
+
+/* T**3 */
+ w3 = 0;
+ for (j = 783; j >= 764; j--) {
+ w3 += fairhd[j][0] * sin(fairhd[j][1] * t + fairhd[j][2]);
+ }
+
+/* T**4 */
+ w4 = 0;
+ for (j = 786; j >= 784; j--) {
+ w4 += fairhd[j][0] * sin(fairhd[j][1] * t + fairhd[j][2]);
+ }
+
+/* Multiply by powers of T and combine. */
+ wf = t * (t * (t * (t * w4 + w3) + w2) + w1) + w0;
+
+/* Adjustments to use JPL planetary masses instead of IAU. */
+ wj = 0.00065e-6 * sin(6069.776754 * t + 4.021194) +
+ 0.00033e-6 * sin( 213.299095 * t + 5.543132) +
+ (-0.00196e-6 * sin(6208.294251 * t + 5.696701)) +
+ (-0.00173e-6 * sin( 74.781599 * t + 2.435900)) +
+ 0.03638e-6 * t * t;
+
+/* ============ */
+/* Final result */
+/* ============ */
+
+/* TDB-TT in seconds. */
+ w = wt + wf + wj;
+
+ return w;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/dtf2d.c b/sofa/dtf2d.c
new file mode 100644
index 0000000..949c6cc
--- /dev/null
+++ b/sofa/dtf2d.c
@@ -0,0 +1,246 @@
+#include "sofam.h"
+#include <string.h>
+
+int iauDtf2d(const char *scale, int iy, int im, int id,
+ int ihr, int imn, double sec, double *d1, double *d2)
+/*
+** - - - - - - - - -
+** i a u D t f 2 d
+** - - - - - - - - -
+**
+** Encode date and time fields into 2-part Julian Date (or in the case
+** of UTC a quasi-JD form that includes special provision for leap
+** seconds).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** scale char[] time scale ID (Note 1)
+** iy,im,id int year, month, day in Gregorian calendar (Note 2)
+** ihr,imn int hour, minute
+** sec double seconds
+**
+** Returned:
+** d1,d2 double 2-part Julian Date (Notes 3,4)
+**
+** Returned (function value):
+** int status: +3 = both of next two
+** +2 = time is after end of day (Note 5)
+** +1 = dubious year (Note 6)
+** 0 = OK
+** -1 = bad year
+** -2 = bad month
+** -3 = bad day
+** -4 = bad hour
+** -5 = bad minute
+** -6 = bad second (<0)
+**
+** Notes:
+**
+** 1) scale identifies the time scale. Only the value "UTC" (in upper
+** case) is significant, and enables handling of leap seconds (see
+** Note 4).
+**
+** 2) For calendar conventions and limitations, see iauCal2jd.
+**
+** 3) The sum of the results, d1+d2, is Julian Date, where normally d1
+** is the Julian Day Number and d2 is the fraction of a day. In the
+** case of UTC, where the use of JD is problematical, special
+** conventions apply: see the next note.
+**
+** 4) JD cannot unambiguously represent UTC during a leap second unless
+** special measures are taken. The SOFA internal convention is that
+** the quasi-JD day represents UTC days whether the length is 86399,
+** 86400 or 86401 SI seconds.
+**
+** 5) The warning status "time is after end of day" usually means that
+** the sec argument is greater than 60.0. However, in a day ending
+** in a leap second the limit changes to 61.0 (or 59.0 in the case
+** of a negative leap second).
+**
+** 6) The warning status "dubious year" flags UTCs that predate the
+** introduction of the time scale and that are too far in the future
+** to be trusted. See iauDat for further details.
+**
+** 7) Only in the case of continuous and regular time scales (TAI, TT,
+** TCG, TCB and TDB) is the result d1+d2 a Julian Date, strictly
+** speaking. In the other cases (UT1 and UTC) the result must be
+** used with circumspection; in particular the difference between
+** two such results cannot be interpreted as a precise time
+** interval.
+**
+** Called:
+** iauCal2jd Gregorian calendar to JD
+** iauDat delta(AT) = TAI-UTC
+** iauJd2cal JD to Gregorian calendar
+**
+** This revision: 2012 February 12
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int js, iy2, im2, id2;
+ double dj, w, day, seclim, dat1, dat2, ddt, time;
+
+
+/* Today's Julian Day Number. */
+ js = iauCal2jd(iy, im, id, &dj, &w);
+ if ( js ) return js;
+ dj += w;
+
+/* Day length and final minute length in seconds (provisional). */
+ day = DAYSEC;
+ seclim = 60;
+
+/* Deal with the UTC leap second case. */
+ if ( ! strcmp(scale,"UTC") ) {
+
+ /* TAI-UTC today. */
+ js = iauDat(iy, im, id, 0.0, &dat1);
+ if ( js < 0 ) return js;
+
+ /* TAI-UTC tomorrow. */
+ js = iauJd2cal ( dj, 1.0, &iy2, &im2, &id2, &w);
+ if ( js ) return js;
+ js = iauDat(iy2, im2, id2, 0.0, &dat2);
+ if ( js < 0 ) return js;
+
+ /* The change in TAI-UTC (seconds). */
+ ddt = dat2 - dat1;
+
+ /* If leap second day, correct the day and final minute lengths. */
+ if ( fabs(ddt) > 0.5 ) {
+ day += ddt;
+ if ( ihr == 23 && imn == 59 ) seclim += ddt;
+ }
+ }
+
+/* Validate the time. */
+ if ( ihr >= 0 && ihr <= 23 ) {
+ if ( imn >= 0 && imn <= 59 ) {
+ if ( sec >= 0 ) {
+ if ( sec >= seclim ) {
+ js += 2;
+ }
+ } else {
+ js = -6;
+ }
+ } else {
+ js = -5;
+ }
+ } else {
+ js = -4;
+ }
+ if ( js < 0 ) return js;
+
+/* The time in days. */
+ time = ( 60.0 * ( (double) ( 60 * ihr + imn ) ) + sec ) / day;
+
+/* Return the date and time. */
+ *d1 = dj;
+ *d2 = time;
+
+/* Status. */
+ return js;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/ee00.c b/sofa/ee00.c
new file mode 100644
index 0000000..2bacd79
--- /dev/null
+++ b/sofa/ee00.c
@@ -0,0 +1,178 @@
+#include "sofa.h"
+
+double iauEe00(double date1, double date2, double epsa, double dpsi)
+/*
+** - - - - - - - -
+** i a u E e 0 0
+** - - - - - - - -
+**
+** The equation of the equinoxes, compatible with IAU 2000 resolutions,
+** given the nutation in longitude and the mean obliquity.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+** epsa double mean obliquity (Note 2)
+** dpsi double nutation in longitude (Note 3)
+**
+** Returned (function value):
+** double equation of the equinoxes (Note 4)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The obliquity, in radians, is mean of date.
+**
+** 3) The result, which is in radians, operates in the following sense:
+**
+** Greenwich apparent ST = GMST + equation of the equinoxes
+**
+** 4) The result is compatible with the IAU 2000 resolutions. For
+** further details, see IERS Conventions 2003 and Capitaine et al.
+** (2002).
+**
+** Called:
+** iauEect00 equation of the equinoxes complementary terms
+**
+** References:
+**
+** Capitaine, N., Wallace, P.T. and McCarthy, D.D., "Expressions to
+** implement the IAU 2000 definition of UT1", Astronomy &
+** Astrophysics, 406, 1135-1149 (2003)
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2008 May 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double ee;
+
+
+/* Equation of the equinoxes. */
+ ee = dpsi * cos(epsa) + iauEect00(date1, date2);
+
+ return ee;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/ee00a.c b/sofa/ee00a.c
new file mode 100644
index 0000000..75d4f57
--- /dev/null
+++ b/sofa/ee00a.c
@@ -0,0 +1,185 @@
+#include "sofa.h"
+
+double iauEe00a(double date1, double date2)
+/*
+** - - - - - - - - -
+** i a u E e 0 0 a
+** - - - - - - - - -
+**
+** Equation of the equinoxes, compatible with IAU 2000 resolutions.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned (function value):
+** double equation of the equinoxes (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The result, which is in radians, operates in the following sense:
+**
+** Greenwich apparent ST = GMST + equation of the equinoxes
+**
+** 3) The result is compatible with the IAU 2000 resolutions. For
+** further details, see IERS Conventions 2003 and Capitaine et al.
+** (2002).
+**
+** Called:
+** iauPr00 IAU 2000 precession adjustments
+** iauObl80 mean obliquity, IAU 1980
+** iauNut00a nutation, IAU 2000A
+** iauEe00 equation of the equinoxes, IAU 2000
+**
+** References:
+**
+** Capitaine, N., Wallace, P.T. and McCarthy, D.D., "Expressions to
+** implement the IAU 2000 definition of UT1", Astronomy &
+** Astrophysics, 406, 1135-1149 (2003).
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004).
+**
+** This revision: 2008 May 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dpsipr, depspr, epsa, dpsi, deps, ee;
+
+
+/* IAU 2000 precession-rate adjustments. */
+ iauPr00(date1, date2, &dpsipr, &depspr);
+
+/* Mean obliquity, consistent with IAU 2000 precession-nutation. */
+ epsa = iauObl80(date1, date2) + depspr;
+
+/* Nutation in longitude. */
+ iauNut00a(date1, date2, &dpsi, &deps);
+
+/* Equation of the equinoxes. */
+ ee = iauEe00(date1, date2, epsa, dpsi);
+
+ return ee;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/ee00b.c b/sofa/ee00b.c
new file mode 100644
index 0000000..cd7d485
--- /dev/null
+++ b/sofa/ee00b.c
@@ -0,0 +1,191 @@
+#include "sofa.h"
+
+double iauEe00b(double date1, double date2)
+/*
+** - - - - - - - - -
+** i a u E e 0 0 b
+** - - - - - - - - -
+**
+** Equation of the equinoxes, compatible with IAU 2000 resolutions but
+** using the truncated nutation model IAU 2000B.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned (function value):
+** double equation of the equinoxes (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The result, which is in radians, operates in the following sense:
+**
+** Greenwich apparent ST = GMST + equation of the equinoxes
+**
+** 3) The result is compatible with the IAU 2000 resolutions except
+** that accuracy has been compromised for the sake of speed. For
+** further details, see McCarthy & Luzum (2001), IERS Conventions
+** 2003 and Capitaine et al. (2003).
+**
+** Called:
+** iauPr00 IAU 2000 precession adjustments
+** iauObl80 mean obliquity, IAU 1980
+** iauNut00b nutation, IAU 2000B
+** iauEe00 equation of the equinoxes, IAU 2000
+**
+** References:
+**
+** Capitaine, N., Wallace, P.T. and McCarthy, D.D., "Expressions to
+** implement the IAU 2000 definition of UT1", Astronomy &
+** Astrophysics, 406, 1135-1149 (2003)
+**
+** McCarthy, D.D. & Luzum, B.J., "An abridged model of the
+** precession-nutation of the celestial pole", Celestial Mechanics &
+** Dynamical Astronomy, 85, 37-49 (2003)
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2008 May 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dpsipr, depspr, epsa, dpsi, deps, ee;
+
+
+/* IAU 2000 precession-rate adjustments. */
+ iauPr00(date1, date2, &dpsipr, &depspr);
+
+/* Mean obliquity, consistent with IAU 2000 precession-nutation. */
+ epsa = iauObl80(date1, date2) + depspr;
+
+/* Nutation in longitude. */
+ iauNut00b(date1, date2, &dpsi, &deps);
+
+/* Equation of the equinoxes. */
+ ee = iauEe00(date1, date2, epsa, dpsi);
+
+ return ee;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/ee06a.c b/sofa/ee06a.c
new file mode 100644
index 0000000..5cea946
--- /dev/null
+++ b/sofa/ee06a.c
@@ -0,0 +1,172 @@
+#include "sofa.h"
+
+double iauEe06a(double date1, double date2)
+/*
+** - - - - - - - - -
+** i a u E e 0 6 a
+** - - - - - - - - -
+**
+** Equation of the equinoxes, compatible with IAU 2000 resolutions and
+** IAU 2006/2000A precession-nutation.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned (function value):
+** double equation of the equinoxes (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The result, which is in radians, operates in the following sense:
+**
+** Greenwich apparent ST = GMST + equation of the equinoxes
+**
+** Called:
+** iauAnpm normalize angle into range +/- pi
+** iauGst06a Greenwich apparent sidereal time, IAU 2006/2000A
+** iauGmst06 Greenwich mean sidereal time, IAU 2006
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), 2004, IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG
+**
+** This revision: 2008 May 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double gst06a, gmst06, ee;
+
+
+/* Apparent and mean sidereal times. */
+ gst06a = iauGst06a(0.0, 0.0, date1, date2);
+ gmst06 = iauGmst06(0.0, 0.0, date1, date2);
+
+/* Equation of the equinoxes. */
+ ee = iauAnpm(gst06a - gmst06);
+
+ return ee;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/eect00.c b/sofa/eect00.c
new file mode 100644
index 0000000..2396dc5
--- /dev/null
+++ b/sofa/eect00.c
@@ -0,0 +1,332 @@
+#include "sofam.h"
+
+double iauEect00(double date1, double date2)
+/*
+** - - - - - - - - - -
+** i a u E e c t 0 0
+** - - - - - - - - - -
+**
+** Equation of the equinoxes complementary terms, consistent with
+** IAU 2000 resolutions.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned (function value):
+** double complementary terms (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The "complementary terms" are part of the equation of the
+** equinoxes (EE), classically the difference between apparent and
+** mean Sidereal Time:
+**
+** GAST = GMST + EE
+**
+** with:
+**
+** EE = dpsi * cos(eps)
+**
+** where dpsi is the nutation in longitude and eps is the obliquity
+** of date. However, if the rotation of the Earth were constant in
+** an inertial frame the classical formulation would lead to
+** apparent irregularities in the UT1 timescale traceable to side-
+** effects of precession-nutation. In order to eliminate these
+** effects from UT1, "complementary terms" were introduced in 1994
+** (IAU, 1994) and took effect from 1997 (Capitaine and Gontier,
+** 1993):
+**
+** GAST = GMST + CT + EE
+**
+** By convention, the complementary terms are included as part of
+** the equation of the equinoxes rather than as part of the mean
+** Sidereal Time. This slightly compromises the "geometrical"
+** interpretation of mean sidereal time but is otherwise
+** inconsequential.
+**
+** The present function computes CT in the above expression,
+** compatible with IAU 2000 resolutions (Capitaine et al., 2002, and
+** IERS Conventions 2003).
+**
+** Called:
+** iauFal03 mean anomaly of the Moon
+** iauFalp03 mean anomaly of the Sun
+** iauFaf03 mean argument of the latitude of the Moon
+** iauFad03 mean elongation of the Moon from the Sun
+** iauFaom03 mean longitude of the Moon's ascending node
+** iauFave03 mean longitude of Venus
+** iauFae03 mean longitude of Earth
+** iauFapa03 general accumulated precession in longitude
+**
+** References:
+**
+** Capitaine, N. & Gontier, A.-M., Astron. Astrophys., 275,
+** 645-650 (1993)
+**
+** Capitaine, N., Wallace, P.T. and McCarthy, D.D., "Expressions to
+** implement the IAU 2000 definition of UT1", Astronomy &
+** Astrophysics, 406, 1135-1149 (2003)
+**
+** IAU Resolution C7, Recommendation 3 (1994)
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Time since J2000.0, in Julian centuries */
+ double t;
+
+/* Miscellaneous */
+ int i, j;
+ double a, s0, s1;
+
+/* Fundamental arguments */
+ double fa[14];
+
+/* Returned value. */
+ double eect;
+
+/* ----------------------------------------- */
+/* The series for the EE complementary terms */
+/* ----------------------------------------- */
+
+ typedef struct {
+ int nfa[8]; /* coefficients of l,l',F,D,Om,LVe,LE,pA */
+ double s, c; /* sine and cosine coefficients */
+ } TERM;
+
+/* Terms of order t^0 */
+ static const TERM e0[] = {
+
+ /* 1-10 */
+ {{ 0, 0, 0, 0, 1, 0, 0, 0}, 2640.96e-6, -0.39e-6 },
+ {{ 0, 0, 0, 0, 2, 0, 0, 0}, 63.52e-6, -0.02e-6 },
+ {{ 0, 0, 2, -2, 3, 0, 0, 0}, 11.75e-6, 0.01e-6 },
+ {{ 0, 0, 2, -2, 1, 0, 0, 0}, 11.21e-6, 0.01e-6 },
+ {{ 0, 0, 2, -2, 2, 0, 0, 0}, -4.55e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 3, 0, 0, 0}, 2.02e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 1, 0, 0, 0}, 1.98e-6, 0.00e-6 },
+ {{ 0, 0, 0, 0, 3, 0, 0, 0}, -1.72e-6, 0.00e-6 },
+ {{ 0, 1, 0, 0, 1, 0, 0, 0}, -1.41e-6, -0.01e-6 },
+ {{ 0, 1, 0, 0, -1, 0, 0, 0}, -1.26e-6, -0.01e-6 },
+
+ /* 11-20 */
+ {{ 1, 0, 0, 0, -1, 0, 0, 0}, -0.63e-6, 0.00e-6 },
+ {{ 1, 0, 0, 0, 1, 0, 0, 0}, -0.63e-6, 0.00e-6 },
+ {{ 0, 1, 2, -2, 3, 0, 0, 0}, 0.46e-6, 0.00e-6 },
+ {{ 0, 1, 2, -2, 1, 0, 0, 0}, 0.45e-6, 0.00e-6 },
+ {{ 0, 0, 4, -4, 4, 0, 0, 0}, 0.36e-6, 0.00e-6 },
+ {{ 0, 0, 1, -1, 1, -8, 12, 0}, -0.24e-6, -0.12e-6 },
+ {{ 0, 0, 2, 0, 0, 0, 0, 0}, 0.32e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 2, 0, 0, 0}, 0.28e-6, 0.00e-6 },
+ {{ 1, 0, 2, 0, 3, 0, 0, 0}, 0.27e-6, 0.00e-6 },
+ {{ 1, 0, 2, 0, 1, 0, 0, 0}, 0.26e-6, 0.00e-6 },
+
+ /* 21-30 */
+ {{ 0, 0, 2, -2, 0, 0, 0, 0}, -0.21e-6, 0.00e-6 },
+ {{ 0, 1, -2, 2, -3, 0, 0, 0}, 0.19e-6, 0.00e-6 },
+ {{ 0, 1, -2, 2, -1, 0, 0, 0}, 0.18e-6, 0.00e-6 },
+ {{ 0, 0, 0, 0, 0, 8,-13, -1}, -0.10e-6, 0.05e-6 },
+ {{ 0, 0, 0, 2, 0, 0, 0, 0}, 0.15e-6, 0.00e-6 },
+ {{ 2, 0, -2, 0, -1, 0, 0, 0}, -0.14e-6, 0.00e-6 },
+ {{ 1, 0, 0, -2, 1, 0, 0, 0}, 0.14e-6, 0.00e-6 },
+ {{ 0, 1, 2, -2, 2, 0, 0, 0}, -0.14e-6, 0.00e-6 },
+ {{ 1, 0, 0, -2, -1, 0, 0, 0}, 0.14e-6, 0.00e-6 },
+ {{ 0, 0, 4, -2, 4, 0, 0, 0}, 0.13e-6, 0.00e-6 },
+
+ /* 31-33 */
+ {{ 0, 0, 2, -2, 4, 0, 0, 0}, -0.11e-6, 0.00e-6 },
+ {{ 1, 0, -2, 0, -3, 0, 0, 0}, 0.11e-6, 0.00e-6 },
+ {{ 1, 0, -2, 0, -1, 0, 0, 0}, 0.11e-6, 0.00e-6 }
+ };
+
+/* Terms of order t^1 */
+ static const TERM e1[] = {
+ {{ 0, 0, 0, 0, 1, 0, 0, 0}, -0.87e-6, 0.00e-6 }
+ };
+
+/* Number of terms in the series */
+ const int NE0 = (int) (sizeof e0 / sizeof (TERM));
+ const int NE1 = (int) (sizeof e1 / sizeof (TERM));
+
+/*--------------------------------------------------------------------*/
+
+/* Interval between fundamental epoch J2000.0 and current date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* Fundamental Arguments (from IERS Conventions 2003) */
+
+/* Mean anomaly of the Moon. */
+ fa[0] = iauFal03(t);
+
+/* Mean anomaly of the Sun. */
+ fa[1] = iauFalp03(t);
+
+/* Mean longitude of the Moon minus that of the ascending node. */
+ fa[2] = iauFaf03(t);
+
+/* Mean elongation of the Moon from the Sun. */
+ fa[3] = iauFad03(t);
+
+/* Mean longitude of the ascending node of the Moon. */
+ fa[4] = iauFaom03(t);
+
+/* Mean longitude of Venus. */
+ fa[5] = iauFave03(t);
+
+/* Mean longitude of Earth. */
+ fa[6] = iauFae03(t);
+
+/* General precession in longitude. */
+ fa[7] = iauFapa03(t);
+
+/* Evaluate the EE complementary terms. */
+ s0 = 0.0;
+ s1 = 0.0;
+
+ for (i = NE0-1; i >= 0; i--) {
+ a = 0.0;
+ for (j = 0; j < 8; j++) {
+ a += (double)(e0[i].nfa[j]) * fa[j];
+ }
+ s0 += e0[i].s * sin(a) + e0[i].c * cos(a);
+ }
+
+ for (i = NE1-1; i >= 0; i--) {
+ a = 0.0;
+ for (j = 0; j < 8; j++) {
+ a += (double)(e1[i].nfa[j]) * fa[j];
+ }
+ s1 += e1[i].s * sin(a) + e1[i].c * cos(a);
+ }
+
+ eect = (s0 + s1 * t ) * DAS2R;
+
+ return eect;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/eform.c b/sofa/eform.c
new file mode 100644
index 0000000..d9b25d8
--- /dev/null
+++ b/sofa/eform.c
@@ -0,0 +1,197 @@
+#include "sofam.h"
+
+int iauEform ( int n, double *a, double *f )
+/*
+** - - - - - - - - -
+** i a u E f o r m
+** - - - - - - - - -
+**
+** Earth reference ellipsoids.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** n int ellipsoid identifier (Note 1)
+**
+** Returned:
+** a double equatorial radius (meters, Note 2)
+** f double flattening (Note 2)
+**
+** Returned (function value):
+** int status: 0 = OK
+** -1 = illegal identifier (Note 3)
+**
+** Notes:
+**
+** 1) The identifier n is a number that specifies the choice of
+** reference ellipsoid. The following are supported:
+**
+** n ellipsoid
+**
+** 1 WGS84
+** 2 GRS80
+** 3 WGS72
+**
+** The n value has no significance outside the SOFA software. For
+** convenience, symbols WGS84 etc. are defined in sofam.h.
+**
+** 2) The ellipsoid parameters are returned in the form of equatorial
+** radius in meters (a) and flattening (f). The latter is a number
+** around 0.00335, i.e. around 1/298.
+**
+** 3) For the case where an unsupported n value is supplied, zero a and
+** f are returned, as well as error status.
+**
+** References:
+**
+** Department of Defense World Geodetic System 1984, National
+** Imagery and Mapping Agency Technical Report 8350.2, Third
+** Edition, p3-2.
+**
+** Moritz, H., Bull. Geodesique 66-2, 187 (1992).
+**
+** The Department of Defense World Geodetic System 1972, World
+** Geodetic System Committee, May 1974.
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992),
+** p220.
+**
+** This revision: 2012 February 23
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+
+/* Look up a and f for the specified reference ellipsoid. */
+ switch ( n ) {
+
+ case WGS84:
+ *a = 6378137.0;
+ *f = 1.0 / 298.257223563;
+ break;
+
+ case GRS80:
+ *a = 6378137.0;
+ *f = 1.0 / 298.257222101;
+ break;
+
+ case WGS72:
+ *a = 6378135.0;
+ *f = 1.0 / 298.26;
+ break;
+
+ default:
+
+ /* Invalid identifier. */
+ *a = 0.0;
+ *f = 0.0;
+ return -1;
+
+ }
+
+/* OK status. */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+
+}
diff --git a/sofa/eo06a.c b/sofa/eo06a.c
new file mode 100644
index 0000000..04cc4da
--- /dev/null
+++ b/sofa/eo06a.c
@@ -0,0 +1,181 @@
+#include "sofam.h"
+
+double iauEo06a(double date1, double date2)
+/*
+** - - - - - - - - -
+** i a u E o 0 6 a
+** - - - - - - - - -
+**
+** Equation of the origins, IAU 2006 precession and IAU 2000A nutation.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned (function value):
+** double equation of the origins in radians
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The equation of the origins is the distance between the true
+** equinox and the celestial intermediate origin and, equivalently,
+** the difference between Earth rotation angle and Greenwich
+** apparent sidereal time (ERA-GST). It comprises the precession
+** (since J2000.0) in right ascension plus the equation of the
+** equinoxes (including the small correction terms).
+**
+** Called:
+** iauPnm06a classical NPB matrix, IAU 2006/2000A
+** iauBpn2xy extract CIP X,Y coordinates from NPB matrix
+** iauS06 the CIO locator s, given X,Y, IAU 2006
+** iauEors equation of the origins, Given NPB matrix and s
+**
+** References:
+**
+** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855
+**
+** Wallace, P.T. & Capitaine, N., 2006, Astron.Astrophys. 459, 981
+**
+** This revision: 2008 May 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double r[3][3], x, y, s, eo;
+
+
+/* Classical nutation x precession x bias matrix. */
+ iauPnm06a(date1, date2, r);
+
+/* Extract CIP coordinates. */
+ iauBpn2xy(r, &x, &y);
+
+/* The CIO locator, s. */
+ s = iauS06(date1, date2, x, y);
+
+/* Solve for the EO. */
+ eo = iauEors(r, s);
+
+ return eo;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/eors.c b/sofa/eors.c
new file mode 100644
index 0000000..0c119b0
--- /dev/null
+++ b/sofa/eors.c
@@ -0,0 +1,158 @@
+#include "sofam.h"
+
+double iauEors(double rnpb[3][3], double s)
+/*
+** - - - - - - - -
+** i a u E o r s
+** - - - - - - - -
+**
+** Equation of the origins, given the classical NPB matrix and the
+** quantity s.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** rnpb double[3][3] classical nutation x precession x bias matrix
+** s double the quantity s (the CIO locator)
+**
+** Returned (function value):
+** double the equation of the origins in radians.
+**
+** Notes:
+**
+** 1) The equation of the origins is the distance between the true
+** equinox and the celestial intermediate origin and, equivalently,
+** the difference between Earth rotation angle and Greenwich
+** apparent sidereal time (ERA-GST). It comprises the precession
+** (since J2000.0) in right ascension plus the equation of the
+** equinoxes (including the small correction terms).
+**
+** 2) The algorithm is from Wallace & Capitaine (2006).
+**
+** References:
+**
+** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855
+**
+** Wallace, P. & Capitaine, N., 2006, Astron.Astrophys. 459, 981
+**
+** This revision: 2008 May 26
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double x, ax, xs, ys, zs, p, q, eo;
+
+
+/* Evaluate Wallace & Capitaine (2006) expression (16). */
+ x = rnpb[2][0];
+ ax = x / (1.0 + rnpb[2][2]);
+ xs = 1.0 - ax * x;
+ ys = -ax * rnpb[2][1];
+ zs = -x;
+ p = rnpb[0][0] * xs + rnpb[0][1] * ys + rnpb[0][2] * zs;
+ q = rnpb[1][0] * xs + rnpb[1][1] * ys + rnpb[1][2] * zs;
+ eo = ((p != 0) || (q != 0)) ? s - atan2(q, p) : s;
+
+ return eo;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/epb.c b/sofa/epb.c
new file mode 100644
index 0000000..4b1008e
--- /dev/null
+++ b/sofa/epb.c
@@ -0,0 +1,146 @@
+#include "sofam.h"
+
+double iauEpb(double dj1, double dj2)
+/*
+** - - - - - - -
+** i a u E p b
+** - - - - - - -
+**
+** Julian Date to Besselian Epoch.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** dj1,dj2 double Julian Date (see note)
+**
+** Returned (function value):
+** double Besselian Epoch.
+**
+** Note:
+**
+** The Julian Date is supplied in two pieces, in the usual SOFA
+** manner, which is designed to preserve time resolution. The
+** Julian Date is available as a single number by adding dj1 and
+** dj2. The maximum resolution is achieved if dj1 is 2451545D0
+** (J2000.0).
+**
+** Reference:
+**
+** Lieske,J.H., 1979. Astron.Astrophys.,73,282.
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* J2000.0 minus B1900.0 (2415019.81352) in Julian days */
+ static const double D1900 = 36524.68648;
+
+ double epb;
+
+
+ epb = 1900.0 + ((dj1 - DJ00) + (dj2 + D1900)) / DTY;
+
+ return epb;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/epb2jd.c b/sofa/epb2jd.c
new file mode 100644
index 0000000..e86f88b
--- /dev/null
+++ b/sofa/epb2jd.c
@@ -0,0 +1,141 @@
+#include "sofam.h"
+
+void iauEpb2jd(double epb, double *djm0, double *djm)
+/*
+** - - - - - - - - - -
+** i a u E p b 2 j d
+** - - - - - - - - - -
+**
+** Besselian Epoch to Julian Date.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** epb double Besselian Epoch (e.g. 1957.3D0)
+**
+** Returned:
+** djm0 double MJD zero-point: always 2400000.5
+** djm double Modified Julian Date
+**
+** Note:
+**
+** The Julian Date is returned in two pieces, in the usual SOFA
+** manner, which is designed to preserve time resolution. The
+** Julian Date is available as a single number by adding djm0 and
+** djm.
+**
+** Reference:
+**
+** Lieske, J.H., 1979, Astron.Astrophys. 73, 282.
+**
+** This revision: 2008 May 24
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ *djm0 = 2400000.5;
+ *djm = 15019.81352 + (epb - 1900.0) * DTY;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/epj.c b/sofa/epj.c
new file mode 100644
index 0000000..b94b201
--- /dev/null
+++ b/sofa/epj.c
@@ -0,0 +1,143 @@
+#include "sofam.h"
+
+double iauEpj(double dj1, double dj2)
+/*
+** - - - - - - -
+** i a u E p j
+** - - - - - - -
+**
+** Julian Date to Julian Epoch.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** dj1,dj2 double Julian Date (see note)
+**
+** Returned (function value):
+** double Julian Epoch
+**
+** Note:
+**
+** The Julian Date is supplied in two pieces, in the usual SOFA
+** manner, which is designed to preserve time resolution. The
+** Julian Date is available as a single number by adding dj1 and
+** dj2. The maximum resolution is achieved if dj1 is 2451545D0
+** (J2000.0).
+**
+** Reference:
+**
+** Lieske, J.H., 1979, Astron.Astrophys. 73, 282.
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double epj;
+
+
+ epj = 2000.0 + ((dj1 - DJ00) + dj2) / DJY;
+
+ return epj;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/epj2jd.c b/sofa/epj2jd.c
new file mode 100644
index 0000000..41ed251
--- /dev/null
+++ b/sofa/epj2jd.c
@@ -0,0 +1,141 @@
+#include "sofam.h"
+
+void iauEpj2jd(double epj, double *djm0, double *djm)
+/*
+** - - - - - - - - - -
+** i a u E p j 2 j d
+** - - - - - - - - - -
+**
+** Julian Epoch to Julian Date.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** epj double Julian Epoch (e.g. 1996.8D0)
+**
+** Returned:
+** djm0 double MJD zero-point: always 2400000.5
+** djm double Modified Julian Date
+**
+** Note:
+**
+** The Julian Date is returned in two pieces, in the usual SOFA
+** manner, which is designed to preserve time resolution. The
+** Julian Date is available as a single number by adding djm0 and
+** djm.
+**
+** Reference:
+**
+** Lieske, J.H., 1979, Astron.Astrophys. 73, 282.
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ *djm0 = 2400000.5;
+ *djm = 51544.5 + (epj - 2000.0) * 365.25;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/epv00.c b/sofa/epv00.c
new file mode 100644
index 0000000..df322a4
--- /dev/null
+++ b/sofa/epv00.c
@@ -0,0 +1,2639 @@
+#include "sofam.h"
+
+int iauEpv00(double date1, double date2,
+ double pvh[2][3], double pvb[2][3])
+/*
+** - - - - - - - - -
+** i a u E p v 0 0
+** - - - - - - - - -
+**
+** Earth position and velocity, heliocentric and barycentric, with
+** respect to the Barycentric Celestial Reference System.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TDB date (Note 1)
+**
+** Returned:
+** pvh double[2][3] heliocentric Earth position/velocity
+** pvb double[2][3] barycentric Earth position/velocity
+**
+** Returned (function value):
+** int status: 0 = OK
+** +1 = warning: date outside
+** the range 1900-2100 AD
+**
+** Notes:
+**
+** 1) The TDB date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TDB)=2450123.7 could be expressed in any of these ways, among
+** others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in cases
+** where the loss of several decimal digits of resolution is
+** acceptable. The J2000 method is best matched to the way the
+** argument is handled internally and will deliver the optimum
+** resolution. The MJD method and the date & time methods are both
+** good compromises between resolution and convenience. However,
+** the accuracy of the result is more likely to be limited by the
+** algorithm itself than the way the date has been expressed.
+**
+** n.b. TT can be used instead of TDB in most applications.
+**
+** 2) On return, the arrays pvh and pvb contain the following:
+**
+** pvh[0][0] x }
+** pvh[0][1] y } heliocentric position, AU
+** pvh[0][2] z }
+**
+** pvh[1][0] xdot }
+** pvh[1][1] ydot } heliocentric velocity, AU/d
+** pvh[1][2] zdot }
+**
+** pvb[0][0] x }
+** pvb[0][1] y } barycentric position, AU
+** pvb[0][2] z }
+**
+** pvb[1][0] xdot }
+** pvb[1][1] ydot } barycentric velocity, AU/d
+** pvb[1][2] zdot }
+**
+** The vectors are with respect to the Barycentric Celestial
+** Reference System. The time unit is one day in TDB.
+**
+** 3) The function is a SIMPLIFIED SOLUTION from the planetary theory
+** VSOP2000 (X. Moisson, P. Bretagnon, 2001, Celes. Mechanics &
+** Dyn. Astron., 80, 3/4, 205-213) and is an adaptation of original
+** Fortran code supplied by P. Bretagnon (private comm., 2000).
+**
+** 4) Comparisons over the time span 1900-2100 with this simplified
+** solution and the JPL DE405 ephemeris give the following results:
+**
+** RMS max
+** Heliocentric:
+** position error 3.7 11.2 km
+** velocity error 1.4 5.0 mm/s
+**
+** Barycentric:
+** position error 4.6 13.4 km
+** velocity error 1.4 4.9 mm/s
+**
+** Comparisons with the JPL DE406 ephemeris show that by 1800 and
+** 2200 the position errors are approximately double their 1900-2100
+** size. By 1500 and 2500 the deterioration is a factor of 10 and
+** by 1000 and 3000 a factor of 60. The velocity accuracy falls off
+** at about half that rate.
+**
+** 5) It is permissible to use the same array for pvh and pvb, which
+** will receive the barycentric values.
+**
+** This revision: 2008 November 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/*
+** Matrix elements for orienting the analytical model to DE405.
+**
+** The corresponding Euler angles are:
+**
+** d ' "
+** 1st rotation - 23 26 21.4091 about the x-axis (obliquity)
+** 2nd rotation + 0.0475 about the z-axis (RA offset)
+**
+** These were obtained empirically, by comparisons with DE405 over
+** 1900-2100.
+*/
+ static const double am12 = 0.000000211284,
+ am13 = -0.000000091603,
+ am21 = -0.000000230286,
+ am22 = 0.917482137087,
+ am23 = -0.397776982902,
+ am32 = 0.397776982902,
+ am33 = 0.917482137087;
+
+/*
+** ----------------------
+** Ephemeris Coefficients
+** ----------------------
+**
+** The ephemeris consists of harmonic terms for predicting (i) the Sun
+** to Earth vector and (ii) the Solar-System-barycenter to Sun vector
+** respectively. The coefficients are stored in arrays which, although
+** 1-demensional, contain groups of three. Each triplet of
+** coefficients is the amplitude, phase and frequency for one term in
+** the model, and each array contains the number of terms called for by
+** the model.
+**
+** There are eighteen such arrays, named as follows:
+**
+** array model power of T component
+**
+** e0x Sun-to-Earth 0 x
+** e0y Sun-to-Earth 0 y
+** e0z Sun-to-Earth 0 z
+**
+** e1x Sun-to-Earth 1 x
+** e1y Sun-to-Earth 1 y
+** e1z Sun-to-Earth 1 z
+**
+** e2x Sun-to-Earth 2 x
+** e2y Sun-to-Earth 2 y
+** e2z Sun-to-Earth 2 z
+**
+** s0x SSB-to-Sun 0 x
+** s0y SSB-to-Sun 0 y
+** s0z SSB-to-Sun 0 z
+**
+** s1x SSB-to-Sun 1 x
+** s1y SSB-to-Sun 1 y
+** s1z SSB-to-Sun 1 z
+**
+** s2x SSB-to-Sun 2 x
+** s2y SSB-to-Sun 2 y
+** s2z SSB-to-Sun 2 z
+*/
+
+/* Sun-to-Earth, T^0, X */
+ static const double e0x[] = {
+ 0.9998292878132e+00, 0.1753485171504e+01, 0.6283075850446e+01,
+ 0.8352579567414e-02, 0.1710344404582e+01, 0.1256615170089e+02,
+ 0.5611445335148e-02, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.1046664295572e-03, 0.1667225416770e+01, 0.1884922755134e+02,
+ 0.3110842534677e-04, 0.6687513390251e+00, 0.8399684731857e+02,
+ 0.2552413503550e-04, 0.5830637358413e+00, 0.5296909721118e+00,
+ 0.2137207845781e-04, 0.1092330954011e+01, 0.1577343543434e+01,
+ 0.1680240182951e-04, 0.4955366134987e+00, 0.6279552690824e+01,
+ 0.1679012370795e-04, 0.6153014091901e+01, 0.6286599010068e+01,
+ 0.1445526946777e-04, 0.3472744100492e+01, 0.2352866153506e+01,
+
+ 0.1091038246184e-04, 0.3689845786119e+01, 0.5223693906222e+01,
+ 0.9344399733932e-05, 0.6073934645672e+01, 0.1203646072878e+02,
+ 0.8993182910652e-05, 0.3175705249069e+01, 0.1021328554739e+02,
+ 0.5665546034116e-05, 0.2152484672246e+01, 0.1059381944224e+01,
+ 0.6844146703035e-05, 0.1306964099750e+01, 0.5753384878334e+01,
+ 0.7346610905565e-05, 0.4354980070466e+01, 0.3981490189893e+00,
+ 0.6815396474414e-05, 0.2218229211267e+01, 0.4705732307012e+01,
+ 0.6112787253053e-05, 0.5384788425458e+01, 0.6812766822558e+01,
+ 0.4518120711239e-05, 0.6087604012291e+01, 0.5884926831456e+01,
+ 0.4521963430706e-05, 0.1279424524906e+01, 0.6256777527156e+01,
+
+ 0.4497426764085e-05, 0.5369129144266e+01, 0.6309374173736e+01,
+ 0.4062190566959e-05, 0.5436473303367e+00, 0.6681224869435e+01,
+ 0.5412193480192e-05, 0.7867838528395e+00, 0.7755226100720e+00,
+ 0.5469839049386e-05, 0.1461440311134e+01, 0.1414349524433e+02,
+ 0.5205264083477e-05, 0.4432944696116e+01, 0.7860419393880e+01,
+ 0.2149759935455e-05, 0.4502237496846e+01, 0.1150676975667e+02,
+ 0.2279109618501e-05, 0.1239441308815e+01, 0.7058598460518e+01,
+ 0.2259282939683e-05, 0.3272430985331e+01, 0.4694002934110e+01,
+ 0.2558950271319e-05, 0.2265471086404e+01, 0.1216800268190e+02,
+ 0.2561581447555e-05, 0.1454740653245e+01, 0.7099330490126e+00,
+
+ 0.1781441115440e-05, 0.2962068630206e+01, 0.7962980379786e+00,
+ 0.1612005874644e-05, 0.1473255041006e+01, 0.5486777812467e+01,
+ 0.1818630667105e-05, 0.3743903293447e+00, 0.6283008715021e+01,
+ 0.1818601377529e-05, 0.6274174354554e+01, 0.6283142985870e+01,
+ 0.1554475925257e-05, 0.1624110906816e+01, 0.2513230340178e+02,
+ 0.2090948029241e-05, 0.5852052276256e+01, 0.1179062909082e+02,
+ 0.2000176345460e-05, 0.4072093298513e+01, 0.1778984560711e+02,
+ 0.1289535917759e-05, 0.5217019331069e+01, 0.7079373888424e+01,
+ 0.1281135307881e-05, 0.4802054538934e+01, 0.3738761453707e+01,
+ 0.1518229005692e-05, 0.8691914742502e+00, 0.2132990797783e+00,
+
+ 0.9450128579027e-06, 0.4601859529950e+01, 0.1097707878456e+02,
+ 0.7781119494996e-06, 0.1844352816694e+01, 0.8827390247185e+01,
+ 0.7733407759912e-06, 0.3582790154750e+01, 0.5507553240374e+01,
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+ 0.1074569126382e-08, 0.1720485636868e+01, 0.8397383534231e+02,
+
+ 0.1074408214509e-08, 0.2758613420318e+01, 0.8401985929482e+02,
+ 0.9700199670465e-09, 0.4216686842097e+01, 0.7826370942180e+02,
+ 0.1258433517061e-08, 0.2575068876639e+00, 0.3115650189215e+03,
+ 0.1240303229539e-08, 0.4800844956756e+00, 0.1784300471910e+03,
+ 0.9018345948127e-09, 0.3896756361552e+00, 0.5886454391678e+02,
+ 0.1135301432805e-08, 0.3700805023550e+00, 0.7842370451713e+02,
+ 0.9215887951370e-09, 0.4364579276638e+01, 0.1014262087719e+03,
+ 0.1055401054147e-08, 0.2156564222111e+01, 0.5660027930059e+02,
+ 0.1008725979831e-08, 0.5454015785234e+01, 0.4245678405627e+02,
+ 0.7217398104321e-09, 0.1597772562175e+01, 0.2457074661053e+03,
+
+ 0.6912033134447e-09, 0.5824090621461e+01, 0.1679936946371e+03,
+ 0.6833881523549e-09, 0.3578778482835e+01, 0.6053048899753e+02,
+ 0.4887304205142e-09, 0.3724362812423e+01, 0.9656299901946e+02,
+ 0.5173709754788e-09, 0.5422427507933e+01, 0.2442876000072e+03,
+ 0.4671353097145e-09, 0.2396106924439e+01, 0.1435713242844e+03,
+ 0.5652608439480e-09, 0.2804028838685e+01, 0.8365903305582e+02,
+ 0.5604061331253e-09, 0.1638816006247e+01, 0.8433466158131e+02,
+ 0.4712723365400e-09, 0.8979003224474e+00, 0.3164282286739e+03,
+ 0.4909967465112e-09, 0.3210426725516e+01, 0.4059982187939e+03,
+ 0.4771358267658e-09, 0.5308027211629e+01, 0.1805255418145e+03,
+
+ 0.3943451445989e-09, 0.2195145341074e+01, 0.2568537517081e+03,
+ 0.3952109120244e-09, 0.5081189491586e+01, 0.2449975330562e+03,
+ 0.3788134594789e-09, 0.4345171264441e+01, 0.1568131045107e+03,
+ 0.3738330190479e-09, 0.2613062847997e+01, 0.3948519331910e+03,
+ 0.3099866678136e-09, 0.2846760817689e+01, 0.1547176098872e+03,
+ 0.2002962716768e-09, 0.4921360989412e+01, 0.2268582385539e+03,
+ 0.2198291338754e-09, 0.1130360117454e+00, 0.1658638954901e+03,
+ 0.1491958330784e-09, 0.4228195232278e+01, 0.2219950288015e+03,
+ 0.1475384076173e-09, 0.3005721811604e+00, 0.3052819430710e+03,
+ 0.1661626624624e-09, 0.7830125621203e+00, 0.2526661704812e+03,
+
+ 0.9015823460025e-10, 0.3807792942715e+01, 0.4171445043968e+03 };
+
+/* Sun-to-Earth, T^0, Y */
+ static const double e0y[] = {
+ 0.9998921098898e+00, 0.1826583913846e+00, 0.6283075850446e+01,
+ -0.2442700893735e-01, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.8352929742915e-02, 0.1395277998680e+00, 0.1256615170089e+02,
+ 0.1046697300177e-03, 0.9641423109763e-01, 0.1884922755134e+02,
+ 0.3110841876663e-04, 0.5381140401712e+01, 0.8399684731857e+02,
+ 0.2570269094593e-04, 0.5301016407128e+01, 0.5296909721118e+00,
+ 0.2147389623610e-04, 0.2662510869850e+01, 0.1577343543434e+01,
+ 0.1680344384050e-04, 0.5207904119704e+01, 0.6279552690824e+01,
+ 0.1679117312193e-04, 0.4582187486968e+01, 0.6286599010068e+01,
+ 0.1440512068440e-04, 0.1900688517726e+01, 0.2352866153506e+01,
+
+ 0.1135139664999e-04, 0.5273108538556e+01, 0.5223693906222e+01,
+ 0.9345482571018e-05, 0.4503047687738e+01, 0.1203646072878e+02,
+ 0.9007418719568e-05, 0.1605621059637e+01, 0.1021328554739e+02,
+ 0.5671536712314e-05, 0.5812849070861e+00, 0.1059381944224e+01,
+ 0.7451401861666e-05, 0.2807346794836e+01, 0.3981490189893e+00,
+ 0.6393470057114e-05, 0.6029224133855e+01, 0.5753384878334e+01,
+ 0.6814275881697e-05, 0.6472990145974e+00, 0.4705732307012e+01,
+ 0.6113705628887e-05, 0.3813843419700e+01, 0.6812766822558e+01,
+ 0.4503851367273e-05, 0.4527804370996e+01, 0.5884926831456e+01,
+ 0.4522249141926e-05, 0.5991783029224e+01, 0.6256777527156e+01,
+
+ 0.4501794307018e-05, 0.3798703844397e+01, 0.6309374173736e+01,
+ 0.5514927480180e-05, 0.3961257833388e+01, 0.5507553240374e+01,
+ 0.4062862799995e-05, 0.5256247296369e+01, 0.6681224869435e+01,
+ 0.5414900429712e-05, 0.5499032014097e+01, 0.7755226100720e+00,
+ 0.5463153987424e-05, 0.6173092454097e+01, 0.1414349524433e+02,
+ 0.5071611859329e-05, 0.2870244247651e+01, 0.7860419393880e+01,
+ 0.2195112094455e-05, 0.2952338617201e+01, 0.1150676975667e+02,
+ 0.2279139233919e-05, 0.5951775132933e+01, 0.7058598460518e+01,
+ 0.2278386100876e-05, 0.4845456398785e+01, 0.4694002934110e+01,
+ 0.2559088003308e-05, 0.6945321117311e+00, 0.1216800268190e+02,
+
+ 0.2561079286856e-05, 0.6167224608301e+01, 0.7099330490126e+00,
+ 0.1792755796387e-05, 0.1400122509632e+01, 0.7962980379786e+00,
+ 0.1818715656502e-05, 0.4703347611830e+01, 0.6283142985870e+01,
+ 0.1818744924791e-05, 0.5086748900237e+01, 0.6283008715021e+01,
+ 0.1554518791390e-05, 0.5331008042713e-01, 0.2513230340178e+02,
+ 0.2063265737239e-05, 0.4283680484178e+01, 0.1179062909082e+02,
+ 0.1497613520041e-05, 0.6074207826073e+01, 0.5486777812467e+01,
+ 0.2000617940427e-05, 0.2501426281450e+01, 0.1778984560711e+02,
+ 0.1289731195580e-05, 0.3646340599536e+01, 0.7079373888424e+01,
+ 0.1282657998934e-05, 0.3232864804902e+01, 0.3738761453707e+01,
+
+ 0.1528915968658e-05, 0.5581433416669e+01, 0.2132990797783e+00,
+ 0.1187304098432e-05, 0.5453576453694e+01, 0.9437762937313e+01,
+ 0.7842782928118e-06, 0.2823953922273e+00, 0.8827390247185e+01,
+ 0.7352892280868e-06, 0.1124369580175e+01, 0.1589072916335e+01,
+ 0.6570189360797e-06, 0.2089154042840e+01, 0.1176985366291e+02,
+ 0.6324967590410e-06, 0.6704855581230e+00, 0.6262300422539e+01,
+ 0.6298289872283e-06, 0.2836414855840e+01, 0.6303851278352e+01,
+ 0.6476686465855e-06, 0.4852433866467e+00, 0.7113454667900e-02,
+ 0.8587034651234e-06, 0.1453511005668e+01, 0.1672837615881e+03,
+ 0.8068948788113e-06, 0.9224087798609e+00, 0.6069776770667e+01,
+
+ 0.8353786011661e-06, 0.4631707184895e+01, 0.3340612434717e+01,
+ 0.6009324532132e-06, 0.1829498827726e+01, 0.4136910472696e+01,
+ 0.7558158559566e-06, 0.2588596800317e+01, 0.6496374930224e+01,
+ 0.5809279504503e-06, 0.5516818853476e+00, 0.1097707878456e+02,
+ 0.5374131950254e-06, 0.6275674734960e+01, 0.1194447056968e+01,
+ 0.5711160507326e-06, 0.1091905956872e+01, 0.6282095334605e+01,
+ 0.5710183170746e-06, 0.2415001635090e+01, 0.6284056366286e+01,
+ 0.5144373590610e-06, 0.6020336443438e+01, 0.6290189305114e+01,
+ 0.5103108927267e-06, 0.3775634564605e+01, 0.6275962395778e+01,
+ 0.4960654697891e-06, 0.1073450946756e+01, 0.6127655567643e+01,
+
+ 0.4786385689280e-06, 0.2431178012310e+01, 0.6438496133249e+01,
+ 0.6109911263665e-06, 0.5343356157914e+01, 0.3154687086868e+01,
+ 0.4839898944024e-06, 0.5830833594047e-01, 0.8018209333619e+00,
+ 0.4734822623919e-06, 0.4536080134821e+01, 0.3128388763578e+01,
+ 0.4834741473290e-06, 0.2585090489754e+00, 0.7084896783808e+01,
+ 0.5134858581156e-06, 0.4213317172603e+01, 0.1235285262111e+02,
+ 0.5064004264978e-06, 0.4814418806478e+00, 0.1185621865188e+02,
+ 0.3753476772761e-06, 0.1599953399788e+01, 0.8429241228195e+01,
+ 0.4935264014283e-06, 0.2157417556873e+01, 0.2544314396739e+01,
+ 0.3950929600897e-06, 0.3359394184254e+01, 0.5481254917084e+01,
+
+ 0.4895849789777e-06, 0.5165704376558e+01, 0.9225539266174e+01,
+ 0.4215241688886e-06, 0.2065368800993e+01, 0.1726015463500e+02,
+ 0.3796773731132e-06, 0.1468606346612e+01, 0.4265981595566e+00,
+ 0.3114178142515e-06, 0.3615638079474e+01, 0.2146165377750e+01,
+ 0.3260664220838e-06, 0.4417134922435e+01, 0.4164311961999e+01,
+ 0.3976996123008e-06, 0.4700866883004e+01, 0.5856477690889e+01,
+ 0.2801459672924e-06, 0.4538902060922e+01, 0.1256967486051e+02,
+ 0.3638931868861e-06, 0.1334197991475e+01, 0.1807370494127e+02,
+ 0.2487013269476e-06, 0.3749275558275e+01, 0.2629832328990e-01,
+ 0.3034165481994e-06, 0.4236622030873e+00, 0.4535059491685e+01,
+
+ 0.2676278825586e-06, 0.5970848007811e+01, 0.3930209696940e+01,
+ 0.2764903818918e-06, 0.5194636754501e+01, 0.1256262854127e+02,
+ 0.2485149930507e-06, 0.1002434207846e+01, 0.5088628793478e+01,
+ 0.2199305540941e-06, 0.3066773098403e+01, 0.1255903824622e+02,
+ 0.2571106500435e-06, 0.7588312459063e+00, 0.1336797263425e+02,
+ 0.2049751817158e-06, 0.3444977434856e+01, 0.1137170464392e+02,
+ 0.2599707296297e-06, 0.1873128542205e+01, 0.7143069561767e+02,
+ 0.1785018072217e-06, 0.5015891306615e+01, 0.1748016358760e+01,
+ 0.2324833891115e-06, 0.4618271239730e+01, 0.1831953657923e+02,
+ 0.1709711119545e-06, 0.5300003455669e+01, 0.4933208510675e+01,
+
+ 0.2107159351716e-06, 0.2229819815115e+01, 0.7477522907414e+01,
+ 0.1750333080295e-06, 0.6161485880008e+01, 0.1044738781244e+02,
+ 0.2000598210339e-06, 0.2967357299999e+01, 0.8031092209206e+01,
+ 0.1380920248681e-06, 0.3027007923917e+01, 0.8635942003952e+01,
+ 0.1412460470299e-06, 0.6037597163798e+01, 0.2942463415728e+01,
+ 0.1888459803001e-06, 0.8561476243374e+00, 0.1561374759853e+03,
+ 0.1788370542585e-06, 0.4869736290209e+01, 0.1592596075957e+01,
+ 0.1360893296167e-06, 0.3626411886436e+01, 0.1309584267300e+02,
+ 0.1506846530160e-06, 0.1550975377427e+01, 0.1649636139783e+02,
+ 0.1800913376176e-06, 0.2075826033190e+01, 0.1729818233119e+02,
+
+ 0.1436261390649e-06, 0.6148876420255e+01, 0.2042657109477e+02,
+ 0.1220227114151e-06, 0.4382583879906e+01, 0.7632943190217e+01,
+ 0.1337883603592e-06, 0.2036644327361e+01, 0.1213955354133e+02,
+ 0.1159326650738e-06, 0.3892276994687e+01, 0.5331357529664e+01,
+ 0.1352853128569e-06, 0.1447950649744e+01, 0.1673046366289e+02,
+ 0.1433408296083e-06, 0.4457854692961e+01, 0.7342457794669e+01,
+ 0.1234701666518e-06, 0.1538818147151e+01, 0.6279485555400e+01,
+ 0.1234027192007e-06, 0.1968523220760e+01, 0.6286666145492e+01,
+ 0.1244024091797e-06, 0.5779803499985e+01, 0.1511046609763e+02,
+ 0.1097934945516e-06, 0.6210975221388e+00, 0.1098880815746e+02,
+
+ 0.1254611329856e-06, 0.2591963807998e+01, 0.1572083878776e+02,
+ 0.1158247286784e-06, 0.2483612812670e+01, 0.5729506548653e+01,
+ 0.9039078252960e-07, 0.3857554579796e+01, 0.9623688285163e+01,
+ 0.9108024978836e-07, 0.5826368512984e+01, 0.7234794171227e+01,
+ 0.8887068108436e-07, 0.3475694573987e+01, 0.6148010737701e+01,
+ 0.8632374035438e-07, 0.3059070488983e-01, 0.6418140963190e+01,
+ 0.7893186992967e-07, 0.1583194837728e+01, 0.2118763888447e+01,
+ 0.8297650201172e-07, 0.8519770534637e+00, 0.1471231707864e+02,
+ 0.1019759578988e-06, 0.1319598738732e+00, 0.1349867339771e+01,
+ 0.1010037696236e-06, 0.9937860115618e+00, 0.6836645152238e+01,
+
+ 0.1047727548266e-06, 0.1382138405399e+01, 0.5999216516294e+01,
+ 0.7351993881086e-07, 0.3833397851735e+01, 0.6040347114260e+01,
+ 0.9868771092341e-07, 0.2124913814390e+01, 0.6566935184597e+01,
+ 0.7007321959390e-07, 0.5946305343763e+01, 0.6525804586632e+01,
+ 0.6861411679709e-07, 0.4574654977089e+01, 0.7238675589263e+01,
+ 0.7554519809614e-07, 0.5949232686844e+01, 0.1253985337760e+02,
+ 0.9541880448335e-07, 0.3495242990564e+01, 0.2122839202813e+02,
+ 0.7185606722155e-07, 0.4310113471661e+01, 0.6245048154254e+01,
+ 0.7131360871710e-07, 0.5480309323650e+01, 0.6321103546637e+01,
+ 0.6651142021039e-07, 0.5411097713654e+01, 0.5327476111629e+01,
+
+ 0.8538618213667e-07, 0.1827849973951e+01, 0.1101510648075e+02,
+ 0.8634954288044e-07, 0.5443584943349e+01, 0.5643178611111e+01,
+ 0.7449415051484e-07, 0.2011535459060e+01, 0.5368044267797e+00,
+ 0.7421047599169e-07, 0.3464562529249e+01, 0.2354323048545e+02,
+ 0.6140694354424e-07, 0.5657556228815e+01, 0.1296430071988e+02,
+ 0.6353525143033e-07, 0.3463816593821e+01, 0.1990745094947e+01,
+ 0.6221964013447e-07, 0.1532259498697e+01, 0.9517183207817e+00,
+ 0.5852480257244e-07, 0.1375396598875e+01, 0.9555997388169e+00,
+ 0.6398637498911e-07, 0.2405645801972e+01, 0.2407292145756e+02,
+ 0.7039744069878e-07, 0.5397541799027e+01, 0.5225775174439e+00,
+
+ 0.6977997694382e-07, 0.4762347105419e+01, 0.1097355562493e+02,
+ 0.7460629558396e-07, 0.2711944692164e+01, 0.2200391463820e+02,
+ 0.5376577536101e-07, 0.2352980430239e+01, 0.1431416805965e+02,
+ 0.7530607893556e-07, 0.1943940180699e+01, 0.1842262939178e+02,
+ 0.6822928971605e-07, 0.4337651846959e+01, 0.1554202828031e+00,
+ 0.6220772380094e-07, 0.6716871369278e+00, 0.1845107853235e+02,
+ 0.6586950799043e-07, 0.2229714460505e+01, 0.5216580451554e+01,
+ 0.5873800565771e-07, 0.7627013920580e+00, 0.6398972393349e+00,
+ 0.6264346929745e-07, 0.6202785478961e+00, 0.6277552955062e+01,
+ 0.6257929115669e-07, 0.2886775596668e+01, 0.6288598745829e+01,
+
+ 0.5343536033409e-07, 0.1977241012051e+01, 0.4690479774488e+01,
+ 0.5587849781714e-07, 0.1922923484825e+01, 0.1551045220144e+01,
+ 0.6905100845603e-07, 0.3570757164631e+01, 0.1030928125552e+00,
+ 0.6178957066649e-07, 0.5197558947765e+01, 0.5230807360890e+01,
+ 0.6187270224331e-07, 0.8193497368922e+00, 0.5650292065779e+01,
+ 0.5385664291426e-07, 0.5406336665586e+01, 0.7771377146812e+02,
+ 0.6329363917926e-07, 0.2837760654536e+01, 0.2608790314060e+02,
+ 0.4546018761604e-07, 0.2933580297050e+01, 0.5535693017924e+00,
+ 0.6196091049375e-07, 0.4157871494377e+01, 0.8467247584405e+02,
+ 0.6159555108218e-07, 0.3211703561703e+01, 0.2394243902548e+03,
+
+ 0.4995340539317e-07, 0.1459098102922e+01, 0.4732030630302e+01,
+ 0.5457031243572e-07, 0.1430457676136e+01, 0.6179983037890e+01,
+ 0.4863461418397e-07, 0.2196425916730e+01, 0.9027992316901e+02,
+ 0.5342947626870e-07, 0.2086612890268e+01, 0.6386168663001e+01,
+ 0.5674296648439e-07, 0.2760204966535e+01, 0.6915859635113e+01,
+ 0.4745783120161e-07, 0.4245368971862e+01, 0.6282970628506e+01,
+ 0.4745676961198e-07, 0.5544725787016e+01, 0.6283181072386e+01,
+ 0.4049796869973e-07, 0.2213984363586e+01, 0.6254626709878e+01,
+ 0.4248333596940e-07, 0.8075781952896e+00, 0.7875671926403e+01,
+ 0.4027178070205e-07, 0.1293268540378e+01, 0.6311524991013e+01,
+
+ 0.4066543943476e-07, 0.3986141175804e+01, 0.3634620989887e+01,
+ 0.4858863787880e-07, 0.1276112738231e+01, 0.5760498333002e+01,
+ 0.5277398263530e-07, 0.4916111741527e+01, 0.2515860172507e+02,
+ 0.4105635656559e-07, 0.1725805864426e+01, 0.6709674010002e+01,
+ 0.4376781925772e-07, 0.2243642442106e+01, 0.6805653367890e+01,
+ 0.3235827894693e-07, 0.3614135118271e+01, 0.1066495398892e+01,
+ 0.3073244740308e-07, 0.2460873393460e+01, 0.5863591145557e+01,
+ 0.3088609271373e-07, 0.5678431771790e+01, 0.9917696840332e+01,
+ 0.3393022279836e-07, 0.3814017477291e+01, 0.1391601904066e+02,
+ 0.3038686508802e-07, 0.4660216229171e+01, 0.1256621883632e+02,
+
+ 0.4019677752497e-07, 0.5906906243735e+01, 0.1334167431096e+02,
+ 0.3288834998232e-07, 0.9536146445882e+00, 0.1620077269078e+02,
+ 0.3889973794631e-07, 0.3942205097644e+01, 0.7478166569050e-01,
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+ 0.3514010952384e-08, 0.2699961831678e+01, 0.7335344340001e+01,
+ 0.3327607571530e-08, 0.3318457714816e+01, 0.5436992986000e+01,
+ 0.3541066946675e-08, 0.4382703582466e+01, 0.1234573916645e+02,
+ 0.3216179847052e-08, 0.5271066317054e+01, 0.3802769619140e-01,
+ 0.2959045059570e-08, 0.5819591585302e+01, 0.2670964694522e+02,
+ 0.3884040326665e-08, 0.5980934960428e+01, 0.6660449441528e+01,
+
+ 0.2922027539886e-08, 0.3337290282483e+01, 0.1375773836557e+01,
+ 0.4110846382042e-08, 0.5742978187327e+01, 0.4480965020977e+02,
+ 0.2934508411032e-08, 0.2278075804200e+01, 0.6408777551755e+00,
+ 0.3966896193000e-08, 0.5835747858477e+01, 0.3773735910827e+00,
+ 0.3286695827610e-08, 0.5838898193902e+01, 0.3932462625300e-02,
+ 0.3720643094196e-08, 0.1122212337858e+01, 0.1646033343740e+02,
+ 0.3285508906174e-08, 0.9182250996416e+00, 0.1081813534213e+02,
+ 0.3753880575973e-08, 0.5174761973266e+01, 0.5642198095270e+01,
+ 0.3022129385587e-08, 0.3381611020639e+01, 0.2982630633589e+02,
+ 0.2798569205621e-08, 0.3546193723922e+01, 0.1937891852345e+02,
+
+ 0.3397872070505e-08, 0.4533203197934e+01, 0.6923953605621e+01,
+ 0.3708099772977e-08, 0.2756168198616e+01, 0.3066615496545e+02,
+ 0.3599283541510e-08, 0.1934395469918e+01, 0.6147450479709e+01,
+ 0.3688702753059e-08, 0.7149920971109e+00, 0.2636725487657e+01,
+ 0.2681084724003e-08, 0.4899819493154e+01, 0.6816289982179e+01,
+ 0.3495993460759e-08, 0.1572418915115e+01, 0.6418701221183e+01,
+ 0.3130770324995e-08, 0.8912190180489e+00, 0.1235996607578e+02,
+ 0.2744353821941e-08, 0.3800821940055e+01, 0.2059724391010e+02,
+ 0.2842732906341e-08, 0.2644717440029e+01, 0.2828699048865e+02,
+ 0.3046882682154e-08, 0.3987793020179e+01, 0.6055599646783e+01,
+
+ 0.2399072455143e-08, 0.9908826440764e+00, 0.6255674361143e+01,
+ 0.2384306274204e-08, 0.2516149752220e+01, 0.6310477339748e+01,
+ 0.2977324500559e-08, 0.5849195642118e+01, 0.1652265972112e+02,
+ 0.3062835258972e-08, 0.1681660100162e+01, 0.1172006883645e+02,
+ 0.3109682589231e-08, 0.5804143987737e+00, 0.2751146787858e+02,
+ 0.2903920355299e-08, 0.5800768280123e+01, 0.6510552054109e+01,
+ 0.2823221989212e-08, 0.9241118370216e+00, 0.5469525544182e+01,
+ 0.3187949696649e-08, 0.3139776445735e+01, 0.1693792562116e+03,
+ 0.2922559771655e-08, 0.3549440782984e+01, 0.2630839062450e+00,
+ 0.2436302066603e-08, 0.4735540696319e+01, 0.3946258593675e+00,
+
+ 0.3049473043606e-08, 0.4998289124561e+01, 0.8390110365991e+01,
+ 0.2863682575784e-08, 0.6709515671102e+00, 0.2243449970715e+00,
+ 0.2641750517966e-08, 0.5410978257284e+01, 0.2986433403208e+02,
+ 0.2704093466243e-08, 0.4778317207821e+01, 0.6129297044991e+01,
+ 0.2445522177011e-08, 0.6009020662222e+01, 0.1171295538178e+02,
+ 0.2623608810230e-08, 0.5010449777147e+01, 0.6436854655901e+01,
+ 0.2079259704053e-08, 0.5980943768809e+01, 0.2019909489111e+02,
+ 0.2820225596771e-08, 0.2679965110468e+01, 0.5934151399930e+01,
+ 0.2365221950927e-08, 0.1894231148810e+01, 0.2470570524223e+02,
+ 0.2359682077149e-08, 0.4220752950780e+01, 0.8671969964381e+01,
+
+ 0.2387577137206e-08, 0.2571783940617e+01, 0.7096626156709e+01,
+ 0.1982102089816e-08, 0.5169765997119e+00, 0.1727188400790e+02,
+ 0.2687502389925e-08, 0.6239078264579e+01, 0.7075506709219e+02,
+ 0.2207751669135e-08, 0.2031184412677e+01, 0.4377611041777e+01,
+ 0.2618370214274e-08, 0.8266079985979e+00, 0.6632000300961e+01,
+ 0.2591951887361e-08, 0.8819350522008e+00, 0.4873985990671e+02,
+ 0.2375055656248e-08, 0.3520944177789e+01, 0.1590676413561e+02,
+ 0.2472019978911e-08, 0.1551431908671e+01, 0.6612329252343e+00,
+ 0.2368157127199e-08, 0.4178610147412e+01, 0.3459636466239e+02,
+ 0.1764846605693e-08, 0.1506764000157e+01, 0.1980094587212e+02,
+
+ 0.2291769608798e-08, 0.2118250611782e+01, 0.2844914056730e-01,
+ 0.2209997316943e-08, 0.3363255261678e+01, 0.2666070658668e+00,
+ 0.2292699097923e-08, 0.4200423956460e+00, 0.1484170571900e-02,
+ 0.1629683015329e-08, 0.2331362582487e+01, 0.3035599730800e+02,
+ 0.2206492862426e-08, 0.3400274026992e+01, 0.6281667977667e+01,
+ 0.2205746568257e-08, 0.1066051230724e+00, 0.6284483723224e+01,
+ 0.2026310767991e-08, 0.2779066487979e+01, 0.2449240616245e+02,
+ 0.1762977622163e-08, 0.9951450691840e+00, 0.2045286941806e+02,
+ 0.1368535049606e-08, 0.6402447365817e+00, 0.2473415438279e+02,
+ 0.1720598775450e-08, 0.2303524214705e+00, 0.1679593901136e+03,
+
+ 0.1702429015449e-08, 0.6164622655048e+01, 0.3338575901272e+03,
+ 0.1414033197685e-08, 0.3954561185580e+01, 0.1624205518357e+03,
+ 0.1573768958043e-08, 0.2028286308984e+01, 0.3144167757552e+02,
+ 0.1650705184447e-08, 0.2304040666128e+01, 0.5267006960365e+02,
+ 0.1651087618855e-08, 0.2538461057280e+01, 0.8956999012000e+02,
+ 0.1616409518983e-08, 0.5111054348152e+01, 0.3332657872986e+02,
+ 0.1537175173581e-08, 0.5601130666603e+01, 0.3852657435933e+02,
+ 0.1593191980553e-08, 0.2614340453411e+01, 0.2282781046519e+03,
+ 0.1499480170643e-08, 0.3624721577264e+01, 0.2823723341956e+02,
+ 0.1493807843235e-08, 0.4214569879008e+01, 0.2876692439167e+02,
+
+ 0.1074571199328e-08, 0.1496911744704e+00, 0.8397383534231e+02,
+ 0.1074406983417e-08, 0.1187817671922e+01, 0.8401985929482e+02,
+ 0.9757576855851e-09, 0.2655703035858e+01, 0.7826370942180e+02,
+ 0.1258432887565e-08, 0.4969896184844e+01, 0.3115650189215e+03,
+ 0.1240336343282e-08, 0.5192460776926e+01, 0.1784300471910e+03,
+ 0.9016107005164e-09, 0.1960356923057e+01, 0.5886454391678e+02,
+ 0.1135392360918e-08, 0.5082427809068e+01, 0.7842370451713e+02,
+ 0.9216046089565e-09, 0.2793775037273e+01, 0.1014262087719e+03,
+ 0.1061276615030e-08, 0.3726144311409e+01, 0.5660027930059e+02,
+ 0.1010110596263e-08, 0.7404080708937e+00, 0.4245678405627e+02,
+
+ 0.7217424756199e-09, 0.2697449980577e-01, 0.2457074661053e+03,
+ 0.6912003846756e-09, 0.4253296276335e+01, 0.1679936946371e+03,
+ 0.6871814664847e-09, 0.5148072412354e+01, 0.6053048899753e+02,
+ 0.4887158016343e-09, 0.2153581148294e+01, 0.9656299901946e+02,
+ 0.5161802866314e-09, 0.3852750634351e+01, 0.2442876000072e+03,
+ 0.5652599559057e-09, 0.1233233356270e+01, 0.8365903305582e+02,
+ 0.4710812608586e-09, 0.5610486976767e+01, 0.3164282286739e+03,
+ 0.4909977500324e-09, 0.1639629524123e+01, 0.4059982187939e+03,
+ 0.4772641839378e-09, 0.3737100368583e+01, 0.1805255418145e+03,
+ 0.4487562567153e-09, 0.1158417054478e+00, 0.8433466158131e+02,
+
+ 0.3943441230497e-09, 0.6243502862796e+00, 0.2568537517081e+03,
+ 0.3952236913598e-09, 0.3510377382385e+01, 0.2449975330562e+03,
+ 0.3788898363417e-09, 0.5916128302299e+01, 0.1568131045107e+03,
+ 0.3738329328831e-09, 0.1042266763456e+01, 0.3948519331910e+03,
+ 0.2451199165151e-09, 0.1166788435700e+01, 0.1435713242844e+03,
+ 0.2436734402904e-09, 0.3254726114901e+01, 0.2268582385539e+03,
+ 0.2213605274325e-09, 0.1687210598530e+01, 0.1658638954901e+03,
+ 0.1491521204829e-09, 0.2657541786794e+01, 0.2219950288015e+03,
+ 0.1474995329744e-09, 0.5013089805819e+01, 0.3052819430710e+03,
+ 0.1661939475656e-09, 0.5495315428418e+01, 0.2526661704812e+03,
+
+ 0.9015946748003e-10, 0.2236989966505e+01, 0.4171445043968e+03 };
+
+/* Sun-to-Earth, T^0, Z */
+ static const double e0z[] = {
+ 0.2796207639075e-05, 0.3198701560209e+01, 0.8433466158131e+02,
+ 0.1016042198142e-05, 0.5422360395913e+01, 0.5507553240374e+01,
+ 0.8044305033647e-06, 0.3880222866652e+01, 0.5223693906222e+01,
+ 0.4385347909274e-06, 0.3704369937468e+01, 0.2352866153506e+01,
+ 0.3186156414906e-06, 0.3999639363235e+01, 0.1577343543434e+01,
+ 0.2272412285792e-06, 0.3984738315952e+01, 0.1047747311755e+01,
+ 0.1645620103007e-06, 0.3565412516841e+01, 0.5856477690889e+01,
+ 0.1815836921166e-06, 0.4984507059020e+01, 0.6283075850446e+01,
+ 0.1447461676364e-06, 0.3702753570108e+01, 0.9437762937313e+01,
+ 0.1430760876382e-06, 0.3409658712357e+01, 0.1021328554739e+02,
+
+ 0.1120445753226e-06, 0.4829561570246e+01, 0.1414349524433e+02,
+ 0.1090232840797e-06, 0.2080729178066e+01, 0.6812766822558e+01,
+ 0.9715727346551e-07, 0.3476295881948e+01, 0.4694002934110e+01,
+ 0.1036267136217e-06, 0.4056639536648e+01, 0.7109288135493e+02,
+ 0.8752665271340e-07, 0.4448159519911e+01, 0.5753384878334e+01,
+ 0.8331864956004e-07, 0.4991704044208e+01, 0.7084896783808e+01,
+ 0.6901658670245e-07, 0.4325358994219e+01, 0.6275962395778e+01,
+ 0.9144536848998e-07, 0.1141826375363e+01, 0.6620890113188e+01,
+ 0.7205085037435e-07, 0.3624344170143e+01, 0.5296909721118e+00,
+ 0.7697874654176e-07, 0.5554257458998e+01, 0.1676215758509e+03,
+
+ 0.5197545738384e-07, 0.6251760961735e+01, 0.1807370494127e+02,
+ 0.5031345378608e-07, 0.2497341091913e+01, 0.4705732307012e+01,
+ 0.4527110205840e-07, 0.2335079920992e+01, 0.6309374173736e+01,
+ 0.4753355798089e-07, 0.7094148987474e+00, 0.5884926831456e+01,
+ 0.4296951977516e-07, 0.1101916352091e+01, 0.6681224869435e+01,
+ 0.3855341568387e-07, 0.1825495405486e+01, 0.5486777812467e+01,
+ 0.5253930970990e-07, 0.4424740687208e+01, 0.7860419393880e+01,
+ 0.4024630496471e-07, 0.5120498157053e+01, 0.1336797263425e+02,
+ 0.4061069791453e-07, 0.6029771435451e+01, 0.3930209696940e+01,
+ 0.3797883804205e-07, 0.4435193600836e+00, 0.3154687086868e+01,
+
+ 0.2933033225587e-07, 0.5124157356507e+01, 0.1059381944224e+01,
+ 0.3503000930426e-07, 0.5421830162065e+01, 0.6069776770667e+01,
+ 0.3670096214050e-07, 0.4582101667297e+01, 0.1219403291462e+02,
+ 0.2905609437008e-07, 0.1926566420072e+01, 0.1097707878456e+02,
+ 0.2466827821713e-07, 0.6090174539834e+00, 0.6496374930224e+01,
+ 0.2691647295332e-07, 0.1393432595077e+01, 0.2200391463820e+02,
+ 0.2150554667946e-07, 0.4308671715951e+01, 0.5643178611111e+01,
+ 0.2237481922680e-07, 0.8133968269414e+00, 0.8635942003952e+01,
+ 0.1817741038157e-07, 0.3755205127454e+01, 0.3340612434717e+01,
+ 0.2227820762132e-07, 0.2759558596664e+01, 0.1203646072878e+02,
+
+ 0.1944713772307e-07, 0.5699645869121e+01, 0.1179062909082e+02,
+ 0.1527340520662e-07, 0.1986749091746e+01, 0.3981490189893e+00,
+ 0.1577282574914e-07, 0.3205017217983e+01, 0.5088628793478e+01,
+ 0.1424738825424e-07, 0.6256747903666e+01, 0.2544314396739e+01,
+ 0.1616563121701e-07, 0.2601671259394e+00, 0.1729818233119e+02,
+ 0.1401210391692e-07, 0.4686939173506e+01, 0.7058598460518e+01,
+ 0.1488726974214e-07, 0.2815862451372e+01, 0.2593412433514e+02,
+ 0.1692626442388e-07, 0.4956894109797e+01, 0.1564752902480e+03,
+ 0.1123571582910e-07, 0.2381192697696e+01, 0.3738761453707e+01,
+ 0.9903308606317e-08, 0.4294851657684e+01, 0.9225539266174e+01,
+
+ 0.9174533187191e-08, 0.3075171510642e+01, 0.4164311961999e+01,
+ 0.8645985631457e-08, 0.5477534821633e+00, 0.8429241228195e+01,
+ -0.1085876492688e-07, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.9264309077815e-08, 0.5968571670097e+01, 0.7079373888424e+01,
+ 0.8243116984954e-08, 0.1489098777643e+01, 0.1044738781244e+02,
+ 0.8268102113708e-08, 0.3512977691983e+01, 0.1150676975667e+02,
+ 0.9043613988227e-08, 0.1290704408221e+00, 0.1101510648075e+02,
+ 0.7432912038789e-08, 0.1991086893337e+01, 0.2608790314060e+02,
+ 0.8586233727285e-08, 0.4238357924414e+01, 0.2986433403208e+02,
+ 0.7612230060131e-08, 0.2911090150166e+01, 0.4732030630302e+01,
+
+ 0.7097787751408e-08, 0.1908938392390e+01, 0.8031092209206e+01,
+ 0.7640237040175e-08, 0.6129219000168e+00, 0.7962980379786e+00,
+ 0.7070445688081e-08, 0.1380417036651e+01, 0.2146165377750e+01,
+ 0.7690770957702e-08, 0.1680504249084e+01, 0.2122839202813e+02,
+ 0.8051292542594e-08, 0.5127423484511e+01, 0.2942463415728e+01,
+ 0.5902709104515e-08, 0.2020274190917e+01, 0.7755226100720e+00,
+ 0.5134567496462e-08, 0.2606778676418e+01, 0.1256615170089e+02,
+ 0.5525802046102e-08, 0.1613011769663e+01, 0.8018209333619e+00,
+ 0.5880724784221e-08, 0.4604483417236e+01, 0.4690479774488e+01,
+ 0.5211699081370e-08, 0.5718964114193e+01, 0.8827390247185e+01,
+
+ 0.4891849573562e-08, 0.3689658932196e+01, 0.2132990797783e+00,
+ 0.5150246069997e-08, 0.4099769855122e+01, 0.6480980550449e+02,
+ 0.5102434319633e-08, 0.5660834602509e+01, 0.3379454372902e+02,
+ 0.5083405254252e-08, 0.9842221218974e+00, 0.4136910472696e+01,
+ 0.4206562585682e-08, 0.1341363634163e+00, 0.3128388763578e+01,
+ 0.4663249683579e-08, 0.8130132735866e+00, 0.5216580451554e+01,
+ 0.4099474416530e-08, 0.5791497770644e+01, 0.4265981595566e+00,
+ 0.4628251220767e-08, 0.1249802769331e+01, 0.1572083878776e+02,
+ 0.5024068728142e-08, 0.4795684802743e+01, 0.6290189305114e+01,
+ 0.5120234327758e-08, 0.3810420387208e+01, 0.5230807360890e+01,
+
+ 0.5524029815280e-08, 0.1029264714351e+01, 0.2397622045175e+03,
+ 0.4757415718860e-08, 0.3528044781779e+01, 0.1649636139783e+02,
+ 0.3915786131127e-08, 0.5593889282646e+01, 0.1589072916335e+01,
+ 0.4869053149991e-08, 0.3299636454433e+01, 0.7632943190217e+01,
+ 0.3649365703729e-08, 0.1286049002584e+01, 0.6206810014183e+01,
+ 0.3992493949002e-08, 0.3100307589464e+01, 0.2515860172507e+02,
+ 0.3320247477418e-08, 0.6212683940807e+01, 0.1216800268190e+02,
+ 0.3287123739696e-08, 0.4699118445928e+01, 0.7234794171227e+01,
+ 0.3472776811103e-08, 0.2630507142004e+01, 0.7342457794669e+01,
+ 0.3423253294767e-08, 0.2946432844305e+01, 0.9623688285163e+01,
+
+ 0.3896173898244e-08, 0.1224834179264e+01, 0.6438496133249e+01,
+ 0.3388455337924e-08, 0.1543807616351e+01, 0.1494531617769e+02,
+ 0.3062704716523e-08, 0.1191777572310e+01, 0.8662240327241e+01,
+ 0.3270075600400e-08, 0.5483498767737e+01, 0.1194447056968e+01,
+ 0.3101209215259e-08, 0.8000833804348e+00, 0.3772475342596e+02,
+ 0.2780883347311e-08, 0.4077980721888e+00, 0.5863591145557e+01,
+ 0.2903605931824e-08, 0.2617490302147e+01, 0.1965104848470e+02,
+ 0.2682014743119e-08, 0.2634703158290e+01, 0.7238675589263e+01,
+ 0.2534360108492e-08, 0.6102446114873e+01, 0.6836645152238e+01,
+ 0.2392564882509e-08, 0.3681820208691e+01, 0.5849364236221e+01,
+
+ 0.2656667254856e-08, 0.6216045388886e+01, 0.6133512519065e+01,
+ 0.2331242096773e-08, 0.5864949777744e+01, 0.4535059491685e+01,
+ 0.2287898363668e-08, 0.4566628532802e+01, 0.7477522907414e+01,
+ 0.2336944521306e-08, 0.2442722126930e+01, 0.1137170464392e+02,
+ 0.3156632236269e-08, 0.1626628050682e+01, 0.2509084901204e+03,
+ 0.2982612402766e-08, 0.2803604512609e+01, 0.1748016358760e+01,
+ 0.2774031674807e-08, 0.4654002897158e+01, 0.8223916695780e+02,
+ 0.2295236548638e-08, 0.4326518333253e+01, 0.3378142627421e+00,
+ 0.2190714699873e-08, 0.4519614578328e+01, 0.2908881142201e+02,
+ 0.2191495845045e-08, 0.3012626912549e+01, 0.1673046366289e+02,
+
+ 0.2492901628386e-08, 0.1290101424052e+00, 0.1543797956245e+03,
+ 0.1993778064319e-08, 0.3864046799414e+01, 0.1778984560711e+02,
+ 0.1898146479022e-08, 0.5053777235891e+01, 0.2042657109477e+02,
+ 0.1918280127634e-08, 0.2222470192548e+01, 0.4165496312290e+02,
+ 0.1916351061607e-08, 0.8719067257774e+00, 0.7737595720538e+02,
+ 0.1834720181466e-08, 0.4031491098040e+01, 0.2358125818164e+02,
+ 0.1249201523806e-08, 0.5938379466835e+01, 0.3301902111895e+02,
+ 0.1477304050539e-08, 0.6544722606797e+00, 0.9548094718417e+02,
+ 0.1264316431249e-08, 0.2059072853236e+01, 0.8399684731857e+02,
+ 0.1203526495039e-08, 0.3644813532605e+01, 0.4558517281984e+02,
+
+ 0.9221681059831e-09, 0.3241815055602e+01, 0.7805158573086e+02,
+ 0.7849278367646e-09, 0.5043812342457e+01, 0.5217580628120e+02,
+ 0.7983392077387e-09, 0.5000024502753e+01, 0.1501922143975e+03,
+ 0.7925395431654e-09, 0.1398734871821e-01, 0.9061773743175e+02,
+ 0.7640473285886e-09, 0.5067111723130e+01, 0.4951538251678e+02,
+ 0.5398937754482e-09, 0.5597382200075e+01, 0.1613385000004e+03,
+ 0.5626247550193e-09, 0.2601338209422e+01, 0.7318837597844e+02,
+ 0.5525197197855e-09, 0.5814832109256e+01, 0.1432335100216e+03,
+ 0.5407629837898e-09, 0.3384820609076e+01, 0.3230491187871e+03,
+ 0.3856739119801e-09, 0.1072391840473e+01, 0.2334791286671e+03,
+
+ 0.3856425239987e-09, 0.2369540393327e+01, 0.1739046517013e+03,
+ 0.4350867755983e-09, 0.5255575751082e+01, 0.1620484330494e+03,
+ 0.3844113924996e-09, 0.5482356246182e+01, 0.9757644180768e+02,
+ 0.2854869155431e-09, 0.9573634763143e+00, 0.1697170704744e+03,
+ 0.1719227671416e-09, 0.1887203025202e+01, 0.2265204242912e+03,
+ 0.1527846879755e-09, 0.3982183931157e+01, 0.3341954043900e+03,
+ 0.1128229264847e-09, 0.2787457156298e+01, 0.3119028331842e+03 };
+
+/* Sun-to-Earth, T^1, X */
+ static const double e1x[] = {
+ 0.1234046326004e-05, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.5150068824701e-06, 0.6002664557501e+01, 0.1256615170089e+02,
+ 0.1290743923245e-07, 0.5959437664199e+01, 0.1884922755134e+02,
+ 0.1068615564952e-07, 0.2015529654209e+01, 0.6283075850446e+01,
+ 0.2079619142538e-08, 0.1732960531432e+01, 0.6279552690824e+01,
+ 0.2078009243969e-08, 0.4915604476996e+01, 0.6286599010068e+01,
+ 0.6206330058856e-09, 0.3616457953824e+00, 0.4705732307012e+01,
+ 0.5989335313746e-09, 0.3802607304474e+01, 0.6256777527156e+01,
+ 0.5958495663840e-09, 0.2845866560031e+01, 0.6309374173736e+01,
+ 0.4866923261539e-09, 0.5213203771824e+01, 0.7755226100720e+00,
+
+ 0.4267785823142e-09, 0.4368189727818e+00, 0.1059381944224e+01,
+ 0.4610675141648e-09, 0.1837249181372e-01, 0.7860419393880e+01,
+ 0.3626989993973e-09, 0.2161590545326e+01, 0.5753384878334e+01,
+ 0.3563071194389e-09, 0.1452631954746e+01, 0.5884926831456e+01,
+ 0.3557015642807e-09, 0.4470593393054e+01, 0.6812766822558e+01,
+ 0.3210412089122e-09, 0.5195926078314e+01, 0.6681224869435e+01,
+ 0.2875473577986e-09, 0.5916256610193e+01, 0.2513230340178e+02,
+ 0.2842913681629e-09, 0.1149902426047e+01, 0.6127655567643e+01,
+ 0.2751248215916e-09, 0.5502088574662e+01, 0.6438496133249e+01,
+ 0.2481432881127e-09, 0.2921989846637e+01, 0.5486777812467e+01,
+
+ 0.2059885976560e-09, 0.3718070376585e+01, 0.7079373888424e+01,
+ 0.2015522342591e-09, 0.5979395259740e+01, 0.6290189305114e+01,
+ 0.1995364084253e-09, 0.6772087985494e+00, 0.6275962395778e+01,
+ 0.1957436436943e-09, 0.2899210654665e+01, 0.5507553240374e+01,
+ 0.1651609818948e-09, 0.6228206482192e+01, 0.1150676975667e+02,
+ 0.1822980550699e-09, 0.1469348746179e+01, 0.1179062909082e+02,
+ 0.1675223159760e-09, 0.3813910555688e+01, 0.7058598460518e+01,
+ 0.1706491764745e-09, 0.3004380506684e+00, 0.7113454667900e-02,
+ 0.1392952362615e-09, 0.1440393973406e+01, 0.7962980379786e+00,
+ 0.1209868266342e-09, 0.4150425791727e+01, 0.4694002934110e+01,
+
+ 0.1009827202611e-09, 0.3290040429843e+01, 0.3738761453707e+01,
+ 0.1047261388602e-09, 0.4229590090227e+01, 0.6282095334605e+01,
+ 0.1047006652004e-09, 0.2418967680575e+01, 0.6284056366286e+01,
+ 0.9609993143095e-10, 0.4627943659201e+01, 0.6069776770667e+01,
+ 0.9590900593873e-10, 0.1894393939924e+01, 0.4136910472696e+01,
+ 0.9146249188071e-10, 0.2010647519562e+01, 0.6496374930224e+01,
+ 0.8545274480290e-10, 0.5529846956226e-01, 0.1194447056968e+01,
+ 0.8224377881194e-10, 0.1254304102174e+01, 0.1589072916335e+01,
+ 0.6183529510410e-10, 0.3360862168815e+01, 0.8827390247185e+01,
+ 0.6259255147141e-10, 0.4755628243179e+01, 0.8429241228195e+01,
+
+ 0.5539291694151e-10, 0.5371746955142e+01, 0.4933208510675e+01,
+ 0.7328259466314e-10, 0.4927699613906e+00, 0.4535059491685e+01,
+ 0.6017835843560e-10, 0.5776682001734e-01, 0.1255903824622e+02,
+ 0.7079827775243e-10, 0.4395059432251e+01, 0.5088628793478e+01,
+ 0.5170358878213e-10, 0.5154062619954e+01, 0.1176985366291e+02,
+ 0.4872301838682e-10, 0.6289611648973e+00, 0.6040347114260e+01,
+ 0.5249869411058e-10, 0.5617272046949e+01, 0.3154687086868e+01,
+ 0.4716172354411e-10, 0.3965901800877e+01, 0.5331357529664e+01,
+ 0.4871214940964e-10, 0.4627507050093e+01, 0.1256967486051e+02,
+ 0.4598076850751e-10, 0.6023631226459e+01, 0.6525804586632e+01,
+
+ 0.4562196089485e-10, 0.4138562084068e+01, 0.3930209696940e+01,
+ 0.4325493872224e-10, 0.1330845906564e+01, 0.7632943190217e+01,
+ 0.5673781176748e-10, 0.2558752615657e+01, 0.5729506548653e+01,
+ 0.3961436642503e-10, 0.2728071734630e+01, 0.7234794171227e+01,
+ 0.5101868209058e-10, 0.4113444965144e+01, 0.6836645152238e+01,
+ 0.5257043167676e-10, 0.6195089830590e+01, 0.8031092209206e+01,
+ 0.5076613989393e-10, 0.2305124132918e+01, 0.7477522907414e+01,
+ 0.3342169352778e-10, 0.5415998155071e+01, 0.1097707878456e+02,
+ 0.3545881983591e-10, 0.3727160564574e+01, 0.4164311961999e+01,
+ 0.3364063738599e-10, 0.2901121049204e+00, 0.1137170464392e+02,
+
+ 0.3357039670776e-10, 0.1652229354331e+01, 0.5223693906222e+01,
+ 0.4307412268687e-10, 0.4938909587445e+01, 0.1592596075957e+01,
+ 0.3405769115435e-10, 0.2408890766511e+01, 0.3128388763578e+01,
+ 0.3001926198480e-10, 0.4862239006386e+01, 0.1748016358760e+01,
+ 0.2778264787325e-10, 0.5241168661353e+01, 0.7342457794669e+01,
+ 0.2676159480666e-10, 0.3423593942199e+01, 0.2146165377750e+01,
+ 0.2954273399939e-10, 0.1881721265406e+01, 0.5368044267797e+00,
+ 0.3309362888795e-10, 0.1931525677349e+01, 0.8018209333619e+00,
+ 0.2810283608438e-10, 0.2414659495050e+01, 0.5225775174439e+00,
+ 0.3378045637764e-10, 0.4238019163430e+01, 0.1554202828031e+00,
+
+ 0.2558134979840e-10, 0.1828225235805e+01, 0.5230807360890e+01,
+ 0.2273755578447e-10, 0.5858184283998e+01, 0.7084896783808e+01,
+ 0.2294176037690e-10, 0.4514589779057e+01, 0.1726015463500e+02,
+ 0.2533506099435e-10, 0.2355717851551e+01, 0.5216580451554e+01,
+ 0.2716685375812e-10, 0.2221003625100e+01, 0.8635942003952e+01,
+ 0.2419043435198e-10, 0.5955704951635e+01, 0.4690479774488e+01,
+ 0.2521232544812e-10, 0.1395676848521e+01, 0.5481254917084e+01,
+ 0.2630195021491e-10, 0.5727468918743e+01, 0.2629832328990e-01,
+ 0.2548395840944e-10, 0.2628351859400e-03, 0.1349867339771e+01 };
+
+/* Sun-to-Earth, T^1, Y */
+ static const double e1y[] = {
+ 0.9304690546528e-06, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.5150715570663e-06, 0.4431807116294e+01, 0.1256615170089e+02,
+ 0.1290825411056e-07, 0.4388610039678e+01, 0.1884922755134e+02,
+ 0.4645466665386e-08, 0.5827263376034e+01, 0.6283075850446e+01,
+ 0.2079625310718e-08, 0.1621698662282e+00, 0.6279552690824e+01,
+ 0.2078189850907e-08, 0.3344713435140e+01, 0.6286599010068e+01,
+ 0.6207190138027e-09, 0.5074049319576e+01, 0.4705732307012e+01,
+ 0.5989826532569e-09, 0.2231842216620e+01, 0.6256777527156e+01,
+ 0.5961360812618e-09, 0.1274975769045e+01, 0.6309374173736e+01,
+ 0.4874165471016e-09, 0.3642277426779e+01, 0.7755226100720e+00,
+
+ 0.4283834034360e-09, 0.5148765510106e+01, 0.1059381944224e+01,
+ 0.4652389287529e-09, 0.4715794792175e+01, 0.7860419393880e+01,
+ 0.3751707476401e-09, 0.6617207370325e+00, 0.5753384878334e+01,
+ 0.3559998806198e-09, 0.6155548875404e+01, 0.5884926831456e+01,
+ 0.3558447558857e-09, 0.2898827297664e+01, 0.6812766822558e+01,
+ 0.3211116927106e-09, 0.3625813502509e+01, 0.6681224869435e+01,
+ 0.2875609914672e-09, 0.4345435813134e+01, 0.2513230340178e+02,
+ 0.2843109704069e-09, 0.5862263940038e+01, 0.6127655567643e+01,
+ 0.2744676468427e-09, 0.3926419475089e+01, 0.6438496133249e+01,
+ 0.2481285237789e-09, 0.1351976572828e+01, 0.5486777812467e+01,
+
+ 0.2060338481033e-09, 0.2147556998591e+01, 0.7079373888424e+01,
+ 0.2015822358331e-09, 0.4408358972216e+01, 0.6290189305114e+01,
+ 0.2001195944195e-09, 0.5385829822531e+01, 0.6275962395778e+01,
+ 0.1953667642377e-09, 0.1304933746120e+01, 0.5507553240374e+01,
+ 0.1839744078713e-09, 0.6173567228835e+01, 0.1179062909082e+02,
+ 0.1643334294845e-09, 0.4635942997523e+01, 0.1150676975667e+02,
+ 0.1768051018652e-09, 0.5086283558874e+01, 0.7113454667900e-02,
+ 0.1674874205489e-09, 0.2243332137241e+01, 0.7058598460518e+01,
+ 0.1421445397609e-09, 0.6186899771515e+01, 0.7962980379786e+00,
+ 0.1255163958267e-09, 0.5730238465658e+01, 0.4694002934110e+01,
+
+ 0.1013945281961e-09, 0.1726055228402e+01, 0.3738761453707e+01,
+ 0.1047294335852e-09, 0.2658801228129e+01, 0.6282095334605e+01,
+ 0.1047103879392e-09, 0.8481047835035e+00, 0.6284056366286e+01,
+ 0.9530343962826e-10, 0.3079267149859e+01, 0.6069776770667e+01,
+ 0.9604637611690e-10, 0.3258679792918e+00, 0.4136910472696e+01,
+ 0.9153518537177e-10, 0.4398599886584e+00, 0.6496374930224e+01,
+ 0.8562458214922e-10, 0.4772686794145e+01, 0.1194447056968e+01,
+ 0.8232525360654e-10, 0.5966220721679e+01, 0.1589072916335e+01,
+ 0.6150223411438e-10, 0.1780985591923e+01, 0.8827390247185e+01,
+ 0.6272087858000e-10, 0.3184305429012e+01, 0.8429241228195e+01,
+
+ 0.5540476311040e-10, 0.3801260595433e+01, 0.4933208510675e+01,
+ 0.7331901699361e-10, 0.5205948591865e+01, 0.4535059491685e+01,
+ 0.6018528702791e-10, 0.4770139083623e+01, 0.1255903824622e+02,
+ 0.5150530724804e-10, 0.3574796899585e+01, 0.1176985366291e+02,
+ 0.6471933741811e-10, 0.2679787266521e+01, 0.5088628793478e+01,
+ 0.5317460644174e-10, 0.9528763345494e+00, 0.3154687086868e+01,
+ 0.4832187748783e-10, 0.5329322498232e+01, 0.6040347114260e+01,
+ 0.4716763555110e-10, 0.2395235316466e+01, 0.5331357529664e+01,
+ 0.4871509139861e-10, 0.3056663648823e+01, 0.1256967486051e+02,
+ 0.4598417696768e-10, 0.4452762609019e+01, 0.6525804586632e+01,
+
+ 0.5674189533175e-10, 0.9879680872193e+00, 0.5729506548653e+01,
+ 0.4073560328195e-10, 0.5939127696986e+01, 0.7632943190217e+01,
+ 0.5040994945359e-10, 0.4549875824510e+01, 0.8031092209206e+01,
+ 0.5078185134679e-10, 0.7346659893982e+00, 0.7477522907414e+01,
+ 0.3769343537061e-10, 0.1071317188367e+01, 0.7234794171227e+01,
+ 0.4980331365299e-10, 0.2500345341784e+01, 0.6836645152238e+01,
+ 0.3458236594757e-10, 0.3825159450711e+01, 0.1097707878456e+02,
+ 0.3578859493602e-10, 0.5299664791549e+01, 0.4164311961999e+01,
+ 0.3370504646419e-10, 0.5002316301593e+01, 0.1137170464392e+02,
+ 0.3299873338428e-10, 0.2526123275282e+01, 0.3930209696940e+01,
+
+ 0.4304917318409e-10, 0.3368078557132e+01, 0.1592596075957e+01,
+ 0.3402418753455e-10, 0.8385495425800e+00, 0.3128388763578e+01,
+ 0.2778460572146e-10, 0.3669905203240e+01, 0.7342457794669e+01,
+ 0.2782710128902e-10, 0.2691664812170e+00, 0.1748016358760e+01,
+ 0.2711725179646e-10, 0.4707487217718e+01, 0.5296909721118e+00,
+ 0.2981760946340e-10, 0.3190260867816e+00, 0.5368044267797e+00,
+ 0.2811672977772e-10, 0.3196532315372e+01, 0.7084896783808e+01,
+ 0.2863454474467e-10, 0.2263240324780e+00, 0.5223693906222e+01,
+ 0.3333464634051e-10, 0.3498451685065e+01, 0.8018209333619e+00,
+ 0.3312991747609e-10, 0.5839154477412e+01, 0.1554202828031e+00,
+
+ 0.2813255564006e-10, 0.8268044346621e+00, 0.5225775174439e+00,
+ 0.2665098083966e-10, 0.3934021725360e+01, 0.5216580451554e+01,
+ 0.2349795705216e-10, 0.5197620913779e+01, 0.2146165377750e+01,
+ 0.2330352293961e-10, 0.2984999231807e+01, 0.1726015463500e+02,
+ 0.2728001683419e-10, 0.6521679638544e+00, 0.8635942003952e+01,
+ 0.2484061007669e-10, 0.3468955561097e+01, 0.5230807360890e+01,
+ 0.2646328768427e-10, 0.1013724533516e+01, 0.2629832328990e-01,
+ 0.2518630264831e-10, 0.6108081057122e+01, 0.5481254917084e+01,
+ 0.2421901455384e-10, 0.1651097776260e+01, 0.1349867339771e+01,
+ 0.6348533267831e-11, 0.3220226560321e+01, 0.8433466158131e+02 };
+
+/* Sun-to-Earth, T^1, Z */
+ static const double e1z[] = {
+ 0.2278290449966e-05, 0.3413716033863e+01, 0.6283075850446e+01,
+ 0.5429458209830e-07, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.1903240492525e-07, 0.3370592358297e+01, 0.1256615170089e+02,
+ 0.2385409276743e-09, 0.3327914718416e+01, 0.1884922755134e+02,
+ 0.8676928342573e-10, 0.1824006811264e+01, 0.5223693906222e+01,
+ 0.7765442593544e-10, 0.3888564279247e+01, 0.5507553240374e+01,
+ 0.7066158332715e-10, 0.5194267231944e+01, 0.2352866153506e+01,
+ 0.7092175288657e-10, 0.2333246960021e+01, 0.8399684731857e+02,
+ 0.5357582213535e-10, 0.2224031176619e+01, 0.5296909721118e+00,
+ 0.3828035865021e-10, 0.2156710933584e+01, 0.6279552690824e+01,
+
+ 0.3824857220427e-10, 0.1529755219915e+01, 0.6286599010068e+01,
+ 0.3286995181628e-10, 0.4879512900483e+01, 0.1021328554739e+02 };
+
+/* Sun-to-Earth, T^2, X */
+ static const double e2x[] = {
+ -0.4143818297913e-10, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.2171497694435e-10, 0.4398225628264e+01, 0.1256615170089e+02,
+ 0.9845398442516e-11, 0.2079720838384e+00, 0.6283075850446e+01,
+ 0.9256833552682e-12, 0.4191264694361e+01, 0.1884922755134e+02,
+ 0.1022049384115e-12, 0.5381133195658e+01, 0.8399684731857e+02 };
+
+/* Sun-to-Earth, T^2, Y */
+ static const double e2y[] = {
+ 0.5063375872532e-10, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.2173815785980e-10, 0.2827805833053e+01, 0.1256615170089e+02,
+ 0.1010231999920e-10, 0.4634612377133e+01, 0.6283075850446e+01,
+ 0.9259745317636e-12, 0.2620612076189e+01, 0.1884922755134e+02,
+ 0.1022202095812e-12, 0.3809562326066e+01, 0.8399684731857e+02 };
+
+/* Sun-to-Earth, T^2, Z */
+ static const double e2z[] = {
+ 0.9722666114891e-10, 0.5152219582658e+01, 0.6283075850446e+01,
+ -0.3494819171909e-11, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.6713034376076e-12, 0.6440188750495e+00, 0.1256615170089e+02 };
+
+/* SSB-to-Sun, T^0, X */
+ static const double s0x[] = {
+ 0.4956757536410e-02, 0.3741073751789e+01, 0.5296909721118e+00,
+ 0.2718490072522e-02, 0.4016011511425e+01, 0.2132990797783e+00,
+ 0.1546493974344e-02, 0.2170528330642e+01, 0.3813291813120e-01,
+ 0.8366855276341e-03, 0.2339614075294e+01, 0.7478166569050e-01,
+ 0.2936777942117e-03, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.1201317439469e-03, 0.4090736353305e+01, 0.1059381944224e+01,
+ 0.7578550887230e-04, 0.3241518088140e+01, 0.4265981595566e+00,
+ 0.1941787367773e-04, 0.1012202064330e+01, 0.2061856251104e+00,
+ 0.1889227765991e-04, 0.3892520416440e+01, 0.2204125344462e+00,
+ 0.1937896968613e-04, 0.4797779441161e+01, 0.1495633313810e+00,
+
+ 0.1434506110873e-04, 0.3868960697933e+01, 0.5225775174439e+00,
+ 0.1406659911580e-04, 0.4759766557397e+00, 0.5368044267797e+00,
+ 0.1179022300202e-04, 0.7774961520598e+00, 0.7626583626240e-01,
+ 0.8085864460959e-05, 0.3254654471465e+01, 0.3664874755930e-01,
+ 0.7622752967615e-05, 0.4227633103489e+01, 0.3961708870310e-01,
+ 0.6209171139066e-05, 0.2791828325711e+00, 0.7329749511860e-01,
+ 0.4366435633970e-05, 0.4440454875925e+01, 0.1589072916335e+01,
+ 0.3792124889348e-05, 0.5156393842356e+01, 0.7113454667900e-02,
+ 0.3154548963402e-05, 0.6157005730093e+01, 0.4194847048887e+00,
+ 0.3088359882942e-05, 0.2494567553163e+01, 0.6398972393349e+00,
+
+ 0.2788440902136e-05, 0.4934318747989e+01, 0.1102062672231e+00,
+ 0.3039928456376e-05, 0.4895077702640e+01, 0.6283075850446e+01,
+ 0.2272258457679e-05, 0.5278394064764e+01, 0.1030928125552e+00,
+ 0.2162007057957e-05, 0.5802978019099e+01, 0.3163918923335e+00,
+ 0.1767632855737e-05, 0.3415346595193e-01, 0.1021328554739e+02,
+ 0.1349413459362e-05, 0.2001643230755e+01, 0.1484170571900e-02,
+ 0.1170141900476e-05, 0.2424750491620e+01, 0.6327837846670e+00,
+ 0.1054355266820e-05, 0.3123311487576e+01, 0.4337116142245e+00,
+ 0.9800822461610e-06, 0.3026258088130e+01, 0.1052268489556e+01,
+ 0.1091203749931e-05, 0.3157811670347e+01, 0.1162474756779e+01,
+
+ 0.6960236715913e-06, 0.8219570542313e+00, 0.1066495398892e+01,
+ 0.5689257296909e-06, 0.1323052375236e+01, 0.9491756770005e+00,
+ 0.6613172135802e-06, 0.2765348881598e+00, 0.8460828644453e+00,
+ 0.6277702517571e-06, 0.5794064466382e+01, 0.1480791608091e+00,
+ 0.6304884066699e-06, 0.7323555380787e+00, 0.2243449970715e+00,
+ 0.4897850467382e-06, 0.3062464235399e+01, 0.3340612434717e+01,
+ 0.3759148598786e-06, 0.4588290469664e+01, 0.3516457698740e-01,
+ 0.3110520548195e-06, 0.1374299536572e+01, 0.6373574839730e-01,
+ 0.3064708359780e-06, 0.4222267485047e+01, 0.1104591729320e-01,
+ 0.2856347168241e-06, 0.3714202944973e+01, 0.1510475019529e+00,
+
+ 0.2840945514288e-06, 0.2847972875882e+01, 0.4110125927500e-01,
+ 0.2378951599405e-06, 0.3762072563388e+01, 0.2275259891141e+00,
+ 0.2714229481417e-06, 0.1036049980031e+01, 0.2535050500000e-01,
+ 0.2323551717307e-06, 0.4682388599076e+00, 0.8582758298370e-01,
+ 0.1881790512219e-06, 0.4790565425418e+01, 0.2118763888447e+01,
+ 0.2261353968371e-06, 0.1669144912212e+01, 0.7181332454670e-01,
+ 0.2214546389848e-06, 0.3937717281614e+01, 0.2968341143800e-02,
+ 0.2184915594933e-06, 0.1129169845099e+00, 0.7775000683430e-01,
+ 0.2000164937936e-06, 0.4030009638488e+01, 0.2093666171530e+00,
+ 0.1966105136719e-06, 0.8745955786834e+00, 0.2172315424036e+00,
+
+ 0.1904742332624e-06, 0.5919743598964e+01, 0.2022531624851e+00,
+ 0.1657399705031e-06, 0.2549141484884e+01, 0.7358765972222e+00,
+ 0.1574070533987e-06, 0.5277533020230e+01, 0.7429900518901e+00,
+ 0.1832261651039e-06, 0.3064688127777e+01, 0.3235053470014e+00,
+ 0.1733615346569e-06, 0.3011432799094e+01, 0.1385174140878e+00,
+ 0.1549124014496e-06, 0.4005569132359e+01, 0.5154640627760e+00,
+ 0.1637044713838e-06, 0.1831375966632e+01, 0.8531963191132e+00,
+ 0.1123420082383e-06, 0.1180270407578e+01, 0.1990721704425e+00,
+ 0.1083754165740e-06, 0.3414101320863e+00, 0.5439178814476e+00,
+ 0.1156638012655e-06, 0.6130479452594e+00, 0.5257585094865e+00,
+
+ 0.1142548785134e-06, 0.3724761948846e+01, 0.5336234347371e+00,
+ 0.7921463895965e-07, 0.2435425589361e+01, 0.1478866649112e+01,
+ 0.7428600285231e-07, 0.3542144398753e+01, 0.2164800718209e+00,
+ 0.8323211246747e-07, 0.3525058072354e+01, 0.1692165728891e+01,
+ 0.7257595116312e-07, 0.1364299431982e+01, 0.2101180877357e+00,
+ 0.7111185833236e-07, 0.2460478875808e+01, 0.4155522422634e+00,
+ 0.6868090383716e-07, 0.4397327670704e+01, 0.1173197218910e+00,
+ 0.7226419974175e-07, 0.4042647308905e+01, 0.1265567569334e+01,
+ 0.6955642383177e-07, 0.2865047906085e+01, 0.9562891316684e+00,
+ 0.7492139296331e-07, 0.5014278994215e+01, 0.1422690933580e-01,
+
+ 0.6598363128857e-07, 0.2376730020492e+01, 0.6470106940028e+00,
+ 0.7381147293385e-07, 0.3272990384244e+01, 0.1581959461667e+01,
+ 0.6402909624032e-07, 0.5302290955138e+01, 0.9597935788730e-01,
+ 0.6237454263857e-07, 0.5444144425332e+01, 0.7084920306520e-01,
+ 0.5241198544016e-07, 0.4215359579205e+01, 0.5265099800692e+00,
+ 0.5144463853918e-07, 0.1218916689916e+00, 0.5328719641544e+00,
+ 0.5868164772299e-07, 0.2369402002213e+01, 0.7871412831580e-01,
+ 0.6233195669151e-07, 0.1254922242403e+01, 0.2608790314060e+02,
+ 0.6068463791422e-07, 0.5679713760431e+01, 0.1114304132498e+00,
+ 0.4359361135065e-07, 0.6097219641646e+00, 0.1375773836557e+01,
+
+ 0.4686510366826e-07, 0.4786231041431e+01, 0.1143987543936e+00,
+ 0.3758977287225e-07, 0.1167368068139e+01, 0.1596186371003e+01,
+ 0.4282051974778e-07, 0.1519471064319e+01, 0.2770348281756e+00,
+ 0.5153765386113e-07, 0.1860532322984e+01, 0.2228608264996e+00,
+ 0.4575129387188e-07, 0.7632857887158e+00, 0.1465949902372e+00,
+ 0.3326844933286e-07, 0.1298219485285e+01, 0.5070101000000e-01,
+ 0.3748617450984e-07, 0.1046510321062e+01, 0.4903339079539e+00,
+ 0.2816756661499e-07, 0.3434522346190e+01, 0.2991266627620e+00,
+ 0.3412750405039e-07, 0.2523766270318e+01, 0.3518164938661e+00,
+ 0.2655796761776e-07, 0.2904422260194e+01, 0.6256703299991e+00,
+
+ 0.2963597929458e-07, 0.5923900431149e+00, 0.1099462426779e+00,
+ 0.2539523734781e-07, 0.4851947722567e+01, 0.1256615170089e+02,
+ 0.2283087914139e-07, 0.3400498595496e+01, 0.6681224869435e+01,
+ 0.2321309799331e-07, 0.5789099148673e+01, 0.3368040641550e-01,
+ 0.2549657649750e-07, 0.3991856479792e-01, 0.1169588211447e+01,
+ 0.2290462303977e-07, 0.2788567577052e+01, 0.1045155034888e+01,
+ 0.1945398522914e-07, 0.3290896998176e+01, 0.1155361302111e+01,
+ 0.1849171512638e-07, 0.2698060129367e+01, 0.4452511715700e-02,
+ 0.1647199834254e-07, 0.3016735644085e+01, 0.4408250688924e+00,
+ 0.1529530765273e-07, 0.5573043116178e+01, 0.6521991896920e-01,
+
+ 0.1433199339978e-07, 0.1481192356147e+01, 0.9420622223326e+00,
+ 0.1729134193602e-07, 0.1422817538933e+01, 0.2108507877249e+00,
+ 0.1716463931346e-07, 0.3469468901855e+01, 0.2157473718317e+00,
+ 0.1391206061378e-07, 0.6122436220547e+01, 0.4123712502208e+00,
+ 0.1404746661924e-07, 0.1647765641936e+01, 0.4258542984690e-01,
+ 0.1410452399455e-07, 0.5989729161964e+01, 0.2258291676434e+00,
+ 0.1089828772168e-07, 0.2833705509371e+01, 0.4226656969313e+00,
+ 0.1047374564948e-07, 0.5090690007331e+00, 0.3092784376656e+00,
+ 0.1358279126532e-07, 0.5128990262836e+01, 0.7923417740620e-01,
+ 0.1020456476148e-07, 0.9632772880808e+00, 0.1456308687557e+00,
+
+ 0.1033428735328e-07, 0.3223779318418e+01, 0.1795258541446e+01,
+ 0.1412435841540e-07, 0.2410271572721e+01, 0.1525316725248e+00,
+ 0.9722759371574e-08, 0.2333531395690e+01, 0.8434341241180e-01,
+ 0.9657334084704e-08, 0.6199270974168e+01, 0.1272681024002e+01,
+ 0.1083641148690e-07, 0.2864222292929e+01, 0.7032915397480e-01,
+ 0.1067318403838e-07, 0.5833458866568e+00, 0.2123349582968e+00,
+ 0.1062366201976e-07, 0.4307753989494e+01, 0.2142632012598e+00,
+ 0.1236364149266e-07, 0.2873917870593e+01, 0.1847279083684e+00,
+ 0.1092759489593e-07, 0.2959887266733e+01, 0.1370332435159e+00,
+ 0.8912069362899e-08, 0.5141213702562e+01, 0.2648454860559e+01,
+
+ 0.9656467707970e-08, 0.4532182462323e+01, 0.4376440768498e+00,
+ 0.8098386150135e-08, 0.2268906338379e+01, 0.2880807454688e+00,
+ 0.7857714675000e-08, 0.4055544260745e+01, 0.2037373330570e+00,
+ 0.7288455940646e-08, 0.5357901655142e+01, 0.1129145838217e+00,
+ 0.9450595950552e-08, 0.4264926963939e+01, 0.5272426800584e+00,
+ 0.9381718247537e-08, 0.7489366976576e-01, 0.5321392641652e+00,
+ 0.7079052646038e-08, 0.1923311052874e+01, 0.6288513220417e+00,
+ 0.9259004415344e-08, 0.2970256853438e+01, 0.1606092486742e+00,
+ 0.8259801499742e-08, 0.3327056314697e+01, 0.8389694097774e+00,
+ 0.6476334355779e-08, 0.2954925505727e+01, 0.2008557621224e+01,
+
+ 0.5984021492007e-08, 0.9138753105829e+00, 0.2042657109477e+02,
+ 0.5989546863181e-08, 0.3244464082031e+01, 0.2111650433779e+01,
+ 0.6233108606023e-08, 0.4995232638403e+00, 0.4305306221819e+00,
+ 0.6877299149965e-08, 0.2834987233449e+01, 0.9561746721300e-02,
+ 0.8311234227190e-08, 0.2202951835758e+01, 0.3801276407308e+00,
+ 0.6599472832414e-08, 0.4478581462618e+01, 0.1063314406849e+01,
+ 0.6160491096549e-08, 0.5145858696411e+01, 0.1368660381889e+01,
+ 0.6164772043891e-08, 0.3762976697911e+00, 0.4234171675140e+00,
+ 0.6363248684450e-08, 0.3162246718685e+01, 0.1253008786510e-01,
+ 0.6448587520999e-08, 0.3442693302119e+01, 0.5287268506303e+00,
+
+ 0.6431662283977e-08, 0.8977549136606e+00, 0.5306550935933e+00,
+ 0.6351223158474e-08, 0.4306447410369e+01, 0.5217580628120e+02,
+ 0.5476721393451e-08, 0.3888529177855e+01, 0.2221856701002e+01,
+ 0.5341772572619e-08, 0.2655560662512e+01, 0.7466759693650e-01,
+ 0.5337055758302e-08, 0.5164990735946e+01, 0.7489573444450e-01,
+ 0.5373120816787e-08, 0.6041214553456e+01, 0.1274714967946e+00,
+ 0.5392351705426e-08, 0.9177763485932e+00, 0.1055449481598e+01,
+ 0.6688495850205e-08, 0.3089608126937e+01, 0.2213766559277e+00,
+ 0.5072003660362e-08, 0.4311316541553e+01, 0.2132517061319e+00,
+ 0.5070726650455e-08, 0.5790675464444e+00, 0.2133464534247e+00,
+
+ 0.5658012950032e-08, 0.2703945510675e+01, 0.7287631425543e+00,
+ 0.4835509924854e-08, 0.2975422976065e+01, 0.7160067364790e-01,
+ 0.6479821978012e-08, 0.1324168733114e+01, 0.2209183458640e-01,
+ 0.6230636494980e-08, 0.2860103632836e+01, 0.3306188016693e+00,
+ 0.4649239516213e-08, 0.4832259763403e+01, 0.7796265773310e-01,
+ 0.6487325792700e-08, 0.2726165825042e+01, 0.3884652414254e+00,
+ 0.4682823682770e-08, 0.6966602455408e+00, 0.1073608853559e+01,
+ 0.5704230804976e-08, 0.5669634104606e+01, 0.8731175355560e-01,
+ 0.6125413585489e-08, 0.1513386538915e+01, 0.7605151500000e-01,
+ 0.6035825038187e-08, 0.1983509168227e+01, 0.9846002785331e+00,
+
+ 0.4331123462303e-08, 0.2782892992807e+01, 0.4297791515992e+00,
+ 0.4681107685143e-08, 0.5337232886836e+01, 0.2127790306879e+00,
+ 0.4669105829655e-08, 0.5837133792160e+01, 0.2138191288687e+00,
+ 0.5138823602365e-08, 0.3080560200507e+01, 0.7233337363710e-01,
+ 0.4615856664534e-08, 0.1661747897471e+01, 0.8603097737811e+00,
+ 0.4496916702197e-08, 0.2112508027068e+01, 0.7381754420900e-01,
+ 0.4278479042945e-08, 0.5716528462627e+01, 0.7574578717200e-01,
+ 0.3840525503932e-08, 0.6424172726492e+00, 0.3407705765729e+00,
+ 0.4866636509685e-08, 0.4919244697715e+01, 0.7722995774390e-01,
+ 0.3526100639296e-08, 0.2550821052734e+01, 0.6225157782540e-01,
+
+ 0.3939558488075e-08, 0.3939331491710e+01, 0.5268983110410e-01,
+ 0.4041268772576e-08, 0.2275337571218e+01, 0.3503323232942e+00,
+ 0.3948761842853e-08, 0.1999324200790e+01, 0.1451108196653e+00,
+ 0.3258394550029e-08, 0.9121001378200e+00, 0.5296435984654e+00,
+ 0.3257897048761e-08, 0.3428428660869e+01, 0.5297383457582e+00,
+ 0.3842559031298e-08, 0.6132927720035e+01, 0.9098186128426e+00,
+ 0.3109920095448e-08, 0.7693650193003e+00, 0.3932462625300e-02,
+ 0.3132237775119e-08, 0.3621293854908e+01, 0.2346394437820e+00,
+ 0.3942189421510e-08, 0.4841863659733e+01, 0.3180992042600e-02,
+ 0.3796972285340e-08, 0.1814174994268e+01, 0.1862120789403e+00,
+
+ 0.3995640233688e-08, 0.1386990406091e+01, 0.4549093064213e+00,
+ 0.2875013727414e-08, 0.9178318587177e+00, 0.1905464808669e+01,
+ 0.3073719932844e-08, 0.2688923811835e+01, 0.3628624111593e+00,
+ 0.2731016580075e-08, 0.1188259127584e+01, 0.2131850110243e+00,
+ 0.2729549896546e-08, 0.3702160634273e+01, 0.2134131485323e+00,
+ 0.3339372892449e-08, 0.7199163960331e+00, 0.2007689919132e+00,
+ 0.2898833764204e-08, 0.1916709364999e+01, 0.5291709230214e+00,
+ 0.2894536549362e-08, 0.2424043195547e+01, 0.5302110212022e+00,
+ 0.3096872473843e-08, 0.4445894977497e+01, 0.2976424921901e+00,
+ 0.2635672326810e-08, 0.3814366984117e+01, 0.1485980103780e+01,
+
+ 0.3649302697001e-08, 0.2924200596084e+01, 0.6044726378023e+00,
+ 0.3127954585895e-08, 0.1842251648327e+01, 0.1084620721060e+00,
+ 0.2616040173947e-08, 0.4155841921984e+01, 0.1258454114666e+01,
+ 0.2597395859860e-08, 0.1158045978874e+00, 0.2103781122809e+00,
+ 0.2593286172210e-08, 0.4771850408691e+01, 0.2162200472757e+00,
+ 0.2481823585747e-08, 0.4608842558889e+00, 0.1062562936266e+01,
+ 0.2742219550725e-08, 0.1538781127028e+01, 0.5651155736444e+00,
+ 0.3199558469610e-08, 0.3226647822878e+00, 0.7036329877322e+00,
+ 0.2666088542957e-08, 0.1967991731219e+00, 0.1400015846597e+00,
+ 0.2397067430580e-08, 0.3707036669873e+01, 0.2125476091956e+00,
+
+ 0.2376570772738e-08, 0.1182086628042e+01, 0.2140505503610e+00,
+ 0.2547228007887e-08, 0.4906256820629e+01, 0.1534957940063e+00,
+ 0.2265575594114e-08, 0.3414949866857e+01, 0.2235935264888e+00,
+ 0.2464381430585e-08, 0.4599122275378e+01, 0.2091065926078e+00,
+ 0.2433408527044e-08, 0.2830751145445e+00, 0.2174915669488e+00,
+ 0.2443605509076e-08, 0.4212046432538e+01, 0.1739420156204e+00,
+ 0.2319779262465e-08, 0.9881978408630e+00, 0.7530171478090e-01,
+ 0.2284622835465e-08, 0.5565347331588e+00, 0.7426161660010e-01,
+ 0.2467268750783e-08, 0.5655708150766e+00, 0.2526561439362e+00,
+ 0.2808513492782e-08, 0.1418405053408e+01, 0.5636314030725e+00,
+
+ 0.2329528932532e-08, 0.4069557545675e+01, 0.1056200952181e+01,
+ 0.9698639532817e-09, 0.1074134313634e+01, 0.7826370942180e+02 };
+
+/* SSB-to-Sun, T^0, Y */
+ static const double s0y[] = {
+ 0.4955392320126e-02, 0.2170467313679e+01, 0.5296909721118e+00,
+ 0.2722325167392e-02, 0.2444433682196e+01, 0.2132990797783e+00,
+ 0.1546579925346e-02, 0.5992779281546e+00, 0.3813291813120e-01,
+ 0.8363140252966e-03, 0.7687356310801e+00, 0.7478166569050e-01,
+ 0.3385792683603e-03, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.1201192221613e-03, 0.2520035601514e+01, 0.1059381944224e+01,
+ 0.7587125720554e-04, 0.1669954006449e+01, 0.4265981595566e+00,
+ 0.1964155361250e-04, 0.5707743963343e+01, 0.2061856251104e+00,
+ 0.1891900364909e-04, 0.2320960679937e+01, 0.2204125344462e+00,
+ 0.1937373433356e-04, 0.3226940689555e+01, 0.1495633313810e+00,
+
+ 0.1437139941351e-04, 0.2301626908096e+01, 0.5225775174439e+00,
+ 0.1406267683099e-04, 0.5188579265542e+01, 0.5368044267797e+00,
+ 0.1178703080346e-04, 0.5489483248476e+01, 0.7626583626240e-01,
+ 0.8079835186041e-05, 0.1683751835264e+01, 0.3664874755930e-01,
+ 0.7623253594652e-05, 0.2656400462961e+01, 0.3961708870310e-01,
+ 0.6248667483971e-05, 0.4992775362055e+01, 0.7329749511860e-01,
+ 0.4366353695038e-05, 0.2869706279678e+01, 0.1589072916335e+01,
+ 0.3829101568895e-05, 0.3572131359950e+01, 0.7113454667900e-02,
+ 0.3175733773908e-05, 0.4535372530045e+01, 0.4194847048887e+00,
+ 0.3092437902159e-05, 0.9230153317909e+00, 0.6398972393349e+00,
+
+ 0.2874168812154e-05, 0.3363143761101e+01, 0.1102062672231e+00,
+ 0.3040119321826e-05, 0.3324250895675e+01, 0.6283075850446e+01,
+ 0.2699723308006e-05, 0.2917882441928e+00, 0.1030928125552e+00,
+ 0.2134832683534e-05, 0.4220997202487e+01, 0.3163918923335e+00,
+ 0.1770412139433e-05, 0.4747318496462e+01, 0.1021328554739e+02,
+ 0.1377264209373e-05, 0.4305058462401e+00, 0.1484170571900e-02,
+ 0.1127814538960e-05, 0.8538177240740e+00, 0.6327837846670e+00,
+ 0.1055608090130e-05, 0.1551800742580e+01, 0.4337116142245e+00,
+ 0.9802673861420e-06, 0.1459646735377e+01, 0.1052268489556e+01,
+ 0.1090329461951e-05, 0.1587351228711e+01, 0.1162474756779e+01,
+
+ 0.6959590025090e-06, 0.5534442628766e+01, 0.1066495398892e+01,
+ 0.5664914529542e-06, 0.6030673003297e+01, 0.9491756770005e+00,
+ 0.6607787763599e-06, 0.4989507233927e+01, 0.8460828644453e+00,
+ 0.6269725742838e-06, 0.4222951804572e+01, 0.1480791608091e+00,
+ 0.6301889697863e-06, 0.5444316669126e+01, 0.2243449970715e+00,
+ 0.4891042662861e-06, 0.1490552839784e+01, 0.3340612434717e+01,
+ 0.3457083123290e-06, 0.3030475486049e+01, 0.3516457698740e-01,
+ 0.3032559967314e-06, 0.2652038793632e+01, 0.1104591729320e-01,
+ 0.2841133988903e-06, 0.1276744786829e+01, 0.4110125927500e-01,
+ 0.2855564444432e-06, 0.2143368674733e+01, 0.1510475019529e+00,
+
+ 0.2765157135038e-06, 0.5444186109077e+01, 0.6373574839730e-01,
+ 0.2382312465034e-06, 0.2190521137593e+01, 0.2275259891141e+00,
+ 0.2808060365077e-06, 0.5735195064841e+01, 0.2535050500000e-01,
+ 0.2332175234405e-06, 0.9481985524859e-01, 0.7181332454670e-01,
+ 0.2322488199659e-06, 0.5180499361533e+01, 0.8582758298370e-01,
+ 0.1881850258423e-06, 0.3219788273885e+01, 0.2118763888447e+01,
+ 0.2196111392808e-06, 0.2366941159761e+01, 0.2968341143800e-02,
+ 0.2183810335519e-06, 0.4825445110915e+01, 0.7775000683430e-01,
+ 0.2002733093326e-06, 0.2457148995307e+01, 0.2093666171530e+00,
+ 0.1967111767229e-06, 0.5586291545459e+01, 0.2172315424036e+00,
+
+ 0.1568473250543e-06, 0.3708003123320e+01, 0.7429900518901e+00,
+ 0.1852528314300e-06, 0.4310638151560e+01, 0.2022531624851e+00,
+ 0.1832111226447e-06, 0.1494665322656e+01, 0.3235053470014e+00,
+ 0.1746805502310e-06, 0.1451378500784e+01, 0.1385174140878e+00,
+ 0.1555730966650e-06, 0.1068040418198e+01, 0.7358765972222e+00,
+ 0.1554883462559e-06, 0.2442579035461e+01, 0.5154640627760e+00,
+ 0.1638380568746e-06, 0.2597913420625e+00, 0.8531963191132e+00,
+ 0.1159938593640e-06, 0.5834512021280e+01, 0.1990721704425e+00,
+ 0.1083427965695e-06, 0.5054033177950e+01, 0.5439178814476e+00,
+ 0.1156480369431e-06, 0.5325677432457e+01, 0.5257585094865e+00,
+
+ 0.1141308860095e-06, 0.2153403923857e+01, 0.5336234347371e+00,
+ 0.7913146470946e-07, 0.8642846847027e+00, 0.1478866649112e+01,
+ 0.7439752463733e-07, 0.1970628496213e+01, 0.2164800718209e+00,
+ 0.7280277104079e-07, 0.6073307250609e+01, 0.2101180877357e+00,
+ 0.8319567719136e-07, 0.1954371928334e+01, 0.1692165728891e+01,
+ 0.7137705549290e-07, 0.8904989440909e+00, 0.4155522422634e+00,
+ 0.6900825396225e-07, 0.2825717714977e+01, 0.1173197218910e+00,
+ 0.7245757216635e-07, 0.2481677513331e+01, 0.1265567569334e+01,
+ 0.6961165696255e-07, 0.1292955312978e+01, 0.9562891316684e+00,
+ 0.7571804456890e-07, 0.3427517575069e+01, 0.1422690933580e-01,
+
+ 0.6605425721904e-07, 0.8052192701492e+00, 0.6470106940028e+00,
+ 0.7375477357248e-07, 0.1705076390088e+01, 0.1581959461667e+01,
+ 0.7041664951470e-07, 0.4848356967891e+00, 0.9597935788730e-01,
+ 0.6322199535763e-07, 0.3878069473909e+01, 0.7084920306520e-01,
+ 0.5244380279191e-07, 0.2645560544125e+01, 0.5265099800692e+00,
+ 0.5143125704988e-07, 0.4834486101370e+01, 0.5328719641544e+00,
+ 0.5871866319373e-07, 0.7981472548900e+00, 0.7871412831580e-01,
+ 0.6300822573871e-07, 0.5979398788281e+01, 0.2608790314060e+02,
+ 0.6062154271548e-07, 0.4108655402756e+01, 0.1114304132498e+00,
+ 0.4361912339976e-07, 0.5322624319280e+01, 0.1375773836557e+01,
+
+ 0.4417005920067e-07, 0.6240817359284e+01, 0.2770348281756e+00,
+ 0.4686806749936e-07, 0.3214977301156e+01, 0.1143987543936e+00,
+ 0.3758892132305e-07, 0.5879809634765e+01, 0.1596186371003e+01,
+ 0.5151351332319e-07, 0.2893377688007e+00, 0.2228608264996e+00,
+ 0.4554683578572e-07, 0.5475427144122e+01, 0.1465949902372e+00,
+ 0.3442381385338e-07, 0.5992034796640e+01, 0.5070101000000e-01,
+ 0.2831093954933e-07, 0.5367350273914e+01, 0.3092784376656e+00,
+ 0.3756267090084e-07, 0.5758171285420e+01, 0.4903339079539e+00,
+ 0.2816374679892e-07, 0.1863718700923e+01, 0.2991266627620e+00,
+ 0.3419307025569e-07, 0.9524347534130e+00, 0.3518164938661e+00,
+
+ 0.2904250494239e-07, 0.5304471615602e+01, 0.1099462426779e+00,
+ 0.2471734511206e-07, 0.1297069793530e+01, 0.6256703299991e+00,
+ 0.2539620831872e-07, 0.3281126083375e+01, 0.1256615170089e+02,
+ 0.2281017868007e-07, 0.1829122133165e+01, 0.6681224869435e+01,
+ 0.2275319473335e-07, 0.5797198160181e+01, 0.3932462625300e-02,
+ 0.2547755368442e-07, 0.4752697708330e+01, 0.1169588211447e+01,
+ 0.2285979669317e-07, 0.1223205292886e+01, 0.1045155034888e+01,
+ 0.1913386560994e-07, 0.1757532993389e+01, 0.1155361302111e+01,
+ 0.1809020525147e-07, 0.4246116108791e+01, 0.3368040641550e-01,
+ 0.1649213300201e-07, 0.1445162890627e+01, 0.4408250688924e+00,
+
+ 0.1834972793932e-07, 0.1126917567225e+01, 0.4452511715700e-02,
+ 0.1439550648138e-07, 0.6160756834764e+01, 0.9420622223326e+00,
+ 0.1487645457041e-07, 0.4358761931792e+01, 0.4123712502208e+00,
+ 0.1731729516660e-07, 0.6134456753344e+01, 0.2108507877249e+00,
+ 0.1717747163567e-07, 0.1898186084455e+01, 0.2157473718317e+00,
+ 0.1418190430374e-07, 0.4180286741266e+01, 0.6521991896920e-01,
+ 0.1404844134873e-07, 0.7654053565412e-01, 0.4258542984690e-01,
+ 0.1409842846538e-07, 0.4418612420312e+01, 0.2258291676434e+00,
+ 0.1090948346291e-07, 0.1260615686131e+01, 0.4226656969313e+00,
+ 0.1357577323612e-07, 0.3558248818690e+01, 0.7923417740620e-01,
+
+ 0.1018154061960e-07, 0.5676087241256e+01, 0.1456308687557e+00,
+ 0.1412073972109e-07, 0.8394392632422e+00, 0.1525316725248e+00,
+ 0.1030938326496e-07, 0.1653593274064e+01, 0.1795258541446e+01,
+ 0.1180081567104e-07, 0.1285802592036e+01, 0.7032915397480e-01,
+ 0.9708510575650e-08, 0.7631889488106e+00, 0.8434341241180e-01,
+ 0.9637689663447e-08, 0.4630642649176e+01, 0.1272681024002e+01,
+ 0.1068910429389e-07, 0.5294934032165e+01, 0.2123349582968e+00,
+ 0.1063716179336e-07, 0.2736266800832e+01, 0.2142632012598e+00,
+ 0.1234858713814e-07, 0.1302891146570e+01, 0.1847279083684e+00,
+ 0.8912631189738e-08, 0.3570415993621e+01, 0.2648454860559e+01,
+
+ 0.1036378285534e-07, 0.4236693440949e+01, 0.1370332435159e+00,
+ 0.9667798501561e-08, 0.2960768892398e+01, 0.4376440768498e+00,
+ 0.8108314201902e-08, 0.6987781646841e+00, 0.2880807454688e+00,
+ 0.7648364324628e-08, 0.2499017863863e+01, 0.2037373330570e+00,
+ 0.7286136828406e-08, 0.3787426951665e+01, 0.1129145838217e+00,
+ 0.9448237743913e-08, 0.2694354332983e+01, 0.5272426800584e+00,
+ 0.9374276106428e-08, 0.4787121277064e+01, 0.5321392641652e+00,
+ 0.7100226287462e-08, 0.3530238792101e+00, 0.6288513220417e+00,
+ 0.9253056659571e-08, 0.1399478925664e+01, 0.1606092486742e+00,
+ 0.6636432145504e-08, 0.3479575438447e+01, 0.1368660381889e+01,
+
+ 0.6469975312932e-08, 0.1383669964800e+01, 0.2008557621224e+01,
+ 0.7335849729765e-08, 0.1243698166898e+01, 0.9561746721300e-02,
+ 0.8743421205855e-08, 0.3776164289301e+01, 0.3801276407308e+00,
+ 0.5993635744494e-08, 0.5627122113596e+01, 0.2042657109477e+02,
+ 0.5981008479693e-08, 0.1674336636752e+01, 0.2111650433779e+01,
+ 0.6188535145838e-08, 0.5214925208672e+01, 0.4305306221819e+00,
+ 0.6596074017566e-08, 0.2907653268124e+01, 0.1063314406849e+01,
+ 0.6630815126226e-08, 0.2127643669658e+01, 0.8389694097774e+00,
+ 0.6156772830040e-08, 0.5082160803295e+01, 0.4234171675140e+00,
+ 0.6446960563014e-08, 0.1872100916905e+01, 0.5287268506303e+00,
+
+ 0.6429324424668e-08, 0.5610276103577e+01, 0.5306550935933e+00,
+ 0.6302232396465e-08, 0.1592152049607e+01, 0.1253008786510e-01,
+ 0.6399244436159e-08, 0.2746214421532e+01, 0.5217580628120e+02,
+ 0.5474965172558e-08, 0.2317666374383e+01, 0.2221856701002e+01,
+ 0.5339293190692e-08, 0.1084724961156e+01, 0.7466759693650e-01,
+ 0.5334733683389e-08, 0.3594106067745e+01, 0.7489573444450e-01,
+ 0.5392665782110e-08, 0.5630254365606e+01, 0.1055449481598e+01,
+ 0.6682075673789e-08, 0.1518480041732e+01, 0.2213766559277e+00,
+ 0.5079130495960e-08, 0.2739765115711e+01, 0.2132517061319e+00,
+ 0.5077759793261e-08, 0.5290711290094e+01, 0.2133464534247e+00,
+
+ 0.4832037368310e-08, 0.1404473217200e+01, 0.7160067364790e-01,
+ 0.6463279674802e-08, 0.6038381695210e+01, 0.2209183458640e-01,
+ 0.6240592771560e-08, 0.1290170653666e+01, 0.3306188016693e+00,
+ 0.4672013521493e-08, 0.3261895939677e+01, 0.7796265773310e-01,
+ 0.6500650750348e-08, 0.1154522312095e+01, 0.3884652414254e+00,
+ 0.6344161389053e-08, 0.6206111545062e+01, 0.7605151500000e-01,
+ 0.4682518370646e-08, 0.5409118796685e+01, 0.1073608853559e+01,
+ 0.5329460015591e-08, 0.1202985784864e+01, 0.7287631425543e+00,
+ 0.5701588675898e-08, 0.4098715257064e+01, 0.8731175355560e-01,
+ 0.6030690867211e-08, 0.4132033218460e+00, 0.9846002785331e+00,
+
+ 0.4336256312655e-08, 0.1211415991827e+01, 0.4297791515992e+00,
+ 0.4688498808975e-08, 0.3765479072409e+01, 0.2127790306879e+00,
+ 0.4675578609335e-08, 0.4265540037226e+01, 0.2138191288687e+00,
+ 0.4225578112158e-08, 0.5237566010676e+01, 0.3407705765729e+00,
+ 0.5139422230028e-08, 0.1507173079513e+01, 0.7233337363710e-01,
+ 0.4619995093571e-08, 0.9023957449848e-01, 0.8603097737811e+00,
+ 0.4494776255461e-08, 0.5414930552139e+00, 0.7381754420900e-01,
+ 0.4274026276788e-08, 0.4145735303659e+01, 0.7574578717200e-01,
+ 0.5018141789353e-08, 0.3344408829055e+01, 0.3180992042600e-02,
+ 0.4866163952181e-08, 0.3348534657607e+01, 0.7722995774390e-01,
+
+ 0.4111986020501e-08, 0.4198823597220e+00, 0.1451108196653e+00,
+ 0.3356142784950e-08, 0.5609144747180e+01, 0.1274714967946e+00,
+ 0.4070575554551e-08, 0.7028411059224e+00, 0.3503323232942e+00,
+ 0.3257451857278e-08, 0.5624697983086e+01, 0.5296435984654e+00,
+ 0.3256973703026e-08, 0.1857842076707e+01, 0.5297383457582e+00,
+ 0.3830771508640e-08, 0.4562887279931e+01, 0.9098186128426e+00,
+ 0.3725024005962e-08, 0.2358058692652e+00, 0.1084620721060e+00,
+ 0.3136763921756e-08, 0.2049731526845e+01, 0.2346394437820e+00,
+ 0.3795147256194e-08, 0.2432356296933e+00, 0.1862120789403e+00,
+ 0.2877342229911e-08, 0.5631101279387e+01, 0.1905464808669e+01,
+
+ 0.3076931798805e-08, 0.1117615737392e+01, 0.3628624111593e+00,
+ 0.2734765945273e-08, 0.5899826516955e+01, 0.2131850110243e+00,
+ 0.2733405296885e-08, 0.2130562964070e+01, 0.2134131485323e+00,
+ 0.2898552353410e-08, 0.3462387048225e+00, 0.5291709230214e+00,
+ 0.2893736103681e-08, 0.8534352781543e+00, 0.5302110212022e+00,
+ 0.3095717734137e-08, 0.2875061429041e+01, 0.2976424921901e+00,
+ 0.2636190425832e-08, 0.2242512846659e+01, 0.1485980103780e+01,
+ 0.3645512095537e-08, 0.1354016903958e+01, 0.6044726378023e+00,
+ 0.2808173547723e-08, 0.6705114365631e-01, 0.6225157782540e-01,
+ 0.2625012866888e-08, 0.4775705748482e+01, 0.5268983110410e-01,
+
+ 0.2572233995651e-08, 0.2638924216139e+01, 0.1258454114666e+01,
+ 0.2604238824792e-08, 0.4826358927373e+01, 0.2103781122809e+00,
+ 0.2596886385239e-08, 0.3200388483118e+01, 0.2162200472757e+00,
+ 0.3228057304264e-08, 0.5384848409563e+01, 0.2007689919132e+00,
+ 0.2481601798252e-08, 0.5173373487744e+01, 0.1062562936266e+01,
+ 0.2745977498864e-08, 0.6250966149853e+01, 0.5651155736444e+00,
+ 0.2669878833811e-08, 0.4906001352499e+01, 0.1400015846597e+00,
+ 0.3203986611711e-08, 0.5034333010005e+01, 0.7036329877322e+00,
+ 0.3354961227212e-08, 0.6108262423137e+01, 0.4549093064213e+00,
+ 0.2400407324558e-08, 0.2135399294955e+01, 0.2125476091956e+00,
+
+ 0.2379905859802e-08, 0.5893721933961e+01, 0.2140505503610e+00,
+ 0.2550844302187e-08, 0.3331940762063e+01, 0.1534957940063e+00,
+ 0.2268824211001e-08, 0.1843418461035e+01, 0.2235935264888e+00,
+ 0.2464700891204e-08, 0.3029548547230e+01, 0.2091065926078e+00,
+ 0.2436814726024e-08, 0.4994717970364e+01, 0.2174915669488e+00,
+ 0.2443623894745e-08, 0.2645102591375e+01, 0.1739420156204e+00,
+ 0.2318701783838e-08, 0.5700547397897e+01, 0.7530171478090e-01,
+ 0.2284448700256e-08, 0.5268898905872e+01, 0.7426161660010e-01,
+ 0.2468848123510e-08, 0.5276280575078e+01, 0.2526561439362e+00,
+ 0.2814052350303e-08, 0.6130168623475e+01, 0.5636314030725e+00,
+
+ 0.2243662755220e-08, 0.6631692457995e+00, 0.8886590321940e-01,
+ 0.2330795855941e-08, 0.2499435487702e+01, 0.1056200952181e+01,
+ 0.9757679038404e-09, 0.5796846023126e+01, 0.7826370942180e+02 };
+
+/* SSB-to-Sun, T^0, Z */
+ static const double s0z[] = {
+ 0.1181255122986e-03, 0.4607918989164e+00, 0.2132990797783e+00,
+ 0.1127777651095e-03, 0.4169146331296e+00, 0.5296909721118e+00,
+ 0.4777754401806e-04, 0.4582657007130e+01, 0.3813291813120e-01,
+ 0.1129354285772e-04, 0.5758735142480e+01, 0.7478166569050e-01,
+ -0.1149543637123e-04, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.3298730512306e-05, 0.5978801994625e+01, 0.4265981595566e+00,
+ 0.2733376706079e-05, 0.7665413691040e+00, 0.1059381944224e+01,
+ 0.9426389657270e-06, 0.3710201265838e+01, 0.2061856251104e+00,
+ 0.8187517749552e-06, 0.3390675605802e+00, 0.2204125344462e+00,
+ 0.4080447871819e-06, 0.4552296640088e+00, 0.5225775174439e+00,
+
+ 0.3169973017028e-06, 0.3445455899321e+01, 0.5368044267797e+00,
+ 0.2438098615549e-06, 0.5664675150648e+01, 0.3664874755930e-01,
+ 0.2601897517235e-06, 0.1931894095697e+01, 0.1495633313810e+00,
+ 0.2314558080079e-06, 0.3666319115574e+00, 0.3961708870310e-01,
+ 0.1962549548002e-06, 0.3167411699020e+01, 0.7626583626240e-01,
+ 0.2180518287925e-06, 0.1544420746580e+01, 0.7113454667900e-02,
+ 0.1451382442868e-06, 0.1583756740070e+01, 0.1102062672231e+00,
+ 0.1358439007389e-06, 0.5239941758280e+01, 0.6398972393349e+00,
+ 0.1050585898028e-06, 0.2266958352859e+01, 0.3163918923335e+00,
+ 0.1050029870186e-06, 0.2711495250354e+01, 0.4194847048887e+00,
+
+ 0.9934920679800e-07, 0.1116208151396e+01, 0.1589072916335e+01,
+ 0.1048395331560e-06, 0.3408619600206e+01, 0.1021328554739e+02,
+ 0.8370147196668e-07, 0.3810459401087e+01, 0.2535050500000e-01,
+ 0.7989856510998e-07, 0.3769910473647e+01, 0.7329749511860e-01,
+ 0.5441221655233e-07, 0.2416994903374e+01, 0.1030928125552e+00,
+ 0.4610812906784e-07, 0.5858503336994e+01, 0.4337116142245e+00,
+ 0.3923022803444e-07, 0.3354170010125e+00, 0.1484170571900e-02,
+ 0.2610725582128e-07, 0.5410600646324e+01, 0.6327837846670e+00,
+ 0.2455279767721e-07, 0.6120216681403e+01, 0.1162474756779e+01,
+ 0.2375530706525e-07, 0.6055443426143e+01, 0.1052268489556e+01,
+
+ 0.1782967577553e-07, 0.3146108708004e+01, 0.8460828644453e+00,
+ 0.1581687095238e-07, 0.6255496089819e+00, 0.3340612434717e+01,
+ 0.1594657672461e-07, 0.3782604300261e+01, 0.1066495398892e+01,
+ 0.1563448615040e-07, 0.1997775733196e+01, 0.2022531624851e+00,
+ 0.1463624258525e-07, 0.1736316792088e+00, 0.3516457698740e-01,
+ 0.1331585056673e-07, 0.4331941830747e+01, 0.9491756770005e+00,
+ 0.1130634557637e-07, 0.6152017751825e+01, 0.2968341143800e-02,
+ 0.1028949607145e-07, 0.2101792614637e+00, 0.2275259891141e+00,
+ 0.1024074971618e-07, 0.4071833211074e+01, 0.5070101000000e-01,
+ 0.8826956060303e-08, 0.4861633688145e+00, 0.2093666171530e+00,
+
+ 0.8572230171541e-08, 0.5268190724302e+01, 0.4110125927500e-01,
+ 0.7649332643544e-08, 0.5134543417106e+01, 0.2608790314060e+02,
+ 0.8581673291033e-08, 0.2920218146681e+01, 0.1480791608091e+00,
+ 0.8430589300938e-08, 0.3604576619108e+01, 0.2172315424036e+00,
+ 0.7776165501012e-08, 0.3772942249792e+01, 0.6373574839730e-01,
+ 0.8311070234408e-08, 0.6200412329888e+01, 0.3235053470014e+00,
+ 0.6927365212582e-08, 0.4543353113437e+01, 0.8531963191132e+00,
+ 0.6791574208598e-08, 0.2882188406238e+01, 0.7181332454670e-01,
+ 0.5593100811839e-08, 0.1776646892780e+01, 0.7429900518901e+00,
+ 0.4553381853021e-08, 0.3949617611240e+01, 0.7775000683430e-01,
+
+ 0.5758000450068e-08, 0.3859251775075e+01, 0.1990721704425e+00,
+ 0.4281283457133e-08, 0.1466294631206e+01, 0.2118763888447e+01,
+ 0.4206935661097e-08, 0.5421776011706e+01, 0.1104591729320e-01,
+ 0.4213751641837e-08, 0.3412048993322e+01, 0.2243449970715e+00,
+ 0.5310506239878e-08, 0.5421641370995e+00, 0.5154640627760e+00,
+ 0.3827450341320e-08, 0.8887314524995e+00, 0.1510475019529e+00,
+ 0.4292435241187e-08, 0.1405043757194e+01, 0.1422690933580e-01,
+ 0.3189780702289e-08, 0.1060049293445e+01, 0.1173197218910e+00,
+ 0.3226611928069e-08, 0.6270858897442e+01, 0.2164800718209e+00,
+ 0.2893897608830e-08, 0.5117563223301e+01, 0.6470106940028e+00,
+
+ 0.3239852024578e-08, 0.4079092237983e+01, 0.2101180877357e+00,
+ 0.2956892222200e-08, 0.1594917021704e+01, 0.3092784376656e+00,
+ 0.2980177912437e-08, 0.5258787667564e+01, 0.4155522422634e+00,
+ 0.3163725690776e-08, 0.3854589225479e+01, 0.8582758298370e-01,
+ 0.2662262399118e-08, 0.3561326430187e+01, 0.5257585094865e+00,
+ 0.2766689135729e-08, 0.3180732086830e+00, 0.1385174140878e+00,
+ 0.2411600278464e-08, 0.3324798335058e+01, 0.5439178814476e+00,
+ 0.2483527695131e-08, 0.4169069291947e+00, 0.5336234347371e+00,
+ 0.7788777276590e-09, 0.1900569908215e+01, 0.5217580628120e+02 };
+
+/* SSB-to-Sun, T^1, X */
+ static const double s1x[] = {
+ -0.1296310361520e-07, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.8975769009438e-08, 0.1128891609250e+01, 0.4265981595566e+00,
+ 0.7771113441307e-08, 0.2706039877077e+01, 0.2061856251104e+00,
+ 0.7538303866642e-08, 0.2191281289498e+01, 0.2204125344462e+00,
+ 0.6061384579336e-08, 0.3248167319958e+01, 0.1059381944224e+01,
+ 0.5726994235594e-08, 0.5569981398610e+01, 0.5225775174439e+00,
+ 0.5616492836424e-08, 0.5057386614909e+01, 0.5368044267797e+00,
+ 0.1010881584769e-08, 0.3473577116095e+01, 0.7113454667900e-02,
+ 0.7259606157626e-09, 0.3651858593665e+00, 0.6398972393349e+00,
+ 0.8755095026935e-09, 0.1662835408338e+01, 0.4194847048887e+00,
+
+ 0.5370491182812e-09, 0.1327673878077e+01, 0.4337116142245e+00,
+ 0.5743773887665e-09, 0.4250200846687e+01, 0.2132990797783e+00,
+ 0.4408103140300e-09, 0.3598752574277e+01, 0.1589072916335e+01,
+ 0.3101892374445e-09, 0.4887822983319e+01, 0.1052268489556e+01,
+ 0.3209453713578e-09, 0.9702272295114e+00, 0.5296909721118e+00,
+ 0.3017228286064e-09, 0.5484462275949e+01, 0.1066495398892e+01,
+ 0.3200700038601e-09, 0.2846613338643e+01, 0.1495633313810e+00,
+ 0.2137637279911e-09, 0.5692163292729e+00, 0.3163918923335e+00,
+ 0.1899686386727e-09, 0.2061077157189e+01, 0.2275259891141e+00,
+ 0.1401994545308e-09, 0.4177771136967e+01, 0.1102062672231e+00,
+
+ 0.1578057810499e-09, 0.5782460597335e+01, 0.7626583626240e-01,
+ 0.1237713253351e-09, 0.5705900866881e+01, 0.5154640627760e+00,
+ 0.1313076837395e-09, 0.5163438179576e+01, 0.3664874755930e-01,
+ 0.1184963304860e-09, 0.3054804427242e+01, 0.6327837846670e+00,
+ 0.1238130878565e-09, 0.2317292575962e+01, 0.3961708870310e-01,
+ 0.1015959527736e-09, 0.2194643645526e+01, 0.7329749511860e-01,
+ 0.9017954423714e-10, 0.2868603545435e+01, 0.1990721704425e+00,
+ 0.8668024955603e-10, 0.4923849675082e+01, 0.5439178814476e+00,
+ 0.7756083930103e-10, 0.3014334135200e+01, 0.9491756770005e+00,
+ 0.7536503401741e-10, 0.2704886279769e+01, 0.1030928125552e+00,
+
+ 0.5483308679332e-10, 0.6010983673799e+01, 0.8531963191132e+00,
+ 0.5184339620428e-10, 0.1952704573291e+01, 0.2093666171530e+00,
+ 0.5108658712030e-10, 0.2958575786649e+01, 0.2172315424036e+00,
+ 0.5019424524650e-10, 0.1736317621318e+01, 0.2164800718209e+00,
+ 0.4909312625978e-10, 0.3167216416257e+01, 0.2101180877357e+00,
+ 0.4456638901107e-10, 0.7697579923471e+00, 0.3235053470014e+00,
+ 0.4227030350925e-10, 0.3490910137928e+01, 0.6373574839730e-01,
+ 0.4095456040093e-10, 0.5178888984491e+00, 0.6470106940028e+00,
+ 0.4990537041422e-10, 0.3323887668974e+01, 0.1422690933580e-01,
+ 0.4321170010845e-10, 0.4288484987118e+01, 0.7358765972222e+00,
+
+ 0.3544072091802e-10, 0.6021051579251e+01, 0.5265099800692e+00,
+ 0.3480198638687e-10, 0.4600027054714e+01, 0.5328719641544e+00,
+ 0.3440287244435e-10, 0.4349525970742e+01, 0.8582758298370e-01,
+ 0.3330628322713e-10, 0.2347391505082e+01, 0.1104591729320e-01,
+ 0.2973060707184e-10, 0.4789409286400e+01, 0.5257585094865e+00,
+ 0.2932606766089e-10, 0.5831693799927e+01, 0.5336234347371e+00,
+ 0.2876972310953e-10, 0.2692638514771e+01, 0.1173197218910e+00,
+ 0.2827488278556e-10, 0.2056052487960e+01, 0.2022531624851e+00,
+ 0.2515028239756e-10, 0.7411863262449e+00, 0.9597935788730e-01,
+ 0.2853033744415e-10, 0.3948481024894e+01, 0.2118763888447e+01 };
+
+/* SSB-to-Sun, T^1, Y */
+ static const double s1y[] = {
+ 0.8989047573576e-08, 0.5840593672122e+01, 0.4265981595566e+00,
+ 0.7815938401048e-08, 0.1129664707133e+01, 0.2061856251104e+00,
+ 0.7550926713280e-08, 0.6196589104845e+00, 0.2204125344462e+00,
+ 0.6056556925895e-08, 0.1677494667846e+01, 0.1059381944224e+01,
+ 0.5734142698204e-08, 0.4000920852962e+01, 0.5225775174439e+00,
+ 0.5614341822459e-08, 0.3486722577328e+01, 0.5368044267797e+00,
+ 0.1028678147656e-08, 0.1877141024787e+01, 0.7113454667900e-02,
+ 0.7270792075266e-09, 0.5077167301739e+01, 0.6398972393349e+00,
+ 0.8734141726040e-09, 0.9069550282609e-01, 0.4194847048887e+00,
+ 0.5377371402113e-09, 0.6039381844671e+01, 0.4337116142245e+00,
+
+ 0.4729719431571e-09, 0.2153086311760e+01, 0.2132990797783e+00,
+ 0.4458052820973e-09, 0.5059830025565e+01, 0.5296909721118e+00,
+ 0.4406855467908e-09, 0.2027971692630e+01, 0.1589072916335e+01,
+ 0.3101659310977e-09, 0.3317677981860e+01, 0.1052268489556e+01,
+ 0.3016749232545e-09, 0.3913703482532e+01, 0.1066495398892e+01,
+ 0.3198541352656e-09, 0.1275513098525e+01, 0.1495633313810e+00,
+ 0.2142065389871e-09, 0.5301351614597e+01, 0.3163918923335e+00,
+ 0.1902615247592e-09, 0.4894943352736e+00, 0.2275259891141e+00,
+ 0.1613410990871e-09, 0.2449891130437e+01, 0.1102062672231e+00,
+ 0.1576992165097e-09, 0.4211421447633e+01, 0.7626583626240e-01,
+
+ 0.1241637259894e-09, 0.4140803368133e+01, 0.5154640627760e+00,
+ 0.1313974830355e-09, 0.3591920305503e+01, 0.3664874755930e-01,
+ 0.1181697118258e-09, 0.1506314382788e+01, 0.6327837846670e+00,
+ 0.1238239742779e-09, 0.7461405378404e+00, 0.3961708870310e-01,
+ 0.1010107068241e-09, 0.6271010795475e+00, 0.7329749511860e-01,
+ 0.9226316616509e-10, 0.1259158839583e+01, 0.1990721704425e+00,
+ 0.8664946419555e-10, 0.3353244696934e+01, 0.5439178814476e+00,
+ 0.7757230468978e-10, 0.1447677295196e+01, 0.9491756770005e+00,
+ 0.7693168628139e-10, 0.1120509896721e+01, 0.1030928125552e+00,
+ 0.5487897454612e-10, 0.4439380426795e+01, 0.8531963191132e+00,
+
+ 0.5196118677218e-10, 0.3788856619137e+00, 0.2093666171530e+00,
+ 0.5110853339935e-10, 0.1386879372016e+01, 0.2172315424036e+00,
+ 0.5027804534813e-10, 0.1647881805466e+00, 0.2164800718209e+00,
+ 0.4922485922674e-10, 0.1594315079862e+01, 0.2101180877357e+00,
+ 0.6155599524400e-10, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.4447147832161e-10, 0.5480720918976e+01, 0.3235053470014e+00,
+ 0.4144691276422e-10, 0.1931371033660e+01, 0.6373574839730e-01,
+ 0.4099950625452e-10, 0.5229611294335e+01, 0.6470106940028e+00,
+ 0.5060541682953e-10, 0.1731112486298e+01, 0.1422690933580e-01,
+ 0.4293615946300e-10, 0.2714571038925e+01, 0.7358765972222e+00,
+
+ 0.3545659845763e-10, 0.4451041444634e+01, 0.5265099800692e+00,
+ 0.3479112041196e-10, 0.3029385448081e+01, 0.5328719641544e+00,
+ 0.3438516493570e-10, 0.2778507143731e+01, 0.8582758298370e-01,
+ 0.3297341285033e-10, 0.7898709807584e+00, 0.1104591729320e-01,
+ 0.2972585818015e-10, 0.3218785316973e+01, 0.5257585094865e+00,
+ 0.2931707295017e-10, 0.4260731012098e+01, 0.5336234347371e+00,
+ 0.2897198149403e-10, 0.1120753978101e+01, 0.1173197218910e+00,
+ 0.2832293240878e-10, 0.4597682717827e+00, 0.2022531624851e+00,
+ 0.2864348326612e-10, 0.2169939928448e+01, 0.9597935788730e-01,
+ 0.2852714675471e-10, 0.2377659870578e+01, 0.2118763888447e+01 };
+
+/* SSB-to-Sun, T^1, Z */
+ static const double s1z[] = {
+ 0.5444220475678e-08, 0.1803825509310e+01, 0.2132990797783e+00,
+ 0.3883412695596e-08, 0.4668616389392e+01, 0.5296909721118e+00,
+ 0.1334341434551e-08, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.3730001266883e-09, 0.5401405918943e+01, 0.2061856251104e+00,
+ 0.2894929197956e-09, 0.4932415609852e+01, 0.2204125344462e+00,
+ 0.2857950357701e-09, 0.3154625362131e+01, 0.7478166569050e-01,
+ 0.2499226432292e-09, 0.3657486128988e+01, 0.4265981595566e+00,
+ 0.1937705443593e-09, 0.5740434679002e+01, 0.1059381944224e+01,
+ 0.1374894396320e-09, 0.1712857366891e+01, 0.5368044267797e+00,
+ 0.1217248678408e-09, 0.2312090870932e+01, 0.5225775174439e+00,
+
+ 0.7961052740870e-10, 0.5283368554163e+01, 0.3813291813120e-01,
+ 0.4979225949689e-10, 0.4298290471860e+01, 0.4194847048887e+00,
+ 0.4388552286597e-10, 0.6145515047406e+01, 0.7113454667900e-02,
+ 0.2586835212560e-10, 0.3019448001809e+01, 0.6398972393349e+00 };
+
+/* SSB-to-Sun, T^2, X */
+ static const double s2x[] = {
+ 0.1603551636587e-11, 0.4404109410481e+01, 0.2061856251104e+00,
+ 0.1556935889384e-11, 0.4818040873603e+00, 0.2204125344462e+00,
+ 0.1182594414915e-11, 0.9935762734472e+00, 0.5225775174439e+00,
+ 0.1158794583180e-11, 0.3353180966450e+01, 0.5368044267797e+00,
+ 0.9597358943932e-12, 0.5567045358298e+01, 0.2132990797783e+00,
+ 0.6511516579605e-12, 0.5630872420788e+01, 0.4265981595566e+00,
+ 0.7419792747688e-12, 0.2156188581957e+01, 0.5296909721118e+00,
+ 0.3951972655848e-12, 0.1981022541805e+01, 0.1059381944224e+01,
+ 0.4478223877045e-12, 0.0000000000000e+00, 0.0000000000000e+00 };
+
+/* SSB-to-Sun, T^2, Y */
+ static const double s2y[] = {
+ 0.1609114495091e-11, 0.2831096993481e+01, 0.2061856251104e+00,
+ 0.1560330784946e-11, 0.5193058213906e+01, 0.2204125344462e+00,
+ 0.1183535479202e-11, 0.5707003443890e+01, 0.5225775174439e+00,
+ 0.1158183066182e-11, 0.1782400404928e+01, 0.5368044267797e+00,
+ 0.1032868027407e-11, 0.4036925452011e+01, 0.2132990797783e+00,
+ 0.6540142847741e-12, 0.4058241056717e+01, 0.4265981595566e+00,
+ 0.7305236491596e-12, 0.6175401942957e+00, 0.5296909721118e+00,
+ -0.5580725052968e-12, 0.0000000000000e+00, 0.0000000000000e+00,
+ 0.3946122651015e-12, 0.4108265279171e+00, 0.1059381944224e+01 };
+
+/* SSB-to-Sun, T^2, Z */
+ static const double s2z[] = {
+ 0.3749920358054e-12, 0.3230285558668e+01, 0.2132990797783e+00,
+ 0.2735037220939e-12, 0.6154322683046e+01, 0.5296909721118e+00 };
+
+/* Pointers to coefficient arrays, in x,y,z sets */
+ static const double *ce0[] = { e0x, e0y, e0z },
+ *ce1[] = { e1x, e1y, e1z },
+ *ce2[] = { e2x, e2y, e2z },
+ *cs0[] = { s0x, s0y, s0z },
+ *cs1[] = { s1x, s1y, s1z },
+ *cs2[] = { s2x, s2y, s2z };
+ const double *coeffs;
+
+/* Numbers of terms for each component of the model, in x,y,z sets */
+ static const int ne0[3] = {(int)(sizeof e0x / sizeof (double) / 3),
+ (int)(sizeof e0y / sizeof (double) / 3),
+ (int)(sizeof e0z / sizeof (double) / 3) },
+ ne1[3] = {(int)(sizeof e1x / sizeof (double) / 3),
+ (int)(sizeof e1y / sizeof (double) / 3),
+ (int)(sizeof e1z / sizeof (double) / 3) },
+ ne2[3] = {(int)(sizeof e2x / sizeof (double) / 3),
+ (int)(sizeof e2y / sizeof (double) / 3),
+ (int)(sizeof e2z / sizeof (double) / 3) },
+ ns0[3] = {(int)(sizeof s0x / sizeof (double) / 3),
+ (int)(sizeof s0y / sizeof (double) / 3),
+ (int)(sizeof s0z / sizeof (double) / 3) },
+ ns1[3] = {(int)(sizeof s1x / sizeof (double) / 3),
+ (int)(sizeof s1y / sizeof (double) / 3),
+ (int)(sizeof s1z / sizeof (double) / 3) },
+ ns2[3] = {(int)(sizeof s2x / sizeof (double) / 3),
+ (int)(sizeof s2y / sizeof (double) / 3),
+ (int)(sizeof s2z / sizeof (double) / 3) };
+ int nterms;
+
+/* Miscellaneous */
+ int jstat, i, j;
+ double t, t2, xyz, xyzd, a, b, c, ct, p, cp,
+ ph[3], vh[3], pb[3], vb[3], x, y, z;
+
+/*--------------------------------------------------------------------*/
+
+/* Time since reference epoch, Julian years. */
+ t = ((date1 - DJ00) + date2) / DJY;
+ t2 = t*t;
+
+/* Set status. */
+ jstat = fabs(t) <= 100.0 ? 0 : 1;
+
+/* X then Y then Z. */
+ for (i = 0; i < 3; i++) {
+
+ /* Initialize position and velocity component. */
+ xyz = 0.0;
+ xyzd = 0.0;
+
+ /* ------------------------------------------------ */
+ /* Obtain component of Sun to Earth ecliptic vector */
+ /* ------------------------------------------------ */
+
+ /* Sun to Earth, T^0 terms. */
+ coeffs = ce0[i];
+ nterms = ne0[i];
+ for (j = 0; j < nterms; j++) {
+ a = *coeffs++;
+ b = *coeffs++;
+ c = *coeffs++;
+ p = b + c*t;
+ xyz += a*cos(p);
+ xyzd -= a*c*sin(p);
+ }
+
+ /* Sun to Earth, T^1 terms. */
+ coeffs = ce1[i];
+ nterms = ne1[i];
+ for (j = 0; j < nterms; j++) {
+ a = *coeffs++;
+ b = *coeffs++;
+ c = *coeffs++;
+ ct = c*t;
+ p = b + ct;
+ cp = cos(p);
+ xyz += a*t*cp;
+ xyzd += a*( cp - ct*sin(p) );
+ }
+
+ /* Sun to Earth, T^2 terms. */
+ coeffs = ce2[i];
+ nterms = ne2[i];
+ for (j = 0; j < nterms; j++) {
+ a = *coeffs++;
+ b = *coeffs++;
+ c = *coeffs++;
+ ct = c*t;
+ p = b + ct;
+ cp = cos(p);
+ xyz += a*t2*cp;
+ xyzd += a*t*( 2.0*cp - ct*sin(p) );
+ }
+
+ /* Heliocentric Earth position and velocity component. */
+ ph[i] = xyz;
+ vh[i] = xyzd / DJY;
+
+ /* ------------------------------------------------ */
+ /* Obtain component of SSB to Earth ecliptic vector */
+ /* ------------------------------------------------ */
+
+ /* SSB to Sun, T^0 terms. */
+ coeffs = cs0[i];
+ nterms = ns0[i];
+ for (j = 0; j < nterms; j++) {
+ a = *coeffs++;
+ b = *coeffs++;
+ c = *coeffs++;
+ p = b + c*t;
+ xyz += a*cos(p);
+ xyzd -= a*c*sin(p);
+ }
+
+ /* SSB to Sun, T^1 terms. */
+ coeffs = cs1[i];
+ nterms = ns1[i];
+ for (j = 0; j < nterms; j++) {
+ a = *coeffs++;
+ b = *coeffs++;
+ c = *coeffs++;
+ ct = c*t;
+ p = b + ct;
+ cp = cos(p);
+ xyz += a*t*cp;
+ xyzd += a*(cp - ct*sin(p));
+ }
+
+ /* SSB to Sun, T^2 terms. */
+ coeffs = cs2[i];
+ nterms = ns2[i];
+ for (j = 0; j < nterms; j++) {
+ a = *coeffs++;
+ b = *coeffs++;
+ c = *coeffs++;
+ ct = c*t;
+ p = b + ct;
+ cp = cos(p);
+ xyz += a*t2*cp;
+ xyzd += a*t*(2.0*cp - ct*sin(p));
+ }
+
+ /* Barycentric Earth position and velocity component. */
+ pb[i] = xyz;
+ vb[i] = xyzd / DJY;
+
+ /* Next Cartesian component. */
+ }
+
+/* Rotate from ecliptic to BCRS coordinates. */
+
+ x = ph[0];
+ y = ph[1];
+ z = ph[2];
+ pvh[0][0] = x + am12*y + am13*z;
+ pvh[0][1] = am21*x + am22*y + am23*z;
+ pvh[0][2] = am32*y + am33*z;
+
+ x = vh[0];
+ y = vh[1];
+ z = vh[2];
+ pvh[1][0] = x + am12*y + am13*z;
+ pvh[1][1] = am21*x + am22*y + am23*z;
+ pvh[1][2] = am32*y + am33*z;
+
+ x = pb[0];
+ y = pb[1];
+ z = pb[2];
+ pvb[0][0] = x + am12*y + am13*z;
+ pvb[0][1] = am21*x + am22*y + am23*z;
+ pvb[0][2] = am32*y + am33*z;
+
+ x = vb[0];
+ y = vb[1];
+ z = vb[2];
+ pvb[1][0] = x + am12*y + am13*z;
+ pvb[1][1] = am21*x + am22*y + am23*z;
+ pvb[1][2] = am32*y + am33*z;
+
+/* Return the status. */
+ return jstat;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/eqeq94.c b/sofa/eqeq94.c
new file mode 100644
index 0000000..0b7e05c
--- /dev/null
+++ b/sofa/eqeq94.c
@@ -0,0 +1,181 @@
+#include "sofam.h"
+
+double iauEqeq94(double date1, double date2)
+/*
+** - - - - - - - - - -
+** i a u E q e q 9 4
+** - - - - - - - - - -
+**
+** Equation of the equinoxes, IAU 1994 model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TDB date (Note 1)
+**
+** Returned (function value):
+** double equation of the equinoxes (Note 2)
+**
+** Notes:
+**
+** 1) The date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The result, which is in radians, operates in the following sense:
+**
+** Greenwich apparent ST = GMST + equation of the equinoxes
+**
+** Called:
+** iauNut80 nutation, IAU 1980
+** iauObl80 mean obliquity, IAU 1980
+**
+** References:
+**
+** IAU Resolution C7, Recommendation 3 (1994).
+**
+** Capitaine, N. & Gontier, A.-M., 1993, Astron. Astrophys., 275,
+** 645-650.
+**
+** This revision: 2008 May 24
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t, om, dpsi, deps, eps0, ee;
+
+
+/* Interval between fundamental epoch J2000.0 and given date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* Longitude of the mean ascending node of the lunar orbit on the */
+/* ecliptic, measured from the mean equinox of date. */
+ om = iauAnpm((450160.280 + (-482890.539
+ + (7.455 + 0.008 * t) * t) * t) * DAS2R
+ + fmod(-5.0 * t, 1.0) * D2PI);
+
+/* Nutation components and mean obliquity. */
+ iauNut80(date1, date2, &dpsi, &deps);
+ eps0 = iauObl80(date1, date2);
+
+/* Equation of the equinoxes. */
+ ee = dpsi*cos(eps0) + DAS2R*(0.00264*sin(om) + 0.000063*sin(om+om));
+
+ return ee;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/era00.c b/sofa/era00.c
new file mode 100644
index 0000000..ab24fee
--- /dev/null
+++ b/sofa/era00.c
@@ -0,0 +1,186 @@
+#include "sofam.h"
+
+double iauEra00(double dj1, double dj2)
+/*
+** - - - - - - - - -
+** i a u E r a 0 0
+** - - - - - - - - -
+**
+** Earth rotation angle (IAU 2000 model).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** dj1,dj2 double UT1 as a 2-part Julian Date (see note)
+**
+** Returned (function value):
+** double Earth rotation angle (radians), range 0-2pi
+**
+** Notes:
+**
+** 1) The UT1 date dj1+dj2 is a Julian Date, apportioned in any
+** convenient way between the arguments dj1 and dj2. For example,
+** JD(UT1)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** dj1 dj2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 and MJD methods are good compromises
+** between resolution and convenience. The date & time method is
+** best matched to the algorithm used: maximum precision is
+** delivered when the dj1 argument is for 0hrs UT1 on the day in
+** question and the dj2 argument lies in the range 0 to 1, or vice
+** versa.
+**
+** 2) The algorithm is adapted from Expression 22 of Capitaine et al.
+** 2000. The time argument has been expressed in days directly,
+** and, to retain precision, integer contributions have been
+** eliminated. The same formulation is given in IERS Conventions
+** (2003), Chap. 5, Eq. 14.
+**
+** Called:
+** iauAnp normalize angle into range 0 to 2pi
+**
+** References:
+**
+** Capitaine N., Guinot B. and McCarthy D.D, 2000, Astron.
+** Astrophys., 355, 398-405.
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2008 May 24
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double d1, d2, t, f, theta;
+
+
+/* Days since fundamental epoch. */
+ if (dj1 < dj2) {
+ d1 = dj1;
+ d2 = dj2;
+ } else {
+ d1 = dj2;
+ d2 = dj1;
+ }
+ t = d1 + (d2- DJ00);
+
+/* Fractional part of T (days). */
+ f = fmod(d1, 1.0) + fmod(d2, 1.0);
+
+/* Earth rotation angle at this UT1. */
+ theta = iauAnp(D2PI * (f + 0.7790572732640
+ + 0.00273781191135448 * t));
+
+ return theta;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fad03.c b/sofa/fad03.c
new file mode 100644
index 0000000..30a336a
--- /dev/null
+++ b/sofa/fad03.c
@@ -0,0 +1,153 @@
+#include "sofam.h"
+
+double iauFad03(double t)
+/*
+** - - - - - - - - -
+** i a u F a d 0 3
+** - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean elongation of the Moon from the Sun.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double D, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** is from Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean elongation of the Moon from the Sun (IERS Conventions 2003). */
+ a = fmod( 1072260.703692 +
+ t * ( 1602961601.2090 +
+ t * ( - 6.3706 +
+ t * ( 0.006593 +
+ t * ( - 0.00003169 ) ) ) ), TURNAS ) * DAS2R;
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fae03.c b/sofa/fae03.c
new file mode 100644
index 0000000..73efe65
--- /dev/null
+++ b/sofa/fae03.c
@@ -0,0 +1,152 @@
+#include "sofam.h"
+
+double iauFae03(double t)
+/*
+** - - - - - - - - -
+** i a u F a e 0 3
+** - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean longitude of Earth.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double mean longitude of Earth, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** comes from Souchay et al. (1999) after Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** Souchay, J., Loysel, B., Kinoshita, H., Folgueira, M. 1999,
+** Astron.Astrophys.Supp.Ser. 135, 111
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean longitude of Earth (IERS Conventions 2003). */
+ a = fmod(1.753470314 + 628.3075849991 * t, D2PI);
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/faf03.c b/sofa/faf03.c
new file mode 100644
index 0000000..3a5cd61
--- /dev/null
+++ b/sofa/faf03.c
@@ -0,0 +1,156 @@
+#include "sofam.h"
+
+double iauFaf03(double t)
+/*
+** - - - - - - - - -
+** i a u F a f 0 3
+** - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean longitude of the Moon minus mean longitude of the ascending
+** node.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double F, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** is from Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean longitude of the Moon minus that of the ascending node */
+/* (IERS Conventions 2003). */
+ a = fmod( 335779.526232 +
+ t * ( 1739527262.8478 +
+ t * ( - 12.7512 +
+ t * ( - 0.001037 +
+ t * ( 0.00000417 ) ) ) ), TURNAS ) * DAS2R;
+
+ return a;
+
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/faju03.c b/sofa/faju03.c
new file mode 100644
index 0000000..d815e63
--- /dev/null
+++ b/sofa/faju03.c
@@ -0,0 +1,152 @@
+#include "sofam.h"
+
+double iauFaju03(double t)
+/*
+** - - - - - - - - - -
+** i a u F a j u 0 3
+** - - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean longitude of Jupiter.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double mean longitude of Jupiter, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** comes from Souchay et al. (1999) after Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** Souchay, J., Loysel, B., Kinoshita, H., Folgueira, M. 1999,
+** Astron.Astrophys.Supp.Ser. 135, 111
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean longitude of Jupiter (IERS Conventions 2003). */
+ a = fmod(0.599546497 + 52.9690962641 * t, D2PI);
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fal03.c b/sofa/fal03.c
new file mode 100644
index 0000000..48987e9
--- /dev/null
+++ b/sofa/fal03.c
@@ -0,0 +1,153 @@
+#include "sofam.h"
+
+double iauFal03(double t)
+/*
+** - - - - - - - - -
+** i a u F a l 0 3
+** - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean anomaly of the Moon.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double l, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** is from Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean anomaly of the Moon (IERS Conventions 2003). */
+ a = fmod( 485868.249036 +
+ t * ( 1717915923.2178 +
+ t * ( 31.8792 +
+ t * ( 0.051635 +
+ t * ( - 0.00024470 ) ) ) ), TURNAS ) * DAS2R;
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/falp03.c b/sofa/falp03.c
new file mode 100644
index 0000000..cde82d5
--- /dev/null
+++ b/sofa/falp03.c
@@ -0,0 +1,153 @@
+#include "sofam.h"
+
+double iauFalp03(double t)
+/*
+** - - - - - - - - - -
+** i a u F a l p 0 3
+** - - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean anomaly of the Sun.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double l', radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** is from Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean anomaly of the Sun (IERS Conventions 2003). */
+ a = fmod( 1287104.793048 +
+ t * ( 129596581.0481 +
+ t * ( - 0.5532 +
+ t * ( 0.000136 +
+ t * ( - 0.00001149 ) ) ) ), TURNAS ) * DAS2R;
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fama03.c b/sofa/fama03.c
new file mode 100644
index 0000000..78c8c20
--- /dev/null
+++ b/sofa/fama03.c
@@ -0,0 +1,152 @@
+#include "sofam.h"
+
+double iauFama03(double t)
+/*
+** - - - - - - - - - -
+** i a u F a m a 0 3
+** - - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean longitude of Mars.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double mean longitude of Mars, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** comes from Souchay et al. (1999) after Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** Souchay, J., Loysel, B., Kinoshita, H., Folgueira, M. 1999,
+** Astron.Astrophys.Supp.Ser. 135, 111
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean longitude of Mars (IERS Conventions 2003). */
+ a = fmod(6.203480913 + 334.0612426700 * t, D2PI);
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fame03.c b/sofa/fame03.c
new file mode 100644
index 0000000..80d2c3b
--- /dev/null
+++ b/sofa/fame03.c
@@ -0,0 +1,152 @@
+#include "sofam.h"
+
+double iauFame03(double t)
+/*
+** - - - - - - - - - -
+** i a u F a m e 0 3
+** - - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean longitude of Mercury.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double mean longitude of Mercury, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** comes from Souchay et al. (1999) after Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** Souchay, J., Loysel, B., Kinoshita, H., Folgueira, M. 1999,
+** Astron.Astrophys.Supp.Ser. 135, 111
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean longitude of Mercury (IERS Conventions 2003). */
+ a = fmod(4.402608842 + 2608.7903141574 * t, D2PI);
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fane03.c b/sofa/fane03.c
new file mode 100644
index 0000000..a6e1870
--- /dev/null
+++ b/sofa/fane03.c
@@ -0,0 +1,149 @@
+#include "sofam.h"
+
+double iauFane03(double t)
+/*
+** - - - - - - - - - -
+** i a u F a n e 0 3
+** - - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean longitude of Neptune.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double mean longitude of Neptune, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** is adapted from Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean longitude of Neptune (IERS Conventions 2003). */
+ a = fmod(5.311886287 + 3.8133035638 * t, D2PI);
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/faom03.c b/sofa/faom03.c
new file mode 100644
index 0000000..ab47ec4
--- /dev/null
+++ b/sofa/faom03.c
@@ -0,0 +1,154 @@
+#include "sofam.h"
+
+double iauFaom03(double t)
+/*
+** - - - - - - - - - -
+** i a u F a o m 0 3
+** - - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean longitude of the Moon's ascending node.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double Omega, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** is from Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean longitude of the Moon's ascending node */
+/* (IERS Conventions 2003). */
+ a = fmod( 450160.398036 +
+ t * ( - 6962890.5431 +
+ t * ( 7.4722 +
+ t * ( 0.007702 +
+ t * ( - 0.00005939 ) ) ) ), TURNAS ) * DAS2R;
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fapa03.c b/sofa/fapa03.c
new file mode 100644
index 0000000..d8d9b5c
--- /dev/null
+++ b/sofa/fapa03.c
@@ -0,0 +1,153 @@
+#include "sofam.h"
+
+double iauFapa03(double t)
+/*
+** - - - - - - - - - -
+** i a u F a p a 0 3
+** - - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** general accumulated precession in longitude.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double general precession in longitude, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003). It
+** is taken from Kinoshita & Souchay (1990) and comes originally
+** from Lieske et al. (1977).
+**
+** References:
+**
+** Kinoshita, H. and Souchay J. 1990, Celest.Mech. and Dyn.Astron.
+** 48, 187
+**
+** Lieske, J.H., Lederle, T., Fricke, W. & Morando, B. 1977,
+** Astron.Astrophys. 58, 1-16
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* General accumulated precession in longitude. */
+ a = (0.024381750 + 0.00000538691 * t) * t;
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fasa03.c b/sofa/fasa03.c
new file mode 100644
index 0000000..5ee3097
--- /dev/null
+++ b/sofa/fasa03.c
@@ -0,0 +1,152 @@
+#include "sofam.h"
+
+double iauFasa03(double t)
+/*
+** - - - - - - - - - -
+** i a u F a s a 0 3
+** - - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean longitude of Saturn.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double mean longitude of Saturn, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** comes from Souchay et al. (1999) after Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** Souchay, J., Loysel, B., Kinoshita, H., Folgueira, M. 1999,
+** Astron.Astrophys.Supp.Ser. 135, 111
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean longitude of Saturn (IERS Conventions 2003). */
+ a = fmod(0.874016757 + 21.3299104960 * t, D2PI);
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/faur03.c b/sofa/faur03.c
new file mode 100644
index 0000000..821bf56
--- /dev/null
+++ b/sofa/faur03.c
@@ -0,0 +1,149 @@
+#include "sofam.h"
+
+double iauFaur03(double t)
+/*
+** - - - - - - - - - -
+** i a u F a u r 0 3
+** - - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean longitude of Uranus.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double mean longitude of Uranus, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** is adapted from Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean longitude of Uranus (IERS Conventions 2003). */
+ a = fmod(5.481293872 + 7.4781598567 * t, D2PI);
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fave03.c b/sofa/fave03.c
new file mode 100644
index 0000000..6cf1003
--- /dev/null
+++ b/sofa/fave03.c
@@ -0,0 +1,152 @@
+#include "sofam.h"
+
+double iauFave03(double t)
+/*
+** - - - - - - - - - -
+** i a u F a v e 0 3
+** - - - - - - - - - -
+**
+** Fundamental argument, IERS Conventions (2003):
+** mean longitude of Venus.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** t double TDB, Julian centuries since J2000.0 (Note 1)
+**
+** Returned (function value):
+** double mean longitude of Venus, radians (Note 2)
+**
+** Notes:
+**
+** 1) Though t is strictly TDB, it is usually more convenient to use
+** TT, which makes no significant difference.
+**
+** 2) The expression used is as adopted in IERS Conventions (2003) and
+** comes from Souchay et al. (1999) after Simon et al. (1994).
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** Souchay, J., Loysel, B., Kinoshita, H., Folgueira, M. 1999,
+** Astron.Astrophys.Supp.Ser. 135, 111
+**
+** This revision: 2009 December 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double a;
+
+
+/* Mean longitude of Venus (IERS Conventions 2003). */
+ a = fmod(3.176146697 + 1021.3285546211 * t, D2PI);
+
+ return a;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fk52h.c b/sofa/fk52h.c
new file mode 100644
index 0000000..7b34315
--- /dev/null
+++ b/sofa/fk52h.c
@@ -0,0 +1,193 @@
+#include "sofam.h"
+
+void iauFk52h(double r5, double d5,
+ double dr5, double dd5, double px5, double rv5,
+ double *rh, double *dh,
+ double *drh, double *ddh, double *pxh, double *rvh)
+/*
+** - - - - - - - - -
+** i a u F k 5 2 h
+** - - - - - - - - -
+**
+** Transform FK5 (J2000.0) star data into the Hipparcos system.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given (all FK5, equinox J2000.0, epoch J2000.0):
+** r5 double RA (radians)
+** d5 double Dec (radians)
+** dr5 double proper motion in RA (dRA/dt, rad/Jyear)
+** dd5 double proper motion in Dec (dDec/dt, rad/Jyear)
+** px5 double parallax (arcsec)
+** rv5 double radial velocity (km/s, positive = receding)
+**
+** Returned (all Hipparcos, epoch J2000.0):
+** rh double RA (radians)
+** dh double Dec (radians)
+** drh double proper motion in RA (dRA/dt, rad/Jyear)
+** ddh double proper motion in Dec (dDec/dt, rad/Jyear)
+** pxh double parallax (arcsec)
+** rvh double radial velocity (km/s, positive = receding)
+**
+** Notes:
+**
+** 1) This function transforms FK5 star positions and proper motions
+** into the system of the Hipparcos catalog.
+**
+** 2) The proper motions in RA are dRA/dt rather than
+** cos(Dec)*dRA/dt, and are per year rather than per century.
+**
+** 3) The FK5 to Hipparcos transformation is modeled as a pure
+** rotation and spin; zonal errors in the FK5 catalog are not
+** taken into account.
+**
+** 4) See also iauH2fk5, iauFk5hz, iauHfk5z.
+**
+** Called:
+** iauStarpv star catalog data to space motion pv-vector
+** iauFk5hip FK5 to Hipparcos rotation and spin
+** iauRxp product of r-matrix and p-vector
+** iauPxp vector product of two p-vectors
+** iauPpp p-vector plus p-vector
+** iauPvstar space motion pv-vector to star catalog data
+**
+** Reference:
+**
+** F.Mignard & M.Froeschle, Astron. Astrophys. 354, 732-739 (2000).
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int i;
+ double pv5[2][3], r5h[3][3], s5h[3], wxp[3], vv[3], pvh[2][3];
+
+
+/* FK5 barycentric position/velocity pv-vector (normalized). */
+ iauStarpv(r5, d5, dr5, dd5, px5, rv5, pv5);
+
+/* FK5 to Hipparcos orientation matrix and spin vector. */
+ iauFk5hip(r5h, s5h);
+
+/* Make spin units per day instead of per year. */
+ for ( i = 0; i < 3; s5h[i++] /= 365.25 );
+
+/* Orient the FK5 position into the Hipparcos system. */
+ iauRxp(r5h, pv5[0], pvh[0]);
+
+/* Apply spin to the position giving an extra space motion component. */
+ iauPxp(pv5[0], s5h, wxp);
+
+/* Add this component to the FK5 space motion. */
+ iauPpp(wxp, pv5[1], vv);
+
+/* Orient the FK5 space motion into the Hipparcos system. */
+ iauRxp(r5h, vv, pvh[1]);
+
+/* Hipparcos pv-vector to spherical. */
+ iauPvstar(pvh, rh, dh, drh, ddh, pxh, rvh);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fk5hip.c b/sofa/fk5hip.c
new file mode 100644
index 0000000..d96b732
--- /dev/null
+++ b/sofa/fk5hip.c
@@ -0,0 +1,176 @@
+#include "sofam.h"
+
+void iauFk5hip(double r5h[3][3], double s5h[3])
+/*
+** - - - - - - - - - -
+** i a u F k 5 h i p
+** - - - - - - - - - -
+**
+** FK5 to Hipparcos rotation and spin.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Returned:
+** r5h double[3][3] r-matrix: FK5 rotation wrt Hipparcos (Note 2)
+** s5h double[3] r-vector: FK5 spin wrt Hipparcos (Note 3)
+**
+** Notes:
+**
+** 1) This function models the FK5 to Hipparcos transformation as a
+** pure rotation and spin; zonal errors in the FK5 catalogue are
+** not taken into account.
+**
+** 2) The r-matrix r5h operates in the sense:
+**
+** P_Hipparcos = r5h x P_FK5
+**
+** where P_FK5 is a p-vector in the FK5 frame, and P_Hipparcos is
+** the equivalent Hipparcos p-vector.
+**
+** 3) The r-vector s5h represents the time derivative of the FK5 to
+** Hipparcos rotation. The units are radians per year (Julian,
+** TDB).
+**
+** Called:
+** iauRv2m r-vector to r-matrix
+**
+** Reference:
+**
+** F.Mignard & M.Froeschle, Astron. Astrophys. 354, 732-739 (2000).
+**
+** This revision: 2009 March 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double v[3];
+
+/* FK5 wrt Hipparcos orientation and spin (radians, radians/year) */
+ double epx, epy, epz;
+ double omx, omy, omz;
+
+
+ epx = -19.9e-3 * DAS2R;
+ epy = -9.1e-3 * DAS2R;
+ epz = 22.9e-3 * DAS2R;
+
+ omx = -0.30e-3 * DAS2R;
+ omy = 0.60e-3 * DAS2R;
+ omz = 0.70e-3 * DAS2R;
+
+/* FK5 to Hipparcos orientation expressed as an r-vector. */
+ v[0] = epx;
+ v[1] = epy;
+ v[2] = epz;
+
+/* Re-express as an r-matrix. */
+ iauRv2m(v, r5h);
+
+/* Hipparcos wrt FK5 spin expressed as an r-vector. */
+ s5h[0] = omx;
+ s5h[1] = omy;
+ s5h[2] = omz;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fk5hz.c b/sofa/fk5hz.c
new file mode 100644
index 0000000..45f96a4
--- /dev/null
+++ b/sofa/fk5hz.c
@@ -0,0 +1,210 @@
+#include "sofam.h"
+
+void iauFk5hz(double r5, double d5, double date1, double date2,
+ double *rh, double *dh)
+/*
+** - - - - - - - - -
+** i a u F k 5 h z
+** - - - - - - - - -
+**
+** Transform an FK5 (J2000.0) star position into the system of the
+** Hipparcos catalogue, assuming zero Hipparcos proper motion.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** r5 double FK5 RA (radians), equinox J2000.0, at date
+** d5 double FK5 Dec (radians), equinox J2000.0, at date
+** date1,date2 double TDB date (Notes 1,2)
+**
+** Returned:
+** rh double Hipparcos RA (radians)
+** dh double Hipparcos Dec (radians)
+**
+** Notes:
+**
+** 1) This function converts a star position from the FK5 system to
+** the Hipparcos system, in such a way that the Hipparcos proper
+** motion is zero. Because such a star has, in general, a non-zero
+** proper motion in the FK5 system, the function requires the date
+** at which the position in the FK5 system was determined.
+**
+** 2) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 3) The FK5 to Hipparcos transformation is modeled as a pure
+** rotation and spin; zonal errors in the FK5 catalogue are not
+** taken into account.
+**
+** 4) The position returned by this function is in the Hipparcos
+** reference system but at date date1+date2.
+**
+** 5) See also iauFk52h, iauH2fk5, iauHfk5z.
+**
+** Called:
+** iauS2c spherical coordinates to unit vector
+** iauFk5hip FK5 to Hipparcos rotation and spin
+** iauSxp multiply p-vector by scalar
+** iauRv2m r-vector to r-matrix
+** iauTrxp product of transpose of r-matrix and p-vector
+** iauPxp vector product of two p-vectors
+** iauC2s p-vector to spherical
+** iauAnp normalize angle into range 0 to 2pi
+**
+** Reference:
+**
+** F.Mignard & M.Froeschle, 2000, Astron.Astrophys. 354, 732-739.
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t, p5e[3], r5h[3][3], s5h[3], vst[3], rst[3][3], p5[3],
+ ph[3], w;
+
+
+/* Interval from given date to fundamental epoch J2000.0 (JY). */
+ t = - ((date1 - DJ00) + date2) / DJY;
+
+/* FK5 barycentric position vector. */
+ iauS2c(r5, d5, p5e);
+
+/* FK5 to Hipparcos orientation matrix and spin vector. */
+ iauFk5hip(r5h, s5h);
+
+/* Accumulated Hipparcos wrt FK5 spin over that interval. */
+ iauSxp(t, s5h, vst);
+
+/* Express the accumulated spin as a rotation matrix. */
+ iauRv2m(vst, rst);
+
+/* Derotate the vector's FK5 axes back to date. */
+ iauTrxp(rst, p5e, p5);
+
+/* Rotate the vector into the Hipparcos system. */
+ iauRxp(r5h, p5, ph);
+
+/* Hipparcos vector to spherical. */
+ iauC2s(ph, &w, dh);
+ *rh = iauAnp(w);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fw2m.c b/sofa/fw2m.c
new file mode 100644
index 0000000..caef4bc
--- /dev/null
+++ b/sofa/fw2m.c
@@ -0,0 +1,184 @@
+#include "sofam.h"
+
+void iauFw2m(double gamb, double phib, double psi, double eps,
+ double r[3][3])
+/*
+** - - - - - - - -
+** i a u F w 2 m
+** - - - - - - - -
+**
+** Form rotation matrix given the Fukushima-Williams angles.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** gamb double F-W angle gamma_bar (radians)
+** phib double F-W angle phi_bar (radians)
+** psi double F-W angle psi (radians)
+** eps double F-W angle epsilon (radians)
+**
+** Returned:
+** r double[3][3] rotation matrix
+**
+** Notes:
+**
+** 1) Naming the following points:
+**
+** e = J2000.0 ecliptic pole,
+** p = GCRS pole,
+** E = ecliptic pole of date,
+** and P = CIP,
+**
+** the four Fukushima-Williams angles are as follows:
+**
+** gamb = gamma = epE
+** phib = phi = pE
+** psi = psi = pEP
+** eps = epsilon = EP
+**
+** 2) The matrix representing the combined effects of frame bias,
+** precession and nutation is:
+**
+** NxPxB = R_1(-eps).R_3(-psi).R_1(phib).R_3(gamb)
+**
+** 3) Three different matrices can be constructed, depending on the
+** supplied angles:
+**
+** o To obtain the nutation x precession x frame bias matrix,
+** generate the four precession angles, generate the nutation
+** components and add them to the psi_bar and epsilon_A angles,
+** and call the present function.
+**
+** o To obtain the precession x frame bias matrix, generate the
+** four precession angles and call the present function.
+**
+** o To obtain the frame bias matrix, generate the four precession
+** angles for date J2000.0 and call the present function.
+**
+** The nutation-only and precession-only matrices can if necessary
+** be obtained by combining these three appropriately.
+**
+** Called:
+** iauIr initialize r-matrix to identity
+** iauRz rotate around Z-axis
+** iauRx rotate around X-axis
+**
+** Reference:
+**
+** Hilton, J. et al., 2006, Celest.Mech.Dyn.Astron. 94, 351
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Construct the matrix. */
+ iauIr(r);
+ iauRz(gamb, r);
+ iauRx(phib, r);
+ iauRz(-psi, r);
+ iauRx(-eps, r);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/fw2xy.c b/sofa/fw2xy.c
new file mode 100644
index 0000000..caaf49c
--- /dev/null
+++ b/sofa/fw2xy.c
@@ -0,0 +1,170 @@
+#include "sofam.h"
+
+void iauFw2xy(double gamb, double phib, double psi, double eps,
+ double *x, double *y)
+/*
+** - - - - - - - - -
+** i a u F w 2 x y
+** - - - - - - - - -
+**
+** CIP X,Y given Fukushima-Williams bias-precession-nutation angles.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** gamb double F-W angle gamma_bar (radians)
+** phib double F-W angle phi_bar (radians)
+** psi double F-W angle psi (radians)
+** eps double F-W angle epsilon (radians)
+**
+** Returned:
+** x,y double CIP X,Y ("radians")
+**
+** Notes:
+**
+** 1) Naming the following points:
+**
+** e = J2000.0 ecliptic pole,
+** p = GCRS pole
+** E = ecliptic pole of date,
+** and P = CIP,
+**
+** the four Fukushima-Williams angles are as follows:
+**
+** gamb = gamma = epE
+** phib = phi = pE
+** psi = psi = pEP
+** eps = epsilon = EP
+**
+** 2) The matrix representing the combined effects of frame bias,
+** precession and nutation is:
+**
+** NxPxB = R_1(-epsA).R_3(-psi).R_1(phib).R_3(gamb)
+**
+** X,Y are elements (3,1) and (3,2) of the matrix.
+**
+** Called:
+** iauFw2m F-W angles to r-matrix
+** iauBpn2xy extract CIP X,Y coordinates from NPB matrix
+**
+** Reference:
+**
+** Hilton, J. et al., 2006, Celest.Mech.Dyn.Astron. 94, 351
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double r[3][3];
+
+
+/* Form NxPxB matrix. */
+ iauFw2m(gamb, phib, psi, eps, r);
+
+/* Extract CIP X,Y. */
+ iauBpn2xy(r, x, y);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/gc2gd.c b/sofa/gc2gd.c
new file mode 100644
index 0000000..e4f5c38
--- /dev/null
+++ b/sofa/gc2gd.c
@@ -0,0 +1,184 @@
+#include "sofam.h"
+
+int iauGc2gd ( int n, double xyz[3],
+ double *elong, double *phi, double *height )
+/*
+** - - - - - - - - -
+** i a u G c 2 g d
+** - - - - - - - - -
+**
+** Transform geocentric coordinates to geodetic using the specified
+** reference ellipsoid.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical transformation.
+**
+** Given:
+** n int ellipsoid identifier (Note 1)
+** xyz double[3] geocentric vector (Note 2)
+**
+** Returned:
+** elong double longitude (radians, east +ve)
+** phi double latitude (geodetic, radians, Note 3)
+** height double height above ellipsoid (geodetic, Notes 2,3)
+**
+** Returned (function value):
+** int status: 0 = OK
+** -1 = illegal identifier (Note 3)
+** -2 = internal error (Note 3)
+**
+** Notes:
+**
+** 1) The identifier n is a number that specifies the choice of
+** reference ellipsoid. The following are supported:
+**
+** n ellipsoid
+**
+** 1 WGS84
+** 2 GRS80
+** 3 WGS72
+**
+** The n value has no significance outside the SOFA software. For
+** convenience, symbols WGS84 etc. are defined in sofam.h.
+**
+** 2) The geocentric vector (xyz, given) and height (height, returned)
+** are in meters.
+**
+** 3) An error status -1 means that the identifier n is illegal. An
+** error status -2 is theoretically impossible. In all error cases,
+** phi and height are both set to -1e9.
+**
+** 4) The inverse transformation is performed in the function iauGd2gc.
+**
+** Called:
+** iauEform Earth reference ellipsoids
+** iauGc2gde geocentric to geodetic transformation, general
+**
+** This revision: 2012 Febuary 23
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int j;
+ double a, f;
+
+
+/* Obtain reference ellipsoid parameters. */
+ j = iauEform ( n, &a, &f );
+
+/* If OK, transform x,y,z to longitude, geodetic latitude, height. */
+ if ( j == 0 ) {
+ j = iauGc2gde ( a, f, xyz, elong, phi, height );
+ if ( j < 0 ) j = -2;
+ }
+
+/* Deal with any errors. */
+ if ( j < 0 ) {
+ *phi = -1e9;
+ *height = -1e9;
+ }
+
+/* Return the status. */
+ return j;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+
+}
diff --git a/sofa/gc2gde.c b/sofa/gc2gde.c
new file mode 100644
index 0000000..359ef76
--- /dev/null
+++ b/sofa/gc2gde.c
@@ -0,0 +1,250 @@
+#include "sofam.h"
+
+int iauGc2gde ( double a, double f, double xyz[3],
+ double *elong, double *phi, double *height )
+/*
+** - - - - - - - - - -
+** i a u G c 2 g d e
+** - - - - - - - - - -
+**
+** Transform geocentric coordinates to geodetic for a reference
+** ellipsoid of specified form.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** a double equatorial radius (Notes 2,4)
+** f double flattening (Note 3)
+** xyz double[3] geocentric vector (Note 4)
+**
+** Returned:
+** elong double longitude (radians, east +ve)
+** phi double latitude (geodetic, radians)
+** height double height above ellipsoid (geodetic, Note 4)
+**
+** Returned (function value):
+** int status: 0 = OK
+** -1 = illegal f
+** -2 = illegal a
+**
+** Notes:
+**
+** 1) This function is based on the GCONV2H Fortran subroutine by
+** Toshio Fukushima (see reference).
+**
+** 2) The equatorial radius, a, can be in any units, but meters is
+** the conventional choice.
+**
+** 3) The flattening, f, is (for the Earth) a value around 0.00335,
+** i.e. around 1/298.
+**
+** 4) The equatorial radius, a, and the geocentric vector, xyz,
+** must be given in the same units, and determine the units of
+** the returned height, height.
+**
+** 5) If an error occurs (status < 0), elong, phi and height are
+** unchanged.
+**
+** 6) The inverse transformation is performed in the function
+** iauGd2gce.
+**
+** 7) The transformation for a standard ellipsoid (such as WGS84) can
+** more conveniently be performed by calling iauGc2gd, which uses a
+** numerical code to identify the required A and F values.
+**
+** Reference:
+**
+** Fukushima, T., "Transformation from Cartesian to geodetic
+** coordinates accelerated by Halley's method", J.Geodesy (2006)
+** 79: 689-693
+**
+** This revision: 2012 February 23
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double aeps2, e2, e4t, ec2, ec, b, x, y, z, p2, absz, p, s0, pn, zc,
+ c0, c02, c03, s02, s03, a02, a0, a03, d0, f0, b0, s1,
+ cc, s12, cc2;
+
+
+/* ------------- */
+/* Preliminaries */
+/* ------------- */
+
+/* Validate ellipsoid parameters. */
+ if ( f < 0.0 || f >= 1.0 ) return -1;
+ if ( a <= 0.0 ) return -2;
+
+/* Functions of ellipsoid parameters (with further validation of f). */
+ aeps2 = a*a * 1e-32;
+ e2 = (2.0 - f) * f;
+ e4t = e2*e2 * 1.5;
+ ec2 = 1.0 - e2;
+ if ( ec2 <= 0.0 ) return -1;
+ ec = sqrt(ec2);
+ b = a * ec;
+
+/* Cartesian components. */
+ x = xyz[0];
+ y = xyz[1];
+ z = xyz[2];
+
+/* Distance from polar axis squared. */
+ p2 = x*x + y*y;
+
+/* Longitude. */
+ *elong = p2 != 0.0 ? atan2(y, x) : 0.0;
+
+/* Unsigned z-coordinate. */
+ absz = fabs(z);
+
+/* Proceed unless polar case. */
+ if ( p2 > aeps2 ) {
+
+ /* Distance from polar axis. */
+ p = sqrt(p2);
+
+ /* Normalization. */
+ s0 = absz / a;
+ pn = p / a;
+ zc = ec * s0;
+
+ /* Prepare Newton correction factors. */
+ c0 = ec * pn;
+ c02 = c0 * c0;
+ c03 = c02 * c0;
+ s02 = s0 * s0;
+ s03 = s02 * s0;
+ a02 = c02 + s02;
+ a0 = sqrt(a02);
+ a03 = a02 * a0;
+ d0 = zc*a03 + e2*s03;
+ f0 = pn*a03 - e2*c03;
+
+ /* Prepare Halley correction factor. */
+ b0 = e4t * s02 * c02 * pn * (a0 - ec);
+ s1 = d0*f0 - b0*s0;
+ cc = ec * (f0*f0 - b0*c0);
+
+ /* Evaluate latitude and height. */
+ *phi = atan(s1/cc);
+ s12 = s1 * s1;
+ cc2 = cc * cc;
+ *height = (p*cc + absz*s1 - a * sqrt(ec2*s12 + cc2)) /
+ sqrt(s12 + cc2);
+ } else {
+
+ /* Exception: pole. */
+ *phi = DPI / 2.0;
+ *height = absz - b;
+ }
+
+/* Restore sign of latitude. */
+ if ( z < 0 ) *phi = -*phi;
+
+/* OK status. */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+
+}
diff --git a/sofa/gd2gc.c b/sofa/gd2gc.c
new file mode 100644
index 0000000..5483059
--- /dev/null
+++ b/sofa/gd2gc.c
@@ -0,0 +1,184 @@
+#include "sofam.h"
+
+int iauGd2gc ( int n, double elong, double phi, double height,
+ double xyz[3] )
+/*
+** - - - - - - - - -
+** i a u G d 2 g c
+** - - - - - - - - -
+**
+** Transform geodetic coordinates to geocentric using the specified
+** reference ellipsoid.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical transformation.
+**
+** Given:
+** n int ellipsoid identifier (Note 1)
+** elong double longitude (radians, east +ve)
+** phi double latitude (geodetic, radians, Note 3)
+** height double height above ellipsoid (geodetic, Notes 2,3)
+**
+** Returned:
+** xyz double[3] geocentric vector (Note 2)
+**
+** Returned (function value):
+** int status: 0 = OK
+** -1 = illegal identifier (Note 3)
+** -2 = illegal case (Note 3)
+**
+** Notes:
+**
+** 1) The identifier n is a number that specifies the choice of
+** reference ellipsoid. The following are supported:
+**
+** n ellipsoid
+**
+** 1 WGS84
+** 2 GRS80
+** 3 WGS72
+**
+** The n value has no significance outside the SOFA software. For
+** convenience, symbols WGS84 etc. are defined in sofam.h.
+**
+** 2) The height (height, given) and the geocentric vector (xyz,
+** returned) are in meters.
+**
+** 3) No validation is performed on the arguments elong, phi and
+** height. An error status -1 means that the identifier n is
+** illegal. An error status -2 protects against cases that would
+** lead to arithmetic exceptions. In all error cases, xyz is set
+** to zeros.
+**
+** 4) The inverse transformation is performed in the function iauGc2gd.
+**
+** Called:
+** iauEform Earth reference ellipsoids
+** iauGd2gce geodetic to geocentric transformation, general
+** iauZp zero p-vector
+**
+** This revision: 2012 February 23
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int j;
+ double a, f;
+
+
+/* Obtain reference ellipsoid parameters. */
+ j = iauEform ( n, &a, &f );
+
+/* If OK, transform longitude, geodetic latitude, height to x,y,z. */
+ if ( j == 0 ) {
+ j = iauGd2gce ( a, f, elong, phi, height, xyz );
+ if ( j != 0 ) j = -2;
+ }
+
+/* Deal with any errors. */
+ if ( j != 0 ) iauZp ( xyz );
+
+/* Return the status. */
+ return j;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+
+}
diff --git a/sofa/gd2gce.c b/sofa/gd2gce.c
new file mode 100644
index 0000000..a745d3c
--- /dev/null
+++ b/sofa/gd2gce.c
@@ -0,0 +1,188 @@
+#include "sofam.h"
+
+int iauGd2gce ( double a, double f, double elong, double phi,
+ double height, double xyz[3] )
+/*
+** - - - - - - - - - -
+** i a u G d 2 g c e
+** - - - - - - - - - -
+**
+** Transform geodetic coordinates to geocentric for a reference
+** ellipsoid of specified form.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** a double equatorial radius (Notes 1,4)
+** f double flattening (Notes 2,4)
+** elong double longitude (radians, east +ve)
+** phi double latitude (geodetic, radians, Note 4)
+** height double height above ellipsoid (geodetic, Notes 3,4)
+**
+** Returned:
+** xyz double[3] geocentric vector (Note 3)
+**
+** Returned (function value):
+** int status: 0 = OK
+** -1 = illegal case (Note 4)
+** Notes:
+**
+** 1) The equatorial radius, a, can be in any units, but meters is
+** the conventional choice.
+**
+** 2) The flattening, f, is (for the Earth) a value around 0.00335,
+** i.e. around 1/298.
+**
+** 3) The equatorial radius, a, and the height, height, must be
+** given in the same units, and determine the units of the
+** returned geocentric vector, xyz.
+**
+** 4) No validation is performed on individual arguments. The error
+** status -1 protects against (unrealistic) cases that would lead
+** to arithmetic exceptions. If an error occurs, xyz is unchanged.
+**
+** 5) The inverse transformation is performed in the function
+** iauGc2gde.
+**
+** 6) The transformation for a standard ellipsoid (such as WGS84) can
+** more conveniently be performed by calling iauGd2gc, which uses a
+** numerical code to identify the required a and f values.
+**
+** References:
+**
+** Green, R.M., Spherical Astronomy, Cambridge University Press,
+** (1985) Section 4.5, p96.
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992),
+** Section 4.22, p202.
+**
+** This revision: 2012 February 23
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double sp, cp, w, d, ac, as, r;
+
+
+/* Functions of geodetic latitude. */
+ sp = sin(phi);
+ cp = cos(phi);
+ w = 1.0 - f;
+ w = w * w;
+ d = cp*cp + w*sp*sp;
+ if ( d <= 0.0 ) return -1;
+ ac = a / sqrt(d);
+ as = w * ac;
+
+/* Geocentric vector. */
+ r = (ac + height) * cp;
+ xyz[0] = r * cos(elong);
+ xyz[1] = r * sin(elong);
+ xyz[2] = (as + height) * sp;
+
+/* Success. */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+
+}
diff --git a/sofa/gmst00.c b/sofa/gmst00.c
new file mode 100644
index 0000000..23ae265
--- /dev/null
+++ b/sofa/gmst00.c
@@ -0,0 +1,195 @@
+#include "sofam.h"
+
+double iauGmst00(double uta, double utb, double tta, double ttb)
+/*
+** - - - - - - - - - -
+** i a u G m s t 0 0
+** - - - - - - - - - -
+**
+** Greenwich mean sidereal time (model consistent with IAU 2000
+** resolutions).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** uta,utb double UT1 as a 2-part Julian Date (Notes 1,2)
+** tta,ttb double TT as a 2-part Julian Date (Notes 1,2)
+**
+** Returned (function value):
+** double Greenwich mean sidereal time (radians)
+**
+** Notes:
+**
+** 1) The UT1 and TT dates uta+utb and tta+ttb respectively, are both
+** Julian Dates, apportioned in any convenient way between the
+** argument pairs. For example, JD=2450123.7 could be expressed in
+** any of these ways, among others:
+**
+** Part A Part B
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable (in the case of UT; the TT is not at all critical
+** in this respect). The J2000 and MJD methods are good compromises
+** between resolution and convenience. For UT, the date & time
+** method is best matched to the algorithm that is used by the Earth
+** Rotation Angle function, called internally: maximum precision is
+** delivered when the uta argument is for 0hrs UT1 on the day in
+** question and the utb argument lies in the range 0 to 1, or vice
+** versa.
+**
+** 2) Both UT1 and TT are required, UT1 to predict the Earth rotation
+** and TT to predict the effects of precession. If UT1 is used for
+** both purposes, errors of order 100 microarcseconds result.
+**
+** 3) This GMST is compatible with the IAU 2000 resolutions and must be
+** used only in conjunction with other IAU 2000 compatible
+** components such as precession-nutation and equation of the
+** equinoxes.
+**
+** 4) The result is returned in the range 0 to 2pi.
+**
+** 5) The algorithm is from Capitaine et al. (2003) and IERS
+** Conventions 2003.
+**
+** Called:
+** iauEra00 Earth rotation angle, IAU 2000
+** iauAnp normalize angle into range 0 to 2pi
+**
+** References:
+**
+** Capitaine, N., Wallace, P.T. and McCarthy, D.D., "Expressions to
+** implement the IAU 2000 definition of UT1", Astronomy &
+** Astrophysics, 406, 1135-1149 (2003)
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2009 March 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t, gmst;
+
+
+/* TT Julian centuries since J2000.0. */
+ t = ((tta - DJ00) + ttb) / DJC;
+
+/* Greenwich Mean Sidereal Time, IAU 2000. */
+ gmst = iauAnp(iauEra00(uta, utb) +
+ ( 0.014506 +
+ ( 4612.15739966 +
+ ( 1.39667721 +
+ ( -0.00009344 +
+ ( 0.00001882 )
+ * t) * t) * t) * t) * DAS2R);
+
+ return gmst;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/gmst06.c b/sofa/gmst06.c
new file mode 100644
index 0000000..619569f
--- /dev/null
+++ b/sofa/gmst06.c
@@ -0,0 +1,186 @@
+#include "sofam.h"
+
+double iauGmst06(double uta, double utb, double tta, double ttb)
+/*
+** - - - - - - - - - -
+** i a u G m s t 0 6
+** - - - - - - - - - -
+**
+** Greenwich mean sidereal time (consistent with IAU 2006 precession).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** uta,utb double UT1 as a 2-part Julian Date (Notes 1,2)
+** tta,ttb double TT as a 2-part Julian Date (Notes 1,2)
+**
+** Returned (function value):
+** double Greenwich mean sidereal time (radians)
+**
+** Notes:
+**
+** 1) The UT1 and TT dates uta+utb and tta+ttb respectively, are both
+** Julian Dates, apportioned in any convenient way between the
+** argument pairs. For example, JD=2450123.7 could be expressed in
+** any of these ways, among others:
+**
+** Part A Part B
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable (in the case of UT; the TT is not at all critical
+** in this respect). The J2000 and MJD methods are good compromises
+** between resolution and convenience. For UT, the date & time
+** method is best matched to the algorithm that is used by the Earth
+** rotation angle function, called internally: maximum precision is
+** delivered when the uta argument is for 0hrs UT1 on the day in
+** question and the utb argument lies in the range 0 to 1, or vice
+** versa.
+**
+** 2) Both UT1 and TT are required, UT1 to predict the Earth rotation
+** and TT to predict the effects of precession. If UT1 is used for
+** both purposes, errors of order 100 microarcseconds result.
+**
+** 3) This GMST is compatible with the IAU 2006 precession and must not
+** be used with other precession models.
+**
+** 4) The result is returned in the range 0 to 2pi.
+**
+** Called:
+** iauEra00 Earth rotation angle, IAU 2000
+** iauAnp normalize angle into range 0 to 2pi
+**
+** Reference:
+**
+** Capitaine, N., Wallace, P.T. & Chapront, J., 2005,
+** Astron.Astrophys. 432, 355
+**
+** This revision: 2008 May 24
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t, gmst;
+
+
+/* TT Julian centuries since J2000.0. */
+ t = ((tta - DJ00) + ttb) / DJC;
+
+/* Greenwich mean sidereal time, IAU 2006. */
+ gmst = iauAnp(iauEra00(uta, utb) +
+ ( 0.014506 +
+ ( 4612.156534 +
+ ( 1.3915817 +
+ ( -0.00000044 +
+ ( -0.000029956 +
+ ( -0.0000000368 )
+ * t) * t) * t) * t) * t) * DAS2R);
+
+ return gmst;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/gmst82.c b/sofa/gmst82.c
new file mode 100644
index 0000000..cd7e4e1
--- /dev/null
+++ b/sofa/gmst82.c
@@ -0,0 +1,201 @@
+#include "sofam.h"
+
+double iauGmst82(double dj1, double dj2)
+/*
+** - - - - - - - - - -
+** i a u G m s t 8 2
+** - - - - - - - - - -
+**
+** Universal Time to Greenwich mean sidereal time (IAU 1982 model).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** dj1,dj2 double UT1 Julian Date (see note)
+**
+** Returned (function value):
+** double Greenwich mean sidereal time (radians)
+**
+** Notes:
+**
+** 1) The UT1 date dj1+dj2 is a Julian Date, apportioned in any
+** convenient way between the arguments dj1 and dj2. For example,
+** JD(UT1)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** dj1 dj2
+**
+** 2450123.7D0 0D0 (JD method)
+** 2451545D0 -1421.3D0 (J2000 method)
+** 2400000.5D0 50123.2D0 (MJD method)
+** 2450123.5D0 0.2D0 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 and MJD methods are good compromises
+** between resolution and convenience. The date & time method is
+** best matched to the algorithm used: maximum accuracy (or, at
+** least, minimum noise) is delivered when the dj1 argument is for
+** 0hrs UT1 on the day in question and the dj2 argument lies in the
+** range 0 to 1, or vice versa.
+**
+** 2) The algorithm is based on the IAU 1982 expression. This is
+** always described as giving the GMST at 0 hours UT1. In fact, it
+** gives the difference between the GMST and the UT, the steady
+** 4-minutes-per-day drawing-ahead of ST with respect to UT. When
+** whole days are ignored, the expression happens to equal the GMST
+** at 0 hours UT1 each day.
+**
+** 3) In this function, the entire UT1 (the sum of the two arguments
+** dj1 and dj2) is used directly as the argument for the standard
+** formula, the constant term of which is adjusted by 12 hours to
+** take account of the noon phasing of Julian Date. The UT1 is then
+** added, but omitting whole days to conserve accuracy.
+**
+** Called:
+** iauAnp normalize angle into range 0 to 2pi
+**
+** References:
+**
+** Transactions of the International Astronomical Union,
+** XVIII B, 67 (1983).
+**
+** Aoki et al., Astron. Astrophys. 105, 359-361 (1982).
+**
+** This revision: 2008 May 24
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Coefficients of IAU 1982 GMST-UT1 model */
+ double A = 24110.54841 - DAYSEC / 2.0;
+ double B = 8640184.812866;
+ double C = 0.093104;
+ double D = -6.2e-6;
+
+/* Note: the first constant, A, has to be adjusted by 12 hours */
+/* because the UT1 is supplied as a Julian date, which begins */
+/* at noon. */
+
+ double d1, d2, t, f, gmst;
+
+
+/* Julian centuries since fundamental epoch. */
+ if (dj1 < dj2) {
+ d1 = dj1;
+ d2 = dj2;
+ } else {
+ d1 = dj2;
+ d2 = dj1;
+ }
+ t = (d1 + (d2 - DJ00)) / DJC;
+
+/* Fractional part of JD(UT1), in seconds. */
+ f = DAYSEC * (fmod(d1, 1.0) + fmod(d2, 1.0));
+
+/* GMST at this UT1. */
+ gmst = iauAnp(DS2R * ((A + (B + (C + D * t) * t) * t) + f));
+
+ return gmst;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/gst00a.c b/sofa/gst00a.c
new file mode 100644
index 0000000..6f50c14
--- /dev/null
+++ b/sofa/gst00a.c
@@ -0,0 +1,188 @@
+#include "sofam.h"
+
+double iauGst00a(double uta, double utb, double tta, double ttb)
+/*
+** - - - - - - - - - -
+** i a u G s t 0 0 a
+** - - - - - - - - - -
+**
+** Greenwich apparent sidereal time (consistent with IAU 2000
+** resolutions).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** uta,utb double UT1 as a 2-part Julian Date (Notes 1,2)
+** tta,ttb double TT as a 2-part Julian Date (Notes 1,2)
+**
+** Returned (function value):
+** double Greenwich apparent sidereal time (radians)
+**
+** Notes:
+**
+** 1) The UT1 and TT dates uta+utb and tta+ttb respectively, are both
+** Julian Dates, apportioned in any convenient way between the
+** argument pairs. For example, JD=2450123.7 could be expressed in
+** any of these ways, among others:
+**
+** Part A Part B
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable (in the case of UT; the TT is not at all critical
+** in this respect). The J2000 and MJD methods are good compromises
+** between resolution and convenience. For UT, the date & time
+** method is best matched to the algorithm that is used by the Earth
+** Rotation Angle function, called internally: maximum precision is
+** delivered when the uta argument is for 0hrs UT1 on the day in
+** question and the utb argument lies in the range 0 to 1, or vice
+** versa.
+**
+** 2) Both UT1 and TT are required, UT1 to predict the Earth rotation
+** and TT to predict the effects of precession-nutation. If UT1 is
+** used for both purposes, errors of order 100 microarcseconds
+** result.
+**
+** 3) This GAST is compatible with the IAU 2000 resolutions and must be
+** used only in conjunction with other IAU 2000 compatible
+** components such as precession-nutation.
+**
+** 4) The result is returned in the range 0 to 2pi.
+**
+** 5) The algorithm is from Capitaine et al. (2003) and IERS
+** Conventions 2003.
+**
+** Called:
+** iauGmst00 Greenwich mean sidereal time, IAU 2000
+** iauEe00a equation of the equinoxes, IAU 2000A
+** iauAnp normalize angle into range 0 to 2pi
+**
+** References:
+**
+** Capitaine, N., Wallace, P.T. and McCarthy, D.D., "Expressions to
+** implement the IAU 2000 definition of UT1", Astronomy &
+** Astrophysics, 406, 1135-1149 (2003)
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2008 May 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double gmst00, ee00a, gst;
+
+
+ gmst00 = iauGmst00(uta, utb, tta, ttb);
+ ee00a = iauEe00a(tta, ttb);
+ gst = iauAnp(gmst00 + ee00a);
+
+ return gst;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/gst00b.c b/sofa/gst00b.c
new file mode 100644
index 0000000..66b8e3d
--- /dev/null
+++ b/sofa/gst00b.c
@@ -0,0 +1,196 @@
+#include "sofam.h"
+
+double iauGst00b(double uta, double utb)
+/*
+** - - - - - - - - - -
+** i a u G s t 0 0 b
+** - - - - - - - - - -
+**
+** Greenwich apparent sidereal time (consistent with IAU 2000
+** resolutions but using the truncated nutation model IAU 2000B).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** uta,utb double UT1 as a 2-part Julian Date (Notes 1,2)
+**
+** Returned (function value):
+** double Greenwich apparent sidereal time (radians)
+**
+** Notes:
+**
+** 1) The UT1 date uta+utb is a Julian Date, apportioned in any
+** convenient way between the argument pair. For example,
+** JD=2450123.7 could be expressed in any of these ways, among
+** others:
+**
+** uta utb
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in cases
+** where the loss of several decimal digits of resolution is
+** acceptable. The J2000 and MJD methods are good compromises
+** between resolution and convenience. For UT, the date & time
+** method is best matched to the algorithm that is used by the Earth
+** Rotation Angle function, called internally: maximum precision is
+** delivered when the uta argument is for 0hrs UT1 on the day in
+** question and the utb argument lies in the range 0 to 1, or vice
+** versa.
+**
+** 2) The result is compatible with the IAU 2000 resolutions, except
+** that accuracy has been compromised for the sake of speed and
+** convenience in two respects:
+**
+** . UT is used instead of TDB (or TT) to compute the precession
+** component of GMST and the equation of the equinoxes. This
+** results in errors of order 0.1 mas at present.
+**
+** . The IAU 2000B abridged nutation model (McCarthy & Luzum, 2001)
+** is used, introducing errors of up to 1 mas.
+**
+** 3) This GAST is compatible with the IAU 2000 resolutions and must be
+** used only in conjunction with other IAU 2000 compatible
+** components such as precession-nutation.
+**
+** 4) The result is returned in the range 0 to 2pi.
+**
+** 5) The algorithm is from Capitaine et al. (2003) and IERS
+** Conventions 2003.
+**
+** Called:
+** iauGmst00 Greenwich mean sidereal time, IAU 2000
+** iauEe00b equation of the equinoxes, IAU 2000B
+** iauAnp normalize angle into range 0 to 2pi
+**
+** References:
+**
+** Capitaine, N., Wallace, P.T. and McCarthy, D.D., "Expressions to
+** implement the IAU 2000 definition of UT1", Astronomy &
+** Astrophysics, 406, 1135-1149 (2003)
+**
+** McCarthy, D.D. & Luzum, B.J., "An abridged model of the
+** precession-nutation of the celestial pole", Celestial Mechanics &
+** Dynamical Astronomy, 85, 37-49 (2003)
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2008 May 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double gmst00, ee00b, gst;
+
+
+ gmst00 = iauGmst00(uta, utb, uta, utb);
+ ee00b = iauEe00b(uta, utb);
+ gst = iauAnp(gmst00 + ee00b);
+
+ return gst;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/gst06.c b/sofa/gst06.c
new file mode 100644
index 0000000..3c35e74
--- /dev/null
+++ b/sofa/gst06.c
@@ -0,0 +1,190 @@
+#include "sofam.h"
+
+double iauGst06(double uta, double utb, double tta, double ttb,
+ double rnpb[3][3])
+/*
+** - - - - - - - - -
+** i a u G s t 0 6
+** - - - - - - - - -
+**
+** Greenwich apparent sidereal time, IAU 2006, given the NPB matrix.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** uta,utb double UT1 as a 2-part Julian Date (Notes 1,2)
+** tta,ttb double TT as a 2-part Julian Date (Notes 1,2)
+** rnpb double[3][3] nutation x precession x bias matrix
+**
+** Returned (function value):
+** double Greenwich apparent sidereal time (radians)
+**
+** Notes:
+**
+** 1) The UT1 and TT dates uta+utb and tta+ttb respectively, are both
+** Julian Dates, apportioned in any convenient way between the
+** argument pairs. For example, JD=2450123.7 could be expressed in
+** any of these ways, among others:
+**
+** Part A Part B
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable (in the case of UT; the TT is not at all critical
+** in this respect). The J2000 and MJD methods are good compromises
+** between resolution and convenience. For UT, the date & time
+** method is best matched to the algorithm that is used by the Earth
+** rotation angle function, called internally: maximum precision is
+** delivered when the uta argument is for 0hrs UT1 on the day in
+** question and the utb argument lies in the range 0 to 1, or vice
+** versa.
+**
+** 2) Both UT1 and TT are required, UT1 to predict the Earth rotation
+** and TT to predict the effects of precession-nutation. If UT1 is
+** used for both purposes, errors of order 100 microarcseconds
+** result.
+**
+** 3) Although the function uses the IAU 2006 series for s+XY/2, it is
+** otherwise independent of the precession-nutation model and can in
+** practice be used with any equinox-based NPB matrix.
+**
+** 4) The result is returned in the range 0 to 2pi.
+**
+** Called:
+** iauBpn2xy extract CIP X,Y coordinates from NPB matrix
+** iauS06 the CIO locator s, given X,Y, IAU 2006
+** iauAnp normalize angle into range 0 to 2pi
+** iauEra00 Earth rotation angle, IAU 2000
+** iauEors equation of the origins, given NPB matrix and s
+**
+** Reference:
+**
+** Wallace, P.T. & Capitaine, N., 2006, Astron.Astrophys. 459, 981
+**
+** This revision: 2008 May 24
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double x, y, s, era, eors, gst;
+
+
+/* Extract CIP coordinates. */
+ iauBpn2xy(rnpb, &x, &y);
+
+/* The CIO locator, s. */
+ s = iauS06(tta, ttb, x, y);
+
+/* Greenwich apparent sidereal time. */
+ era = iauEra00(uta, utb);
+ eors = iauEors(rnpb, s);
+ gst = iauAnp(era - eors);
+
+ return gst;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/gst06a.c b/sofa/gst06a.c
new file mode 100644
index 0000000..7b5c542
--- /dev/null
+++ b/sofa/gst06a.c
@@ -0,0 +1,181 @@
+#include "sofam.h"
+
+double iauGst06a(double uta, double utb, double tta, double ttb)
+/*
+** - - - - - - - - - -
+** i a u G s t 0 6 a
+** - - - - - - - - - -
+**
+** Greenwich apparent sidereal time (consistent with IAU 2000 and 2006
+** resolutions).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** uta,utb double UT1 as a 2-part Julian Date (Notes 1,2)
+** tta,ttb double TT as a 2-part Julian Date (Notes 1,2)
+**
+** Returned (function value):
+** double Greenwich apparent sidereal time (radians)
+**
+** Notes:
+**
+** 1) The UT1 and TT dates uta+utb and tta+ttb respectively, are both
+** Julian Dates, apportioned in any convenient way between the
+** argument pairs. For example, JD=2450123.7 could be expressed in
+** any of these ways, among others:
+**
+** Part A Part B
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable (in the case of UT; the TT is not at all critical
+** in this respect). The J2000 and MJD methods are good compromises
+** between resolution and convenience. For UT, the date & time
+** method is best matched to the algorithm that is used by the Earth
+** rotation angle function, called internally: maximum precision is
+** delivered when the uta argument is for 0hrs UT1 on the day in
+** question and the utb argument lies in the range 0 to 1, or vice
+** versa.
+**
+** 2) Both UT1 and TT are required, UT1 to predict the Earth rotation
+** and TT to predict the effects of precession-nutation. If UT1 is
+** used for both purposes, errors of order 100 microarcseconds
+** result.
+**
+** 3) This GAST is compatible with the IAU 2000/2006 resolutions and
+** must be used only in conjunction with IAU 2006 precession and
+** IAU 2000A nutation.
+**
+** 4) The result is returned in the range 0 to 2pi.
+**
+** Called:
+** iauPnm06a classical NPB matrix, IAU 2006/2000A
+** iauGst06 Greenwich apparent ST, IAU 2006, given NPB matrix
+**
+** Reference:
+**
+** Wallace, P.T. & Capitaine, N., 2006, Astron.Astrophys. 459, 981
+**
+** This revision: 2008 May 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rnpb[3][3], gst;
+
+
+/* Classical nutation x precession x bias matrix, IAU 2000A. */
+ iauPnm06a(tta, ttb, rnpb);
+
+/* Greenwich apparent sidereal time. */
+ gst = iauGst06(uta, utb, tta, ttb, rnpb);
+
+ return gst;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/gst94.c b/sofa/gst94.c
new file mode 100644
index 0000000..652f99f
--- /dev/null
+++ b/sofa/gst94.c
@@ -0,0 +1,181 @@
+#include "sofa.h"
+
+double iauGst94(double uta, double utb)
+/*
+** - - - - - - - - -
+** i a u G s t 9 4
+** - - - - - - - - -
+**
+** Greenwich apparent sidereal time (consistent with IAU 1982/94
+** resolutions).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** uta,utb double UT1 as a 2-part Julian Date (Notes 1,2)
+**
+** Returned (function value):
+** double Greenwich apparent sidereal time (radians)
+**
+** Notes:
+**
+** 1) The UT1 date uta+utb is a Julian Date, apportioned in any
+** convenient way between the argument pair. For example,
+** JD=2450123.7 could be expressed in any of these ways, among
+** others:
+**
+** uta utb
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in cases
+** where the loss of several decimal digits of resolution is
+** acceptable. The J2000 and MJD methods are good compromises
+** between resolution and convenience. For UT, the date & time
+** method is best matched to the algorithm that is used by the Earth
+** Rotation Angle function, called internally: maximum precision is
+** delivered when the uta argument is for 0hrs UT1 on the day in
+** question and the utb argument lies in the range 0 to 1, or vice
+** versa.
+**
+** 2) The result is compatible with the IAU 1982 and 1994 resolutions,
+** except that accuracy has been compromised for the sake of
+** convenience in that UT is used instead of TDB (or TT) to compute
+** the equation of the equinoxes.
+**
+** 3) This GAST must be used only in conjunction with contemporaneous
+** IAU standards such as 1976 precession, 1980 obliquity and 1982
+** nutation. It is not compatible with the IAU 2000 resolutions.
+**
+** 4) The result is returned in the range 0 to 2pi.
+**
+** Called:
+** iauGmst82 Greenwich mean sidereal time, IAU 1982
+** iauEqeq94 equation of the equinoxes, IAU 1994
+** iauAnp normalize angle into range 0 to 2pi
+**
+** References:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992)
+**
+** IAU Resolution C7, Recommendation 3 (1994)
+**
+** This revision: 2008 May 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double gmst82, eqeq94, gst;
+
+
+ gmst82 = iauGmst82(uta, utb);
+ eqeq94 = iauEqeq94(uta, utb);
+ gst = iauAnp(gmst82 + eqeq94);
+
+ return gst;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/h2fk5.c b/sofa/h2fk5.c
new file mode 100644
index 0000000..4cfc04a
--- /dev/null
+++ b/sofa/h2fk5.c
@@ -0,0 +1,198 @@
+#include "sofam.h"
+
+void iauH2fk5(double rh, double dh,
+ double drh, double ddh, double pxh, double rvh,
+ double *r5, double *d5,
+ double *dr5, double *dd5, double *px5, double *rv5)
+/*
+** - - - - - - - - -
+** i a u H 2 f k 5
+** - - - - - - - - -
+**
+** Transform Hipparcos star data into the FK5 (J2000.0) system.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given (all Hipparcos, epoch J2000.0):
+** rh double RA (radians)
+** dh double Dec (radians)
+** drh double proper motion in RA (dRA/dt, rad/Jyear)
+** ddh double proper motion in Dec (dDec/dt, rad/Jyear)
+** pxh double parallax (arcsec)
+** rvh double radial velocity (km/s, positive = receding)
+**
+** Returned (all FK5, equinox J2000.0, epoch J2000.0):
+** r5 double RA (radians)
+** d5 double Dec (radians)
+** dr5 double proper motion in RA (dRA/dt, rad/Jyear)
+** dd5 double proper motion in Dec (dDec/dt, rad/Jyear)
+** px5 double parallax (arcsec)
+** rv5 double radial velocity (km/s, positive = receding)
+**
+** Notes:
+**
+** 1) This function transforms Hipparcos star positions and proper
+** motions into FK5 J2000.0.
+**
+** 2) The proper motions in RA are dRA/dt rather than
+** cos(Dec)*dRA/dt, and are per year rather than per century.
+**
+** 3) The FK5 to Hipparcos transformation is modeled as a pure
+** rotation and spin; zonal errors in the FK5 catalog are not
+** taken into account.
+**
+** 4) See also iauFk52h, iauFk5hz, iauHfk5z.
+**
+** Called:
+** iauStarpv star catalog data to space motion pv-vector
+** iauFk5hip FK5 to Hipparcos rotation and spin
+** iauRv2m r-vector to r-matrix
+** iauRxp product of r-matrix and p-vector
+** iauTrxp product of transpose of r-matrix and p-vector
+** iauPxp vector product of two p-vectors
+** iauPmp p-vector minus p-vector
+** iauPvstar space motion pv-vector to star catalog data
+**
+** Reference:
+**
+** F.Mignard & M.Froeschle, Astron. Astrophys. 354, 732-739 (2000).
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int i;
+ double pvh[2][3], r5h[3][3], s5h[3], sh[3], wxp[3], vv[3], pv5[2][3];
+
+
+/* Hipparcos barycentric position/velocity pv-vector (normalized). */
+ iauStarpv(rh, dh, drh, ddh, pxh, rvh, pvh);
+
+/* FK5 to Hipparcos orientation matrix and spin vector. */
+ iauFk5hip(r5h, s5h);
+
+/* Make spin units per day instead of per year. */
+ for ( i = 0; i < 3; s5h[i++] /= 365.25 );
+
+/* Orient the spin into the Hipparcos system. */
+ iauRxp(r5h, s5h, sh);
+
+/* De-orient the Hipparcos position into the FK5 system. */
+ iauTrxp(r5h, pvh[0], pv5[0]);
+
+/* Apply spin to the position giving an extra space motion component. */
+ iauPxp(pvh[0], sh, wxp);
+
+/* Subtract this component from the Hipparcos space motion. */
+ iauPmp(pvh[1], wxp, vv);
+
+/* De-orient the Hipparcos space motion into the FK5 system. */
+ iauTrxp(r5h, vv, pv5[1]);
+
+/* FK5 pv-vector to spherical. */
+ iauPvstar(pv5, r5, d5, dr5, dd5, px5, rv5);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/hfk5z.c b/sofa/hfk5z.c
new file mode 100644
index 0000000..5104771
--- /dev/null
+++ b/sofa/hfk5z.c
@@ -0,0 +1,225 @@
+#include "sofam.h"
+
+void iauHfk5z(double rh, double dh, double date1, double date2,
+ double *r5, double *d5, double *dr5, double *dd5)
+/*
+** - - - - - - - - -
+** i a u H f k 5 z
+** - - - - - - - - -
+**
+** Transform a Hipparcos star position into FK5 J2000.0, assuming
+** zero Hipparcos proper motion.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** rh double Hipparcos RA (radians)
+** dh double Hipparcos Dec (radians)
+** date1,date2 double TDB date (Note 1)
+**
+** Returned (all FK5, equinox J2000.0, date date1+date2):
+** r5 double RA (radians)
+** d5 double Dec (radians)
+** dr5 double FK5 RA proper motion (rad/year, Note 4)
+** dd5 double Dec proper motion (rad/year, Note 4)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The proper motion in RA is dRA/dt rather than cos(Dec)*dRA/dt.
+**
+** 3) The FK5 to Hipparcos transformation is modeled as a pure rotation
+** and spin; zonal errors in the FK5 catalogue are not taken into
+** account.
+**
+** 4) It was the intention that Hipparcos should be a close
+** approximation to an inertial frame, so that distant objects have
+** zero proper motion; such objects have (in general) non-zero
+** proper motion in FK5, and this function returns those fictitious
+** proper motions.
+**
+** 5) The position returned by this function is in the FK5 J2000.0
+** reference system but at date date1+date2.
+**
+** 6) See also iauFk52h, iauH2fk5, iauFk5zhz.
+**
+** Called:
+** iauS2c spherical coordinates to unit vector
+** iauFk5hip FK5 to Hipparcos rotation and spin
+** iauRxp product of r-matrix and p-vector
+** iauSxp multiply p-vector by scalar
+** iauRxr product of two r-matrices
+** iauTrxp product of transpose of r-matrix and p-vector
+** iauPxp vector product of two p-vectors
+** iauPv2s pv-vector to spherical
+** iauAnp normalize angle into range 0 to 2pi
+**
+** Reference:
+**
+** F.Mignard & M.Froeschle, 2000, Astron.Astrophys. 354, 732-739.
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t, ph[3], r5h[3][3], s5h[3], sh[3], vst[3],
+ rst[3][3], r5ht[3][3], pv5e[2][3], vv[3],
+ w, r, v;
+
+
+/* Time interval from fundamental epoch J2000.0 to given date (JY). */
+ t = ((date1 - DJ00) + date2) / DJY;
+
+/* Hipparcos barycentric position vector (normalized). */
+ iauS2c(rh, dh, ph);
+
+/* FK5 to Hipparcos orientation matrix and spin vector. */
+ iauFk5hip(r5h, s5h);
+
+/* Rotate the spin into the Hipparcos system. */
+ iauRxp(r5h, s5h, sh);
+
+/* Accumulated Hipparcos wrt FK5 spin over that interval. */
+ iauSxp(t, s5h, vst);
+
+/* Express the accumulated spin as a rotation matrix. */
+ iauRv2m(vst, rst);
+
+/* Rotation matrix: accumulated spin, then FK5 to Hipparcos. */
+ iauRxr(r5h, rst, r5ht);
+
+/* De-orient & de-spin the Hipparcos position into FK5 J2000.0. */
+ iauTrxp(r5ht, ph, pv5e[0]);
+
+/* Apply spin to the position giving a space motion. */
+ iauPxp(sh, ph, vv);
+
+/* De-orient & de-spin the Hipparcos space motion into FK5 J2000.0. */
+ iauTrxp(r5ht, vv, pv5e[1]);
+
+/* FK5 position/velocity pv-vector to spherical. */
+ iauPv2s(pv5e, &w, d5, &r, dr5, dd5, &v);
+ *r5 = iauAnp(w);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/ir.c b/sofa/ir.c
new file mode 100644
index 0000000..0552891
--- /dev/null
+++ b/sofa/ir.c
@@ -0,0 +1,131 @@
+#include "sofam.h"
+
+void iauIr(double r[3][3])
+/*
+** - - - - - -
+** i a u I r
+** - - - - - -
+**
+** Initialize an r-matrix to the identity matrix.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Returned:
+** r double[3][3] r-matrix
+**
+** Called:
+** iauZr zero r-matrix
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauZr(r);
+ r[0][0] = 1.0;
+ r[1][1] = 1.0;
+ r[2][2] = 1.0;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/jd2cal.c b/sofa/jd2cal.c
new file mode 100644
index 0000000..0b788ec
--- /dev/null
+++ b/sofa/jd2cal.c
@@ -0,0 +1,205 @@
+#include "sofam.h"
+
+int iauJd2cal(double dj1, double dj2,
+ int *iy, int *im, int *id, double *fd)
+/*
+** - - - - - - - - - -
+** i a u J d 2 c a l
+** - - - - - - - - - -
+**
+** Julian Date to Gregorian year, month, day, and fraction of a day.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** dj1,dj2 double Julian Date (Notes 1, 2)
+**
+** Returned (arguments):
+** iy int year
+** im int month
+** id int day
+** fd double fraction of day
+**
+** Returned (function value):
+** int status:
+** 0 = OK
+** -1 = unacceptable date (Note 3)
+**
+** Notes:
+**
+** 1) The earliest valid date is -68569.5 (-4900 March 1). The
+** largest value accepted is 10^9.
+**
+** 2) The Julian Date is apportioned in any convenient way between
+** the arguments dj1 and dj2. For example, JD=2450123.7 could
+** be expressed in any of these ways, among others:
+**
+** dj1 dj2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** 3) In early eras the conversion is from the "proleptic Gregorian
+** calendar"; no account is taken of the date(s) of adoption of
+** the Gregorian calendar, nor is the AD/BC numbering convention
+** observed.
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992),
+** Section 12.92 (p604).
+**
+** This revision: 2008 May 26
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Minimum and maximum allowed JD */
+ static const double djmin = -68569.5;
+ static const double djmax = 1e9;
+
+ long jd, l, n, i, k;
+ double dj, d1, d2, f1, f2, f, d;
+
+
+/* Verify date is acceptable. */
+ dj = dj1 + dj2;
+ if (dj < djmin || dj > djmax) return -1;
+
+/* Copy the date, big then small, and re-align to midnight. */
+ if (dj1 >= dj2) {
+ d1 = dj1;
+ d2 = dj2;
+ } else {
+ d1 = dj2;
+ d2 = dj1;
+ }
+ d2 -= 0.5;
+
+/* Separate day and fraction. */
+ f1 = fmod(d1, 1.0);
+ f2 = fmod(d2, 1.0);
+ f = fmod(f1 + f2, 1.0);
+ if (f < 0.0) f += 1.0;
+ d = floor(d1 - f1) + floor(d2 - f2) + floor(f1 + f2 - f);
+ jd = (long) floor(d) + 1L;
+
+/* Express day in Gregorian calendar. */
+ l = jd + 68569L;
+ n = (4L * l) / 146097L;
+ l -= (146097L * n + 3L) / 4L;
+ i = (4000L * (l + 1L)) / 1461001L;
+ l -= (1461L * i) / 4L - 31L;
+ k = (80L * l) / 2447L;
+ *id = (int) (l - (2447L * k) / 80L);
+ l = k / 11L;
+ *im = (int) (k + 2L - 12L * l);
+ *iy = (int) (100L * (n - 49L) + i + l);
+ *fd = f;
+
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/jdcalf.c b/sofa/jdcalf.c
new file mode 100644
index 0000000..1a64ae7
--- /dev/null
+++ b/sofa/jdcalf.c
@@ -0,0 +1,211 @@
+#include "sofam.h"
+
+int iauJdcalf(int ndp, double dj1, double dj2, int iymdf[4])
+/*
+** - - - - - - - - - -
+** i a u J d c a l f
+** - - - - - - - - - -
+**
+** Julian Date to Gregorian Calendar, expressed in a form convenient
+** for formatting messages: rounded to a specified precision.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** ndp int number of decimal places of days in fraction
+** dj1,dj2 double dj1+dj2 = Julian Date (Note 1)
+**
+** Returned:
+** iymdf int[4] year, month, day, fraction in Gregorian
+** calendar
+**
+** Returned (function value):
+** int status:
+** -1 = date out of range
+** 0 = OK
+** +1 = NDP not 0-9 (interpreted as 0)
+**
+** Notes:
+**
+** 1) The Julian Date is apportioned in any convenient way between
+** the arguments dj1 and dj2. For example, JD=2450123.7 could
+** be expressed in any of these ways, among others:
+**
+** dj1 dj2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** 2) In early eras the conversion is from the "Proleptic Gregorian
+** Calendar"; no account is taken of the date(s) of adoption of
+** the Gregorian Calendar, nor is the AD/BC numbering convention
+** observed.
+**
+** 3) Refer to the function iauJd2cal.
+**
+** 4) NDP should be 4 or less if internal overflows are to be
+** avoided on machines which use 16-bit integers.
+**
+** Called:
+** iauJd2cal JD to Gregorian calendar
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992),
+** Section 12.92 (p604).
+**
+** This revision: 2010 July 27
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int j, js;
+ double denom, d1, d2, f1, f2, f;
+
+
+/* Denominator of fraction (e.g. 100 for 2 decimal places). */
+ if ((ndp >= 0) && (ndp <= 9)) {
+ j = 0;
+ denom = pow(10.0, ndp);
+ } else {
+ j = 1;
+ denom = 1.0;
+ }
+
+/* Copy the date, big then small, and realign to midnight. */
+ if (dj1 >= dj2) {
+ d1 = dj1;
+ d2 = dj2;
+ } else {
+ d1 = dj2;
+ d2 = dj1;
+ }
+ d2 -= 0.5;
+
+/* Separate days and fractions. */
+ f1 = fmod(d1, 1.0);
+ f2 = fmod(d2, 1.0);
+ d1 = floor(d1 - f1);
+ d2 = floor(d2 - f2);
+
+/* Round the total fraction to the specified number of places. */
+ f = floor((f1+f2)*denom + 0.5) / denom;
+
+/* Re-assemble the rounded date and re-align to noon. */
+ d2 += f + 0.5;
+
+/* Convert to Gregorian calendar. */
+ js = iauJd2cal(d1, d2, &iymdf[0], &iymdf[1], &iymdf[2], &f);
+ if (js == 0) {
+ iymdf[3] = (int) (f * denom);
+ } else {
+ j = js;
+ }
+
+/* Return the status. */
+ return j;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/num00a.c b/sofa/num00a.c
new file mode 100644
index 0000000..4d8cba0
--- /dev/null
+++ b/sofa/num00a.c
@@ -0,0 +1,171 @@
+#include "sofam.h"
+
+void iauNum00a(double date1, double date2, double rmatn[3][3])
+/*
+** - - - - - - - - - -
+** i a u N u m 0 0 a
+** - - - - - - - - - -
+**
+** Form the matrix of nutation for a given date, IAU 2000A model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rmatn double[3][3] nutation matrix
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix operates in the sense V(true) = rmatn * V(mean), where
+** the p-vector V(true) is with respect to the true equatorial triad
+** of date and the p-vector V(mean) is with respect to the mean
+** equatorial triad of date.
+**
+** 3) A faster, but slightly less accurate result (about 1 mas), can be
+** obtained by using instead the iauNum00b function.
+**
+** Called:
+** iauPn00a bias/precession/nutation, IAU 2000A
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992),
+** Section 3.222-3 (p114).
+**
+** This revision: 2008 May 12
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dpsi, deps, epsa, rb[3][3], rp[3][3], rbp[3][3], rbpn[3][3];
+
+
+/* Obtain the required matrix (discarding other results). */
+ iauPn00a(date1, date2,
+ &dpsi, &deps, &epsa, rb, rp, rbp, rmatn, rbpn);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/num00b.c b/sofa/num00b.c
new file mode 100644
index 0000000..38f4bcb
--- /dev/null
+++ b/sofa/num00b.c
@@ -0,0 +1,171 @@
+#include "sofam.h"
+
+void iauNum00b(double date1, double date2, double rmatn[3][3])
+/*
+** - - - - - - - - - -
+** i a u N u m 0 0 b
+** - - - - - - - - - -
+**
+** Form the matrix of nutation for a given date, IAU 2000B model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rmatn double[3][3] nutation matrix
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix operates in the sense V(true) = rmatn * V(mean), where
+** the p-vector V(true) is with respect to the true equatorial triad
+** of date and the p-vector V(mean) is with respect to the mean
+** equatorial triad of date.
+**
+** 3) The present function is faster, but slightly less accurate (about
+** 1 mas), than the iauNum00a function.
+**
+** Called:
+** iauPn00b bias/precession/nutation, IAU 2000B
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992),
+** Section 3.222-3 (p114).
+**
+** This revision: 2008 May 12
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dpsi, deps, epsa, rb[3][3], rp[3][3], rbp[3][3], rbpn[3][3];
+
+
+/* Obtain the required matrix (discarding other results). */
+ iauPn00b(date1, date2,
+ &dpsi, &deps, &epsa, rb, rp, rbp, rmatn, rbpn);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/num06a.c b/sofa/num06a.c
new file mode 100644
index 0000000..c903f30
--- /dev/null
+++ b/sofa/num06a.c
@@ -0,0 +1,175 @@
+#include "sofam.h"
+
+void iauNum06a(double date1, double date2, double rmatn[3][3])
+/*
+** - - - - - - - - - -
+** i a u N u m 0 6 a
+** - - - - - - - - - -
+**
+** Form the matrix of nutation for a given date, IAU 2006/2000A model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rmatn double[3][3] nutation matrix
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix operates in the sense V(true) = rmatn * V(mean), where
+** the p-vector V(true) is with respect to the true equatorial triad
+** of date and the p-vector V(mean) is with respect to the mean
+** equatorial triad of date.
+**
+** Called:
+** iauObl06 mean obliquity, IAU 2006
+** iauNut06a nutation, IAU 2006/2000A
+** iauNumat form nutation matrix
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992),
+** Section 3.222-3 (p114).
+**
+** This revision: 2008 May 12
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double eps, dp, de;
+
+
+/* Mean obliquity. */
+ eps = iauObl06(date1, date2);
+
+/* Nutation components. */
+ iauNut06a(date1, date2, &dp, &de);
+
+/* Nutation matrix. */
+ iauNumat(eps, dp, de, rmatn);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/numat.c b/sofa/numat.c
new file mode 100644
index 0000000..846f7c8
--- /dev/null
+++ b/sofa/numat.c
@@ -0,0 +1,159 @@
+#include "sofam.h"
+
+void iauNumat(double epsa, double dpsi, double deps, double rmatn[3][3])
+/*
+** - - - - - - - - -
+** i a u N u m a t
+** - - - - - - - - -
+**
+** Form the matrix of nutation.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** epsa double mean obliquity of date (Note 1)
+** dpsi,deps double nutation (Note 2)
+**
+** Returned:
+** rmatn double[3][3] nutation matrix (Note 3)
+**
+** Notes:
+**
+**
+** 1) The supplied mean obliquity epsa, must be consistent with the
+** precession-nutation models from which dpsi and deps were obtained.
+**
+** 2) The caller is responsible for providing the nutation components;
+** they are in longitude and obliquity, in radians and are with
+** respect to the equinox and ecliptic of date.
+**
+** 3) The matrix operates in the sense V(true) = rmatn * V(mean),
+** where the p-vector V(true) is with respect to the true
+** equatorial triad of date and the p-vector V(mean) is with
+** respect to the mean equatorial triad of date.
+**
+** Called:
+** iauIr initialize r-matrix to identity
+** iauRx rotate around X-axis
+** iauRz rotate around Z-axis
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992),
+** Section 3.222-3 (p114).
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Build the rotation matrix. */
+ iauIr(rmatn);
+ iauRx(epsa, rmatn);
+ iauRz(-dpsi, rmatn);
+ iauRx(-(epsa + deps), rmatn);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/nut00a.c b/sofa/nut00a.c
new file mode 100644
index 0000000..6742ed1
--- /dev/null
+++ b/sofa/nut00a.c
@@ -0,0 +1,2097 @@
+#include "sofam.h"
+
+void iauNut00a(double date1, double date2, double *dpsi, double *deps)
+/*
+** - - - - - - - - - -
+** i a u N u t 0 0 a
+** - - - - - - - - - -
+**
+** Nutation, IAU 2000A model (MHB2000 luni-solar and planetary nutation
+** with free core nutation omitted).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** dpsi,deps double nutation, luni-solar + planetary (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The nutation components in longitude and obliquity are in radians
+** and with respect to the equinox and ecliptic of date. The
+** obliquity at J2000.0 is assumed to be the Lieske et al. (1977)
+** value of 84381.448 arcsec.
+**
+** Both the luni-solar and planetary nutations are included. The
+** latter are due to direct planetary nutations and the
+** perturbations of the lunar and terrestrial orbits.
+**
+** 3) The function computes the MHB2000 nutation series with the
+** associated corrections for planetary nutations. It is an
+** implementation of the nutation part of the IAU 2000A precession-
+** nutation model, formally adopted by the IAU General Assembly in
+** 2000, namely MHB2000 (Mathews et al. 2002), but with the free
+** core nutation (FCN - see Note 4) omitted.
+**
+** 4) The full MHB2000 model also contains contributions to the
+** nutations in longitude and obliquity due to the free-excitation
+** of the free-core-nutation during the period 1979-2000. These FCN
+** terms, which are time-dependent and unpredictable, are NOT
+** included in the present function and, if required, must be
+** independently computed. With the FCN corrections included, the
+** present function delivers a pole which is at current epochs
+** accurate to a few hundred microarcseconds. The omission of FCN
+** introduces further errors of about that size.
+**
+** 5) The present function provides classical nutation. The MHB2000
+** algorithm, from which it is adapted, deals also with (i) the
+** offsets between the GCRS and mean poles and (ii) the adjustments
+** in longitude and obliquity due to the changed precession rates.
+** These additional functions, namely frame bias and precession
+** adjustments, are supported by the SOFA functions iauBi00 and
+** iauPr00.
+**
+** 6) The MHB2000 algorithm also provides "total" nutations, comprising
+** the arithmetic sum of the frame bias, precession adjustments,
+** luni-solar nutation and planetary nutation. These total
+** nutations can be used in combination with an existing IAU 1976
+** precession implementation, such as iauPmat76, to deliver GCRS-
+** to-true predictions of sub-mas accuracy at current dates.
+** However, there are three shortcomings in the MHB2000 model that
+** must be taken into account if more accurate or definitive results
+** are required (see Wallace 2002):
+**
+** (i) The MHB2000 total nutations are simply arithmetic sums,
+** yet in reality the various components are successive Euler
+** rotations. This slight lack of rigor leads to cross terms
+** that exceed 1 mas after a century. The rigorous procedure
+** is to form the GCRS-to-true rotation matrix by applying the
+** bias, precession and nutation in that order.
+**
+** (ii) Although the precession adjustments are stated to be with
+** respect to Lieske et al. (1977), the MHB2000 model does
+** not specify which set of Euler angles are to be used and
+** how the adjustments are to be applied. The most literal
+** and straightforward procedure is to adopt the 4-rotation
+** epsilon_0, psi_A, omega_A, xi_A option, and to add DPSIPR
+** to psi_A and DEPSPR to both omega_A and eps_A.
+**
+** (iii) The MHB2000 model predates the determination by Chapront
+** et al. (2002) of a 14.6 mas displacement between the
+** J2000.0 mean equinox and the origin of the ICRS frame. It
+** should, however, be noted that neglecting this displacement
+** when calculating star coordinates does not lead to a
+** 14.6 mas change in right ascension, only a small second-
+** order distortion in the pattern of the precession-nutation
+** effect.
+**
+** For these reasons, the SOFA functions do not generate the "total
+** nutations" directly, though they can of course easily be
+** generated by calling iauBi00, iauPr00 and the present function
+** and adding the results.
+**
+** 7) The MHB2000 model contains 41 instances where the same frequency
+** appears multiple times, of which 38 are duplicates and three are
+** triplicates. To keep the present code close to the original MHB
+** algorithm, this small inefficiency has not been corrected.
+**
+** Called:
+** iauFal03 mean anomaly of the Moon
+** iauFaf03 mean argument of the latitude of the Moon
+** iauFaom03 mean longitude of the Moon's ascending node
+** iauFame03 mean longitude of Mercury
+** iauFave03 mean longitude of Venus
+** iauFae03 mean longitude of Earth
+** iauFama03 mean longitude of Mars
+** iauFaju03 mean longitude of Jupiter
+** iauFasa03 mean longitude of Saturn
+** iauFaur03 mean longitude of Uranus
+** iauFapa03 general accumulated precession in longitude
+**
+** References:
+**
+** Chapront, J., Chapront-Touze, M. & Francou, G. 2002,
+** Astron.Astrophys. 387, 700
+**
+** Lieske, J.H., Lederle, T., Fricke, W. & Morando, B. 1977,
+** Astron.Astrophys. 58, 1-16
+**
+** Mathews, P.M., Herring, T.A., Buffet, B.A. 2002, J.Geophys.Res.
+** 107, B4. The MHB_2000 code itself was obtained on 9th September
+** 2002 from ftp//maia.usno.navy.mil/conv2000/chapter5/IAU2000A.
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** Souchay, J., Loysel, B., Kinoshita, H., Folgueira, M. 1999,
+** Astron.Astrophys.Supp.Ser. 135, 111
+**
+** Wallace, P.T., "Software for Implementing the IAU 2000
+** Resolutions", in IERS Workshop 5.1 (2002)
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int i;
+ double t, el, elp, f, d, om, arg, dp, de, sarg, carg,
+ al, af, ad, aom, alme, alve, alea, alma,
+ alju, alsa, alur, alne, apa, dpsils, depsls,
+ dpsipl, depspl;
+
+/* Units of 0.1 microarcsecond to radians */
+ const double U2R = DAS2R / 1e7;
+
+/* ------------------------- */
+/* Luni-Solar nutation model */
+/* ------------------------- */
+
+/* The units for the sine and cosine coefficients are */
+/* 0.1 microarcsecond and the same per Julian century */
+
+ static const struct {
+ int nl,nlp,nf,nd,nom; /* coefficients of l,l',F,D,Om */
+ double sp,spt,cp; /* longitude sin, t*sin, cos coefficients */
+ double ce,cet,se; /* obliquity cos, t*cos, sin coefficients */
+ } xls[] = {
+
+ /* 1- 10 */
+ { 0, 0, 0, 0, 1,
+ -172064161.0, -174666.0, 33386.0, 92052331.0, 9086.0, 15377.0},
+ { 0, 0, 2,-2, 2,
+ -13170906.0, -1675.0, -13696.0, 5730336.0, -3015.0, -4587.0},
+ { 0, 0, 2, 0, 2,-2276413.0,-234.0,2796.0,978459.0,-485.0, 1374.0},
+ { 0, 0, 0, 0, 2,2074554.0, 207.0, -698.0,-897492.0,470.0, -291.0},
+ { 0, 1, 0, 0, 0,1475877.0,-3633.0,11817.0,73871.0,-184.0,-1924.0},
+ { 0, 1, 2,-2, 2,-516821.0,1226.0, -524.0,224386.0,-677.0, -174.0},
+ { 1, 0, 0, 0, 0, 711159.0, 73.0, -872.0, -6750.0, 0.0, 358.0},
+ { 0, 0, 2, 0, 1,-387298.0,-367.0, 380.0, 200728.0, 18.0, 318.0},
+ { 1, 0, 2, 0, 2,-301461.0, -36.0, 816.0, 129025.0,-63.0, 367.0},
+ { 0,-1, 2,-2, 2, 215829.0,-494.0, 111.0, -95929.0,299.0, 132.0},
+
+ /* 11-20 */
+ { 0, 0, 2,-2, 1, 128227.0, 137.0, 181.0, -68982.0, -9.0, 39.0},
+ {-1, 0, 2, 0, 2, 123457.0, 11.0, 19.0, -53311.0, 32.0, -4.0},
+ {-1, 0, 0, 2, 0, 156994.0, 10.0, -168.0, -1235.0, 0.0, 82.0},
+ { 1, 0, 0, 0, 1, 63110.0, 63.0, 27.0, -33228.0, 0.0, -9.0},
+ {-1, 0, 0, 0, 1, -57976.0, -63.0, -189.0, 31429.0, 0.0, -75.0},
+ {-1, 0, 2, 2, 2, -59641.0, -11.0, 149.0, 25543.0,-11.0, 66.0},
+ { 1, 0, 2, 0, 1, -51613.0, -42.0, 129.0, 26366.0, 0.0, 78.0},
+ {-2, 0, 2, 0, 1, 45893.0, 50.0, 31.0, -24236.0,-10.0, 20.0},
+ { 0, 0, 0, 2, 0, 63384.0, 11.0, -150.0, -1220.0, 0.0, 29.0},
+ { 0, 0, 2, 2, 2, -38571.0, -1.0, 158.0, 16452.0,-11.0, 68.0},
+
+ /* 21-30 */
+ { 0,-2, 2,-2, 2, 32481.0, 0.0, 0.0, -13870.0, 0.0, 0.0},
+ {-2, 0, 0, 2, 0, -47722.0, 0.0, -18.0, 477.0, 0.0, -25.0},
+ { 2, 0, 2, 0, 2, -31046.0, -1.0, 131.0, 13238.0,-11.0, 59.0},
+ { 1, 0, 2,-2, 2, 28593.0, 0.0, -1.0, -12338.0, 10.0, -3.0},
+ {-1, 0, 2, 0, 1, 20441.0, 21.0, 10.0, -10758.0, 0.0, -3.0},
+ { 2, 0, 0, 0, 0, 29243.0, 0.0, -74.0, -609.0, 0.0, 13.0},
+ { 0, 0, 2, 0, 0, 25887.0, 0.0, -66.0, -550.0, 0.0, 11.0},
+ { 0, 1, 0, 0, 1, -14053.0, -25.0, 79.0, 8551.0, -2.0, -45.0},
+ {-1, 0, 0, 2, 1, 15164.0, 10.0, 11.0, -8001.0, 0.0, -1.0},
+ { 0, 2, 2,-2, 2, -15794.0, 72.0, -16.0, 6850.0,-42.0, -5.0},
+
+ /* 31-40 */
+ { 0, 0,-2, 2, 0, 21783.0, 0.0, 13.0, -167.0, 0.0, 13.0},
+ { 1, 0, 0,-2, 1, -12873.0, -10.0, -37.0, 6953.0, 0.0, -14.0},
+ { 0,-1, 0, 0, 1, -12654.0, 11.0, 63.0, 6415.0, 0.0, 26.0},
+ {-1, 0, 2, 2, 1, -10204.0, 0.0, 25.0, 5222.0, 0.0, 15.0},
+ { 0, 2, 0, 0, 0, 16707.0, -85.0, -10.0, 168.0, -1.0, 10.0},
+ { 1, 0, 2, 2, 2, -7691.0, 0.0, 44.0, 3268.0, 0.0, 19.0},
+ {-2, 0, 2, 0, 0, -11024.0, 0.0, -14.0, 104.0, 0.0, 2.0},
+ { 0, 1, 2, 0, 2, 7566.0, -21.0, -11.0, -3250.0, 0.0, -5.0},
+ { 0, 0, 2, 2, 1, -6637.0, -11.0, 25.0, 3353.0, 0.0, 14.0},
+ { 0,-1, 2, 0, 2, -7141.0, 21.0, 8.0, 3070.0, 0.0, 4.0},
+
+ /* 41-50 */
+ { 0, 0, 0, 2, 1, -6302.0, -11.0, 2.0, 3272.0, 0.0, 4.0},
+ { 1, 0, 2,-2, 1, 5800.0, 10.0, 2.0, -3045.0, 0.0, -1.0},
+ { 2, 0, 2,-2, 2, 6443.0, 0.0, -7.0, -2768.0, 0.0, -4.0},
+ {-2, 0, 0, 2, 1, -5774.0, -11.0, -15.0, 3041.0, 0.0, -5.0},
+ { 2, 0, 2, 0, 1, -5350.0, 0.0, 21.0, 2695.0, 0.0, 12.0},
+ { 0,-1, 2,-2, 1, -4752.0, -11.0, -3.0, 2719.0, 0.0, -3.0},
+ { 0, 0, 0,-2, 1, -4940.0, -11.0, -21.0, 2720.0, 0.0, -9.0},
+ {-1,-1, 0, 2, 0, 7350.0, 0.0, -8.0, -51.0, 0.0, 4.0},
+ { 2, 0, 0,-2, 1, 4065.0, 0.0, 6.0, -2206.0, 0.0, 1.0},
+ { 1, 0, 0, 2, 0, 6579.0, 0.0, -24.0, -199.0, 0.0, 2.0},
+
+ /* 51-60 */
+ { 0, 1, 2,-2, 1, 3579.0, 0.0, 5.0, -1900.0, 0.0, 1.0},
+ { 1,-1, 0, 0, 0, 4725.0, 0.0, -6.0, -41.0, 0.0, 3.0},
+ {-2, 0, 2, 0, 2, -3075.0, 0.0, -2.0, 1313.0, 0.0, -1.0},
+ { 3, 0, 2, 0, 2, -2904.0, 0.0, 15.0, 1233.0, 0.0, 7.0},
+ { 0,-1, 0, 2, 0, 4348.0, 0.0, -10.0, -81.0, 0.0, 2.0},
+ { 1,-1, 2, 0, 2, -2878.0, 0.0, 8.0, 1232.0, 0.0, 4.0},
+ { 0, 0, 0, 1, 0, -4230.0, 0.0, 5.0, -20.0, 0.0, -2.0},
+ {-1,-1, 2, 2, 2, -2819.0, 0.0, 7.0, 1207.0, 0.0, 3.0},
+ {-1, 0, 2, 0, 0, -4056.0, 0.0, 5.0, 40.0, 0.0, -2.0},
+ { 0,-1, 2, 2, 2, -2647.0, 0.0, 11.0, 1129.0, 0.0, 5.0},
+
+ /* 61-70 */
+ {-2, 0, 0, 0, 1, -2294.0, 0.0, -10.0, 1266.0, 0.0, -4.0},
+ { 1, 1, 2, 0, 2, 2481.0, 0.0, -7.0, -1062.0, 0.0, -3.0},
+ { 2, 0, 0, 0, 1, 2179.0, 0.0, -2.0, -1129.0, 0.0, -2.0},
+ {-1, 1, 0, 1, 0, 3276.0, 0.0, 1.0, -9.0, 0.0, 0.0},
+ { 1, 1, 0, 0, 0, -3389.0, 0.0, 5.0, 35.0, 0.0, -2.0},
+ { 1, 0, 2, 0, 0, 3339.0, 0.0, -13.0, -107.0, 0.0, 1.0},
+ {-1, 0, 2,-2, 1, -1987.0, 0.0, -6.0, 1073.0, 0.0, -2.0},
+ { 1, 0, 0, 0, 2, -1981.0, 0.0, 0.0, 854.0, 0.0, 0.0},
+ {-1, 0, 0, 1, 0, 4026.0, 0.0, -353.0, -553.0, 0.0, -139.0},
+ { 0, 0, 2, 1, 2, 1660.0, 0.0, -5.0, -710.0, 0.0, -2.0},
+
+ /* 71-80 */
+ {-1, 0, 2, 4, 2, -1521.0, 0.0, 9.0, 647.0, 0.0, 4.0},
+ {-1, 1, 0, 1, 1, 1314.0, 0.0, 0.0, -700.0, 0.0, 0.0},
+ { 0,-2, 2,-2, 1, -1283.0, 0.0, 0.0, 672.0, 0.0, 0.0},
+ { 1, 0, 2, 2, 1, -1331.0, 0.0, 8.0, 663.0, 0.0, 4.0},
+ {-2, 0, 2, 2, 2, 1383.0, 0.0, -2.0, -594.0, 0.0, -2.0},
+ {-1, 0, 0, 0, 2, 1405.0, 0.0, 4.0, -610.0, 0.0, 2.0},
+ { 1, 1, 2,-2, 2, 1290.0, 0.0, 0.0, -556.0, 0.0, 0.0},
+ {-2, 0, 2, 4, 2, -1214.0, 0.0, 5.0, 518.0, 0.0, 2.0},
+ {-1, 0, 4, 0, 2, 1146.0, 0.0, -3.0, -490.0, 0.0, -1.0},
+ { 2, 0, 2,-2, 1, 1019.0, 0.0, -1.0, -527.0, 0.0, -1.0},
+
+ /* 81-90 */
+ { 2, 0, 2, 2, 2, -1100.0, 0.0, 9.0, 465.0, 0.0, 4.0},
+ { 1, 0, 0, 2, 1, -970.0, 0.0, 2.0, 496.0, 0.0, 1.0},
+ { 3, 0, 0, 0, 0, 1575.0, 0.0, -6.0, -50.0, 0.0, 0.0},
+ { 3, 0, 2,-2, 2, 934.0, 0.0, -3.0, -399.0, 0.0, -1.0},
+ { 0, 0, 4,-2, 2, 922.0, 0.0, -1.0, -395.0, 0.0, -1.0},
+ { 0, 1, 2, 0, 1, 815.0, 0.0, -1.0, -422.0, 0.0, -1.0},
+ { 0, 0,-2, 2, 1, 834.0, 0.0, 2.0, -440.0, 0.0, 1.0},
+ { 0, 0, 2,-2, 3, 1248.0, 0.0, 0.0, -170.0, 0.0, 1.0},
+ {-1, 0, 0, 4, 0, 1338.0, 0.0, -5.0, -39.0, 0.0, 0.0},
+ { 2, 0,-2, 0, 1, 716.0, 0.0, -2.0, -389.0, 0.0, -1.0},
+
+ /* 91-100 */
+ {-2, 0, 0, 4, 0, 1282.0, 0.0, -3.0, -23.0, 0.0, 1.0},
+ {-1,-1, 0, 2, 1, 742.0, 0.0, 1.0, -391.0, 0.0, 0.0},
+ {-1, 0, 0, 1, 1, 1020.0, 0.0, -25.0, -495.0, 0.0, -10.0},
+ { 0, 1, 0, 0, 2, 715.0, 0.0, -4.0, -326.0, 0.0, 2.0},
+ { 0, 0,-2, 0, 1, -666.0, 0.0, -3.0, 369.0, 0.0, -1.0},
+ { 0,-1, 2, 0, 1, -667.0, 0.0, 1.0, 346.0, 0.0, 1.0},
+ { 0, 0, 2,-1, 2, -704.0, 0.0, 0.0, 304.0, 0.0, 0.0},
+ { 0, 0, 2, 4, 2, -694.0, 0.0, 5.0, 294.0, 0.0, 2.0},
+ {-2,-1, 0, 2, 0, -1014.0, 0.0, -1.0, 4.0, 0.0, -1.0},
+ { 1, 1, 0,-2, 1, -585.0, 0.0, -2.0, 316.0, 0.0, -1.0},
+
+ /* 101-110 */
+ {-1, 1, 0, 2, 0, -949.0, 0.0, 1.0, 8.0, 0.0, -1.0},
+ {-1, 1, 0, 1, 2, -595.0, 0.0, 0.0, 258.0, 0.0, 0.0},
+ { 1,-1, 0, 0, 1, 528.0, 0.0, 0.0, -279.0, 0.0, 0.0},
+ { 1,-1, 2, 2, 2, -590.0, 0.0, 4.0, 252.0, 0.0, 2.0},
+ {-1, 1, 2, 2, 2, 570.0, 0.0, -2.0, -244.0, 0.0, -1.0},
+ { 3, 0, 2, 0, 1, -502.0, 0.0, 3.0, 250.0, 0.0, 2.0},
+ { 0, 1,-2, 2, 0, -875.0, 0.0, 1.0, 29.0, 0.0, 0.0},
+ {-1, 0, 0,-2, 1, -492.0, 0.0, -3.0, 275.0, 0.0, -1.0},
+ { 0, 1, 2, 2, 2, 535.0, 0.0, -2.0, -228.0, 0.0, -1.0},
+ {-1,-1, 2, 2, 1, -467.0, 0.0, 1.0, 240.0, 0.0, 1.0},
+
+ /* 111-120 */
+ { 0,-1, 0, 0, 2, 591.0, 0.0, 0.0, -253.0, 0.0, 0.0},
+ { 1, 0, 2,-4, 1, -453.0, 0.0, -1.0, 244.0, 0.0, -1.0},
+ {-1, 0,-2, 2, 0, 766.0, 0.0, 1.0, 9.0, 0.0, 0.0},
+ { 0,-1, 2, 2, 1, -446.0, 0.0, 2.0, 225.0, 0.0, 1.0},
+ { 2,-1, 2, 0, 2, -488.0, 0.0, 2.0, 207.0, 0.0, 1.0},
+ { 0, 0, 0, 2, 2, -468.0, 0.0, 0.0, 201.0, 0.0, 0.0},
+ { 1,-1, 2, 0, 1, -421.0, 0.0, 1.0, 216.0, 0.0, 1.0},
+ {-1, 1, 2, 0, 2, 463.0, 0.0, 0.0, -200.0, 0.0, 0.0},
+ { 0, 1, 0, 2, 0, -673.0, 0.0, 2.0, 14.0, 0.0, 0.0},
+ { 0,-1,-2, 2, 0, 658.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+
+ /* 121-130 */
+ { 0, 3, 2,-2, 2, -438.0, 0.0, 0.0, 188.0, 0.0, 0.0},
+ { 0, 0, 0, 1, 1, -390.0, 0.0, 0.0, 205.0, 0.0, 0.0},
+ {-1, 0, 2, 2, 0, 639.0, -11.0, -2.0, -19.0, 0.0, 0.0},
+ { 2, 1, 2, 0, 2, 412.0, 0.0, -2.0, -176.0, 0.0, -1.0},
+ { 1, 1, 0, 0, 1, -361.0, 0.0, 0.0, 189.0, 0.0, 0.0},
+ { 1, 1, 2, 0, 1, 360.0, 0.0, -1.0, -185.0, 0.0, -1.0},
+ { 2, 0, 0, 2, 0, 588.0, 0.0, -3.0, -24.0, 0.0, 0.0},
+ { 1, 0,-2, 2, 0, -578.0, 0.0, 1.0, 5.0, 0.0, 0.0},
+ {-1, 0, 0, 2, 2, -396.0, 0.0, 0.0, 171.0, 0.0, 0.0},
+ { 0, 1, 0, 1, 0, 565.0, 0.0, -1.0, -6.0, 0.0, 0.0},
+
+ /* 131-140 */
+ { 0, 1, 0,-2, 1, -335.0, 0.0, -1.0, 184.0, 0.0, -1.0},
+ {-1, 0, 2,-2, 2, 357.0, 0.0, 1.0, -154.0, 0.0, 0.0},
+ { 0, 0, 0,-1, 1, 321.0, 0.0, 1.0, -174.0, 0.0, 0.0},
+ {-1, 1, 0, 0, 1, -301.0, 0.0, -1.0, 162.0, 0.0, 0.0},
+ { 1, 0, 2,-1, 2, -334.0, 0.0, 0.0, 144.0, 0.0, 0.0},
+ { 1,-1, 0, 2, 0, 493.0, 0.0, -2.0, -15.0, 0.0, 0.0},
+ { 0, 0, 0, 4, 0, 494.0, 0.0, -2.0, -19.0, 0.0, 0.0},
+ { 1, 0, 2, 1, 2, 337.0, 0.0, -1.0, -143.0, 0.0, -1.0},
+ { 0, 0, 2, 1, 1, 280.0, 0.0, -1.0, -144.0, 0.0, 0.0},
+ { 1, 0, 0,-2, 2, 309.0, 0.0, 1.0, -134.0, 0.0, 0.0},
+
+ /* 141-150 */
+ {-1, 0, 2, 4, 1, -263.0, 0.0, 2.0, 131.0, 0.0, 1.0},
+ { 1, 0,-2, 0, 1, 253.0, 0.0, 1.0, -138.0, 0.0, 0.0},
+ { 1, 1, 2,-2, 1, 245.0, 0.0, 0.0, -128.0, 0.0, 0.0},
+ { 0, 0, 2, 2, 0, 416.0, 0.0, -2.0, -17.0, 0.0, 0.0},
+ {-1, 0, 2,-1, 1, -229.0, 0.0, 0.0, 128.0, 0.0, 0.0},
+ {-2, 0, 2, 2, 1, 231.0, 0.0, 0.0, -120.0, 0.0, 0.0},
+ { 4, 0, 2, 0, 2, -259.0, 0.0, 2.0, 109.0, 0.0, 1.0},
+ { 2,-1, 0, 0, 0, 375.0, 0.0, -1.0, -8.0, 0.0, 0.0},
+ { 2, 1, 2,-2, 2, 252.0, 0.0, 0.0, -108.0, 0.0, 0.0},
+ { 0, 1, 2, 1, 2, -245.0, 0.0, 1.0, 104.0, 0.0, 0.0},
+
+ /* 151-160 */
+ { 1, 0, 4,-2, 2, 243.0, 0.0, -1.0, -104.0, 0.0, 0.0},
+ {-1,-1, 0, 0, 1, 208.0, 0.0, 1.0, -112.0, 0.0, 0.0},
+ { 0, 1, 0, 2, 1, 199.0, 0.0, 0.0, -102.0, 0.0, 0.0},
+ {-2, 0, 2, 4, 1, -208.0, 0.0, 1.0, 105.0, 0.0, 0.0},
+ { 2, 0, 2, 0, 0, 335.0, 0.0, -2.0, -14.0, 0.0, 0.0},
+ { 1, 0, 0, 1, 0, -325.0, 0.0, 1.0, 7.0, 0.0, 0.0},
+ {-1, 0, 0, 4, 1, -187.0, 0.0, 0.0, 96.0, 0.0, 0.0},
+ {-1, 0, 4, 0, 1, 197.0, 0.0, -1.0, -100.0, 0.0, 0.0},
+ { 2, 0, 2, 2, 1, -192.0, 0.0, 2.0, 94.0, 0.0, 1.0},
+ { 0, 0, 2,-3, 2, -188.0, 0.0, 0.0, 83.0, 0.0, 0.0},
+
+ /* 161-170 */
+ {-1,-2, 0, 2, 0, 276.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 2, 1, 0, 0, 0, -286.0, 0.0, 1.0, 6.0, 0.0, 0.0},
+ { 0, 0, 4, 0, 2, 186.0, 0.0, -1.0, -79.0, 0.0, 0.0},
+ { 0, 0, 0, 0, 3, -219.0, 0.0, 0.0, 43.0, 0.0, 0.0},
+ { 0, 3, 0, 0, 0, 276.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 0, 0, 2,-4, 1, -153.0, 0.0, -1.0, 84.0, 0.0, 0.0},
+ { 0,-1, 0, 2, 1, -156.0, 0.0, 0.0, 81.0, 0.0, 0.0},
+ { 0, 0, 0, 4, 1, -154.0, 0.0, 1.0, 78.0, 0.0, 0.0},
+ {-1,-1, 2, 4, 2, -174.0, 0.0, 1.0, 75.0, 0.0, 0.0},
+ { 1, 0, 2, 4, 2, -163.0, 0.0, 2.0, 69.0, 0.0, 1.0},
+
+ /* 171-180 */
+ {-2, 2, 0, 2, 0, -228.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ {-2,-1, 2, 0, 1, 91.0, 0.0, -4.0, -54.0, 0.0, -2.0},
+ {-2, 0, 0, 2, 2, 175.0, 0.0, 0.0, -75.0, 0.0, 0.0},
+ {-1,-1, 2, 0, 2, -159.0, 0.0, 0.0, 69.0, 0.0, 0.0},
+ { 0, 0, 4,-2, 1, 141.0, 0.0, 0.0, -72.0, 0.0, 0.0},
+ { 3, 0, 2,-2, 1, 147.0, 0.0, 0.0, -75.0, 0.0, 0.0},
+ {-2,-1, 0, 2, 1, -132.0, 0.0, 0.0, 69.0, 0.0, 0.0},
+ { 1, 0, 0,-1, 1, 159.0, 0.0, -28.0, -54.0, 0.0, 11.0},
+ { 0,-2, 0, 2, 0, 213.0, 0.0, 0.0, -4.0, 0.0, 0.0},
+ {-2, 0, 0, 4, 1, 123.0, 0.0, 0.0, -64.0, 0.0, 0.0},
+
+ /* 181-190 */
+ {-3, 0, 0, 0, 1, -118.0, 0.0, -1.0, 66.0, 0.0, 0.0},
+ { 1, 1, 2, 2, 2, 144.0, 0.0, -1.0, -61.0, 0.0, 0.0},
+ { 0, 0, 2, 4, 1, -121.0, 0.0, 1.0, 60.0, 0.0, 0.0},
+ { 3, 0, 2, 2, 2, -134.0, 0.0, 1.0, 56.0, 0.0, 1.0},
+ {-1, 1, 2,-2, 1, -105.0, 0.0, 0.0, 57.0, 0.0, 0.0},
+ { 2, 0, 0,-4, 1, -102.0, 0.0, 0.0, 56.0, 0.0, 0.0},
+ { 0, 0, 0,-2, 2, 120.0, 0.0, 0.0, -52.0, 0.0, 0.0},
+ { 2, 0, 2,-4, 1, 101.0, 0.0, 0.0, -54.0, 0.0, 0.0},
+ {-1, 1, 0, 2, 1, -113.0, 0.0, 0.0, 59.0, 0.0, 0.0},
+ { 0, 0, 2,-1, 1, -106.0, 0.0, 0.0, 61.0, 0.0, 0.0},
+
+ /* 191-200 */
+ { 0,-2, 2, 2, 2, -129.0, 0.0, 1.0, 55.0, 0.0, 0.0},
+ { 2, 0, 0, 2, 1, -114.0, 0.0, 0.0, 57.0, 0.0, 0.0},
+ { 4, 0, 2,-2, 2, 113.0, 0.0, -1.0, -49.0, 0.0, 0.0},
+ { 2, 0, 0,-2, 2, -102.0, 0.0, 0.0, 44.0, 0.0, 0.0},
+ { 0, 2, 0, 0, 1, -94.0, 0.0, 0.0, 51.0, 0.0, 0.0},
+ { 1, 0, 0,-4, 1, -100.0, 0.0, -1.0, 56.0, 0.0, 0.0},
+ { 0, 2, 2,-2, 1, 87.0, 0.0, 0.0, -47.0, 0.0, 0.0},
+ {-3, 0, 0, 4, 0, 161.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ {-1, 1, 2, 0, 1, 96.0, 0.0, 0.0, -50.0, 0.0, 0.0},
+ {-1,-1, 0, 4, 0, 151.0, 0.0, -1.0, -5.0, 0.0, 0.0},
+
+ /* 201-210 */
+ {-1,-2, 2, 2, 2, -104.0, 0.0, 0.0, 44.0, 0.0, 0.0},
+ {-2,-1, 2, 4, 2, -110.0, 0.0, 0.0, 48.0, 0.0, 0.0},
+ { 1,-1, 2, 2, 1, -100.0, 0.0, 1.0, 50.0, 0.0, 0.0},
+ {-2, 1, 0, 2, 0, 92.0, 0.0, -5.0, 12.0, 0.0, -2.0},
+ {-2, 1, 2, 0, 1, 82.0, 0.0, 0.0, -45.0, 0.0, 0.0},
+ { 2, 1, 0,-2, 1, 82.0, 0.0, 0.0, -45.0, 0.0, 0.0},
+ {-3, 0, 2, 0, 1, -78.0, 0.0, 0.0, 41.0, 0.0, 0.0},
+ {-2, 0, 2,-2, 1, -77.0, 0.0, 0.0, 43.0, 0.0, 0.0},
+ {-1, 1, 0, 2, 2, 2.0, 0.0, 0.0, 54.0, 0.0, 0.0},
+ { 0,-1, 2,-1, 2, 94.0, 0.0, 0.0, -40.0, 0.0, 0.0},
+
+ /* 211-220 */
+ {-1, 0, 4,-2, 2, -93.0, 0.0, 0.0, 40.0, 0.0, 0.0},
+ { 0,-2, 2, 0, 2, -83.0, 0.0, 10.0, 40.0, 0.0, -2.0},
+ {-1, 0, 2, 1, 2, 83.0, 0.0, 0.0, -36.0, 0.0, 0.0},
+ { 2, 0, 0, 0, 2, -91.0, 0.0, 0.0, 39.0, 0.0, 0.0},
+ { 0, 0, 2, 0, 3, 128.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ {-2, 0, 4, 0, 2, -79.0, 0.0, 0.0, 34.0, 0.0, 0.0},
+ {-1, 0,-2, 0, 1, -83.0, 0.0, 0.0, 47.0, 0.0, 0.0},
+ {-1, 1, 2, 2, 1, 84.0, 0.0, 0.0, -44.0, 0.0, 0.0},
+ { 3, 0, 0, 0, 1, 83.0, 0.0, 0.0, -43.0, 0.0, 0.0},
+ {-1, 0, 2, 3, 2, 91.0, 0.0, 0.0, -39.0, 0.0, 0.0},
+
+ /* 221-230 */
+ { 2,-1, 2, 0, 1, -77.0, 0.0, 0.0, 39.0, 0.0, 0.0},
+ { 0, 1, 2, 2, 1, 84.0, 0.0, 0.0, -43.0, 0.0, 0.0},
+ { 0,-1, 2, 4, 2, -92.0, 0.0, 1.0, 39.0, 0.0, 0.0},
+ { 2,-1, 2, 2, 2, -92.0, 0.0, 1.0, 39.0, 0.0, 0.0},
+ { 0, 2,-2, 2, 0, -94.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1,-1, 2,-1, 1, 68.0, 0.0, 0.0, -36.0, 0.0, 0.0},
+ { 0,-2, 0, 0, 1, -61.0, 0.0, 0.0, 32.0, 0.0, 0.0},
+ { 1, 0, 2,-4, 2, 71.0, 0.0, 0.0, -31.0, 0.0, 0.0},
+ { 1,-1, 0,-2, 1, 62.0, 0.0, 0.0, -34.0, 0.0, 0.0},
+ {-1,-1, 2, 0, 1, -63.0, 0.0, 0.0, 33.0, 0.0, 0.0},
+
+ /* 231-240 */
+ { 1,-1, 2,-2, 2, -73.0, 0.0, 0.0, 32.0, 0.0, 0.0},
+ {-2,-1, 0, 4, 0, 115.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ {-1, 0, 0, 3, 0, -103.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-2,-1, 2, 2, 2, 63.0, 0.0, 0.0, -28.0, 0.0, 0.0},
+ { 0, 2, 2, 0, 2, 74.0, 0.0, 0.0, -32.0, 0.0, 0.0},
+ { 1, 1, 0, 2, 0, -103.0, 0.0, -3.0, 3.0, 0.0, -1.0},
+ { 2, 0, 2,-1, 2, -69.0, 0.0, 0.0, 30.0, 0.0, 0.0},
+ { 1, 0, 2, 1, 1, 57.0, 0.0, 0.0, -29.0, 0.0, 0.0},
+ { 4, 0, 0, 0, 0, 94.0, 0.0, 0.0, -4.0, 0.0, 0.0},
+ { 2, 1, 2, 0, 1, 64.0, 0.0, 0.0, -33.0, 0.0, 0.0},
+
+ /* 241-250 */
+ { 3,-1, 2, 0, 2, -63.0, 0.0, 0.0, 26.0, 0.0, 0.0},
+ {-2, 2, 0, 2, 1, -38.0, 0.0, 0.0, 20.0, 0.0, 0.0},
+ { 1, 0, 2,-3, 1, -43.0, 0.0, 0.0, 24.0, 0.0, 0.0},
+ { 1, 1, 2,-4, 1, -45.0, 0.0, 0.0, 23.0, 0.0, 0.0},
+ {-1,-1, 2,-2, 1, 47.0, 0.0, 0.0, -24.0, 0.0, 0.0},
+ { 0,-1, 0,-1, 1, -48.0, 0.0, 0.0, 25.0, 0.0, 0.0},
+ { 0,-1, 0,-2, 1, 45.0, 0.0, 0.0, -26.0, 0.0, 0.0},
+ {-2, 0, 0, 0, 2, 56.0, 0.0, 0.0, -25.0, 0.0, 0.0},
+ {-2, 0,-2, 2, 0, 88.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-1, 0,-2, 4, 0, -75.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+
+ /* 251-260 */
+ { 1,-2, 0, 0, 0, 85.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 1, 0, 1, 1, 49.0, 0.0, 0.0, -26.0, 0.0, 0.0},
+ {-1, 2, 0, 2, 0, -74.0, 0.0, -3.0, -1.0, 0.0, -1.0},
+ { 1,-1, 2,-2, 1, -39.0, 0.0, 0.0, 21.0, 0.0, 0.0},
+ { 1, 2, 2,-2, 2, 45.0, 0.0, 0.0, -20.0, 0.0, 0.0},
+ { 2,-1, 2,-2, 2, 51.0, 0.0, 0.0, -22.0, 0.0, 0.0},
+ { 1, 0, 2,-1, 1, -40.0, 0.0, 0.0, 21.0, 0.0, 0.0},
+ { 2, 1, 2,-2, 1, 41.0, 0.0, 0.0, -21.0, 0.0, 0.0},
+ {-2, 0, 0,-2, 1, -42.0, 0.0, 0.0, 24.0, 0.0, 0.0},
+ { 1,-2, 2, 0, 2, -51.0, 0.0, 0.0, 22.0, 0.0, 0.0},
+
+ /* 261-270 */
+ { 0, 1, 2, 1, 1, -42.0, 0.0, 0.0, 22.0, 0.0, 0.0},
+ { 1, 0, 4,-2, 1, 39.0, 0.0, 0.0, -21.0, 0.0, 0.0},
+ {-2, 0, 4, 2, 2, 46.0, 0.0, 0.0, -18.0, 0.0, 0.0},
+ { 1, 1, 2, 1, 2, -53.0, 0.0, 0.0, 22.0, 0.0, 0.0},
+ { 1, 0, 0, 4, 0, 82.0, 0.0, 0.0, -4.0, 0.0, 0.0},
+ { 1, 0, 2, 2, 0, 81.0, 0.0, -1.0, -4.0, 0.0, 0.0},
+ { 2, 0, 2, 1, 2, 47.0, 0.0, 0.0, -19.0, 0.0, 0.0},
+ { 3, 1, 2, 0, 2, 53.0, 0.0, 0.0, -23.0, 0.0, 0.0},
+ { 4, 0, 2, 0, 1, -45.0, 0.0, 0.0, 22.0, 0.0, 0.0},
+ {-2,-1, 2, 0, 0, -44.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+
+ /* 271-280 */
+ { 0, 1,-2, 2, 1, -33.0, 0.0, 0.0, 16.0, 0.0, 0.0},
+ { 1, 0,-2, 1, 0, -61.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ { 0,-1,-2, 2, 1, 28.0, 0.0, 0.0, -15.0, 0.0, 0.0},
+ { 2,-1, 0,-2, 1, -38.0, 0.0, 0.0, 19.0, 0.0, 0.0},
+ {-1, 0, 2,-1, 2, -33.0, 0.0, 0.0, 21.0, 0.0, 0.0},
+ { 1, 0, 2,-3, 2, -60.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 1, 2,-2, 3, 48.0, 0.0, 0.0, -10.0, 0.0, 0.0},
+ { 0, 0, 2,-3, 1, 27.0, 0.0, 0.0, -14.0, 0.0, 0.0},
+ {-1, 0,-2, 2, 1, 38.0, 0.0, 0.0, -20.0, 0.0, 0.0},
+ { 0, 0, 2,-4, 2, 31.0, 0.0, 0.0, -13.0, 0.0, 0.0},
+
+ /* 281-290 */
+ {-2, 1, 0, 0, 1, -29.0, 0.0, 0.0, 15.0, 0.0, 0.0},
+ {-1, 0, 0,-1, 1, 28.0, 0.0, 0.0, -15.0, 0.0, 0.0},
+ { 2, 0, 2,-4, 2, -32.0, 0.0, 0.0, 15.0, 0.0, 0.0},
+ { 0, 0, 4,-4, 4, 45.0, 0.0, 0.0, -8.0, 0.0, 0.0},
+ { 0, 0, 4,-4, 2, -44.0, 0.0, 0.0, 19.0, 0.0, 0.0},
+ {-1,-2, 0, 2, 1, 28.0, 0.0, 0.0, -15.0, 0.0, 0.0},
+ {-2, 0, 0, 3, 0, -51.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1, 0,-2, 2, 1, -36.0, 0.0, 0.0, 20.0, 0.0, 0.0},
+ {-3, 0, 2, 2, 2, 44.0, 0.0, 0.0, -19.0, 0.0, 0.0},
+ {-3, 0, 2, 2, 1, 26.0, 0.0, 0.0, -14.0, 0.0, 0.0},
+
+ /* 291-300 */
+ {-2, 0, 2, 2, 0, -60.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 2,-1, 0, 0, 1, 35.0, 0.0, 0.0, -18.0, 0.0, 0.0},
+ {-2, 1, 2, 2, 2, -27.0, 0.0, 0.0, 11.0, 0.0, 0.0},
+ { 1, 1, 0, 1, 0, 47.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 0, 1, 4,-2, 2, 36.0, 0.0, 0.0, -15.0, 0.0, 0.0},
+ {-1, 1, 0,-2, 1, -36.0, 0.0, 0.0, 20.0, 0.0, 0.0},
+ { 0, 0, 0,-4, 1, -35.0, 0.0, 0.0, 19.0, 0.0, 0.0},
+ { 1,-1, 0, 2, 1, -37.0, 0.0, 0.0, 19.0, 0.0, 0.0},
+ { 1, 1, 0, 2, 1, 32.0, 0.0, 0.0, -16.0, 0.0, 0.0},
+ {-1, 2, 2, 2, 2, 35.0, 0.0, 0.0, -14.0, 0.0, 0.0},
+
+ /* 301-310 */
+ { 3, 1, 2,-2, 2, 32.0, 0.0, 0.0, -13.0, 0.0, 0.0},
+ { 0,-1, 0, 4, 0, 65.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 2,-1, 0, 2, 0, 47.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 0, 0, 4, 0, 1, 32.0, 0.0, 0.0, -16.0, 0.0, 0.0},
+ { 2, 0, 4,-2, 2, 37.0, 0.0, 0.0, -16.0, 0.0, 0.0},
+ {-1,-1, 2, 4, 1, -30.0, 0.0, 0.0, 15.0, 0.0, 0.0},
+ { 1, 0, 0, 4, 1, -32.0, 0.0, 0.0, 16.0, 0.0, 0.0},
+ { 1,-2, 2, 2, 2, -31.0, 0.0, 0.0, 13.0, 0.0, 0.0},
+ { 0, 0, 2, 3, 2, 37.0, 0.0, 0.0, -16.0, 0.0, 0.0},
+ {-1, 1, 2, 4, 2, 31.0, 0.0, 0.0, -13.0, 0.0, 0.0},
+
+ /* 311-320 */
+ { 3, 0, 0, 2, 0, 49.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ {-1, 0, 4, 2, 2, 32.0, 0.0, 0.0, -13.0, 0.0, 0.0},
+ { 1, 1, 2, 2, 1, 23.0, 0.0, 0.0, -12.0, 0.0, 0.0},
+ {-2, 0, 2, 6, 2, -43.0, 0.0, 0.0, 18.0, 0.0, 0.0},
+ { 2, 1, 2, 2, 2, 26.0, 0.0, 0.0, -11.0, 0.0, 0.0},
+ {-1, 0, 2, 6, 2, -32.0, 0.0, 0.0, 14.0, 0.0, 0.0},
+ { 1, 0, 2, 4, 1, -29.0, 0.0, 0.0, 14.0, 0.0, 0.0},
+ { 2, 0, 2, 4, 2, -27.0, 0.0, 0.0, 12.0, 0.0, 0.0},
+ { 1, 1,-2, 1, 0, 30.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-3, 1, 2, 1, 2, -11.0, 0.0, 0.0, 5.0, 0.0, 0.0},
+
+ /* 321-330 */
+ { 2, 0,-2, 0, 2, -21.0, 0.0, 0.0, 10.0, 0.0, 0.0},
+ {-1, 0, 0, 1, 2, -34.0, 0.0, 0.0, 15.0, 0.0, 0.0},
+ {-4, 0, 2, 2, 1, -10.0, 0.0, 0.0, 6.0, 0.0, 0.0},
+ {-1,-1, 0, 1, 0, -36.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 0,-2, 2, 2, -9.0, 0.0, 0.0, 4.0, 0.0, 0.0},
+ { 1, 0, 0,-1, 2, -12.0, 0.0, 0.0, 5.0, 0.0, 0.0},
+ { 0,-1, 2,-2, 3, -21.0, 0.0, 0.0, 5.0, 0.0, 0.0},
+ {-2, 1, 2, 0, 0, -29.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 0, 0, 2,-2, 4, -15.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ {-2,-2, 0, 2, 0, -20.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+
+ /* 331-340 */
+ {-2, 0,-2, 4, 0, 28.0, 0.0, 0.0, 0.0, 0.0, -2.0},
+ { 0,-2,-2, 2, 0, 17.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1, 2, 0,-2, 1, -22.0, 0.0, 0.0, 12.0, 0.0, 0.0},
+ { 3, 0, 0,-4, 1, -14.0, 0.0, 0.0, 7.0, 0.0, 0.0},
+ {-1, 1, 2,-2, 2, 24.0, 0.0, 0.0, -11.0, 0.0, 0.0},
+ { 1,-1, 2,-4, 1, 11.0, 0.0, 0.0, -6.0, 0.0, 0.0},
+ { 1, 1, 0,-2, 2, 14.0, 0.0, 0.0, -6.0, 0.0, 0.0},
+ {-3, 0, 2, 0, 0, 24.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-3, 0, 2, 0, 2, 18.0, 0.0, 0.0, -8.0, 0.0, 0.0},
+ {-2, 0, 0, 1, 0, -38.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+
+ /* 341-350 */
+ { 0, 0,-2, 1, 0, -31.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-3, 0, 0, 2, 1, -16.0, 0.0, 0.0, 8.0, 0.0, 0.0},
+ {-1,-1,-2, 2, 0, 29.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 1, 2,-4, 1, -18.0, 0.0, 0.0, 10.0, 0.0, 0.0},
+ { 2, 1, 0,-4, 1, -10.0, 0.0, 0.0, 5.0, 0.0, 0.0},
+ { 0, 2, 0,-2, 1, -17.0, 0.0, 0.0, 10.0, 0.0, 0.0},
+ { 1, 0, 0,-3, 1, 9.0, 0.0, 0.0, -4.0, 0.0, 0.0},
+ {-2, 0, 2,-2, 2, 16.0, 0.0, 0.0, -6.0, 0.0, 0.0},
+ {-2,-1, 0, 0, 1, 22.0, 0.0, 0.0, -12.0, 0.0, 0.0},
+ {-4, 0, 0, 2, 0, 20.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+
+ /* 351-360 */
+ { 1, 1, 0,-4, 1, -13.0, 0.0, 0.0, 6.0, 0.0, 0.0},
+ {-1, 0, 2,-4, 1, -17.0, 0.0, 0.0, 9.0, 0.0, 0.0},
+ { 0, 0, 4,-4, 1, -14.0, 0.0, 0.0, 8.0, 0.0, 0.0},
+ { 0, 3, 2,-2, 2, 0.0, 0.0, 0.0, -7.0, 0.0, 0.0},
+ {-3,-1, 0, 4, 0, 14.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-3, 0, 0, 4, 1, 19.0, 0.0, 0.0, -10.0, 0.0, 0.0},
+ { 1,-1,-2, 2, 0, -34.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1,-1, 0, 2, 2, -20.0, 0.0, 0.0, 8.0, 0.0, 0.0},
+ { 1,-2, 0, 0, 1, 9.0, 0.0, 0.0, -5.0, 0.0, 0.0},
+ { 1,-1, 0, 0, 2, -18.0, 0.0, 0.0, 7.0, 0.0, 0.0},
+
+ /* 361-370 */
+ { 0, 0, 0, 1, 2, 13.0, 0.0, 0.0, -6.0, 0.0, 0.0},
+ {-1,-1, 2, 0, 0, 17.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1,-2, 2,-2, 2, -12.0, 0.0, 0.0, 5.0, 0.0, 0.0},
+ { 0,-1, 2,-1, 1, 15.0, 0.0, 0.0, -8.0, 0.0, 0.0},
+ {-1, 0, 2, 0, 3, -11.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ { 1, 1, 0, 0, 2, 13.0, 0.0, 0.0, -5.0, 0.0, 0.0},
+ {-1, 1, 2, 0, 0, -18.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1, 2, 0, 0, 0, -35.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1, 2, 2, 0, 2, 9.0, 0.0, 0.0, -4.0, 0.0, 0.0},
+ {-1, 0, 4,-2, 1, -19.0, 0.0, 0.0, 10.0, 0.0, 0.0},
+
+ /* 371-380 */
+ { 3, 0, 2,-4, 2, -26.0, 0.0, 0.0, 11.0, 0.0, 0.0},
+ { 1, 2, 2,-2, 1, 8.0, 0.0, 0.0, -4.0, 0.0, 0.0},
+ { 1, 0, 4,-4, 2, -10.0, 0.0, 0.0, 4.0, 0.0, 0.0},
+ {-2,-1, 0, 4, 1, 10.0, 0.0, 0.0, -6.0, 0.0, 0.0},
+ { 0,-1, 0, 2, 2, -21.0, 0.0, 0.0, 9.0, 0.0, 0.0},
+ {-2, 1, 0, 4, 0, -15.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-2,-1, 2, 2, 1, 9.0, 0.0, 0.0, -5.0, 0.0, 0.0},
+ { 2, 0,-2, 2, 0, -29.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1, 0, 0, 1, 1, -19.0, 0.0, 0.0, 10.0, 0.0, 0.0},
+ { 0, 1, 0, 2, 2, 12.0, 0.0, 0.0, -5.0, 0.0, 0.0},
+
+ /* 381-390 */
+ { 1,-1, 2,-1, 2, 22.0, 0.0, 0.0, -9.0, 0.0, 0.0},
+ {-2, 0, 4, 0, 1, -10.0, 0.0, 0.0, 5.0, 0.0, 0.0},
+ { 2, 1, 0, 0, 1, -20.0, 0.0, 0.0, 11.0, 0.0, 0.0},
+ { 0, 1, 2, 0, 0, -20.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0,-1, 4,-2, 2, -17.0, 0.0, 0.0, 7.0, 0.0, 0.0},
+ { 0, 0, 4,-2, 4, 15.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 0, 2, 2, 0, 1, 8.0, 0.0, 0.0, -4.0, 0.0, 0.0},
+ {-3, 0, 0, 6, 0, 14.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1,-1, 0, 4, 1, -12.0, 0.0, 0.0, 6.0, 0.0, 0.0},
+ { 1,-2, 0, 2, 0, 25.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+
+ /* 391-400 */
+ {-1, 0, 0, 4, 2, -13.0, 0.0, 0.0, 6.0, 0.0, 0.0},
+ {-1,-2, 2, 2, 1, -14.0, 0.0, 0.0, 8.0, 0.0, 0.0},
+ {-1, 0, 0,-2, 2, 13.0, 0.0, 0.0, -5.0, 0.0, 0.0},
+ { 1, 0,-2,-2, 1, -17.0, 0.0, 0.0, 9.0, 0.0, 0.0},
+ { 0, 0,-2,-2, 1, -12.0, 0.0, 0.0, 6.0, 0.0, 0.0},
+ {-2, 0,-2, 0, 1, -10.0, 0.0, 0.0, 5.0, 0.0, 0.0},
+ { 0, 0, 0, 3, 1, 10.0, 0.0, 0.0, -6.0, 0.0, 0.0},
+ { 0, 0, 0, 3, 0, -15.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1, 1, 0, 4, 0, -22.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1,-1, 2, 2, 0, 28.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+
+ /* 401-410 */
+ {-2, 0, 2, 3, 2, 15.0, 0.0, 0.0, -7.0, 0.0, 0.0},
+ { 1, 0, 0, 2, 2, 23.0, 0.0, 0.0, -10.0, 0.0, 0.0},
+ { 0,-1, 2, 1, 2, 12.0, 0.0, 0.0, -5.0, 0.0, 0.0},
+ { 3,-1, 0, 0, 0, 29.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 2, 0, 0, 1, 0, -25.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ { 1,-1, 2, 0, 0, 22.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 0, 2, 1, 0, -18.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1, 0, 2, 0, 3, 15.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ { 3, 1, 0, 0, 0, -23.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 3,-1, 2,-2, 2, 12.0, 0.0, 0.0, -5.0, 0.0, 0.0},
+
+ /* 411-420 */
+ { 2, 0, 2,-1, 1, -8.0, 0.0, 0.0, 4.0, 0.0, 0.0},
+ { 1, 1, 2, 0, 0, -19.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 0, 4,-1, 2, -10.0, 0.0, 0.0, 4.0, 0.0, 0.0},
+ { 1, 2, 2, 0, 2, 21.0, 0.0, 0.0, -9.0, 0.0, 0.0},
+ {-2, 0, 0, 6, 0, 23.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 0,-1, 0, 4, 1, -16.0, 0.0, 0.0, 8.0, 0.0, 0.0},
+ {-2,-1, 2, 4, 1, -19.0, 0.0, 0.0, 9.0, 0.0, 0.0},
+ { 0,-2, 2, 2, 1, -22.0, 0.0, 0.0, 10.0, 0.0, 0.0},
+ { 0,-1, 2, 2, 0, 27.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ {-1, 0, 2, 3, 1, 16.0, 0.0, 0.0, -8.0, 0.0, 0.0},
+
+ /* 421-430 */
+ {-2, 1, 2, 4, 2, 19.0, 0.0, 0.0, -8.0, 0.0, 0.0},
+ { 2, 0, 0, 2, 2, 9.0, 0.0, 0.0, -4.0, 0.0, 0.0},
+ { 2,-2, 2, 0, 2, -9.0, 0.0, 0.0, 4.0, 0.0, 0.0},
+ {-1, 1, 2, 3, 2, -9.0, 0.0, 0.0, 4.0, 0.0, 0.0},
+ { 3, 0, 2,-1, 2, -8.0, 0.0, 0.0, 4.0, 0.0, 0.0},
+ { 4, 0, 2,-2, 1, 18.0, 0.0, 0.0, -9.0, 0.0, 0.0},
+ {-1, 0, 0, 6, 0, 16.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ {-1,-2, 2, 4, 2, -10.0, 0.0, 0.0, 4.0, 0.0, 0.0},
+ {-3, 0, 2, 6, 2, -23.0, 0.0, 0.0, 9.0, 0.0, 0.0},
+ {-1, 0, 2, 4, 0, 16.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+
+ /* 431-440 */
+ { 3, 0, 0, 2, 1, -12.0, 0.0, 0.0, 6.0, 0.0, 0.0},
+ { 3,-1, 2, 0, 1, -8.0, 0.0, 0.0, 4.0, 0.0, 0.0},
+ { 3, 0, 2, 0, 0, 30.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 1, 0, 4, 0, 2, 24.0, 0.0, 0.0, -10.0, 0.0, 0.0},
+ { 5, 0, 2,-2, 2, 10.0, 0.0, 0.0, -4.0, 0.0, 0.0},
+ { 0,-1, 2, 4, 1, -16.0, 0.0, 0.0, 7.0, 0.0, 0.0},
+ { 2,-1, 2, 2, 1, -16.0, 0.0, 0.0, 7.0, 0.0, 0.0},
+ { 0, 1, 2, 4, 2, 17.0, 0.0, 0.0, -7.0, 0.0, 0.0},
+ { 1,-1, 2, 4, 2, -24.0, 0.0, 0.0, 10.0, 0.0, 0.0},
+ { 3,-1, 2, 2, 2, -12.0, 0.0, 0.0, 5.0, 0.0, 0.0},
+
+ /* 441-450 */
+ { 3, 0, 2, 2, 1, -24.0, 0.0, 0.0, 11.0, 0.0, 0.0},
+ { 5, 0, 2, 0, 2, -23.0, 0.0, 0.0, 9.0, 0.0, 0.0},
+ { 0, 0, 2, 6, 2, -13.0, 0.0, 0.0, 5.0, 0.0, 0.0},
+ { 4, 0, 2, 2, 2, -15.0, 0.0, 0.0, 7.0, 0.0, 0.0},
+ { 0,-1, 1,-1, 1, 0.0, 0.0,-1988.0, 0.0, 0.0,-1679.0},
+ {-1, 0, 1, 0, 3, 0.0, 0.0, -63.0, 0.0, 0.0, -27.0},
+ { 0,-2, 2,-2, 3, -4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1, 0,-1, 0, 1, 0.0, 0.0, 5.0, 0.0, 0.0, 4.0},
+ { 2,-2, 0,-2, 1, 5.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ {-1, 0, 1, 0, 2, 0.0, 0.0, 364.0, 0.0, 0.0, 176.0},
+
+ /* 451-460 */
+ {-1, 0, 1, 0, 1, 0.0, 0.0,-1044.0, 0.0, 0.0, -891.0},
+ {-1,-1, 2,-1, 2, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ {-2, 2, 0, 2, 2, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ {-1, 0, 1, 0, 0, 0.0, 0.0, 330.0, 0.0, 0.0, 0.0},
+ {-4, 1, 2, 2, 2, 5.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ {-3, 0, 2, 1, 1, 3.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ {-2,-1, 2, 0, 2, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ { 1, 0,-2, 1, 1, -5.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 2,-1,-2, 0, 1, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ {-4, 0, 2, 2, 0, 3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+
+ /* 461-470 */
+ {-3, 1, 0, 3, 0, 3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1, 0,-1, 2, 0, 0.0, 0.0, 5.0, 0.0, 0.0, 0.0},
+ { 0,-2, 0, 0, 2, 0.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ { 0,-2, 0, 0, 2, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ {-3, 0, 0, 3, 0, 6.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-2,-1, 0, 2, 2, 5.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ {-1, 0,-2, 3, 0, -7.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-4, 0, 0, 4, 0, -12.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 2, 1,-2, 0, 1, 5.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 2,-1, 0,-2, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+
+ /* 471-480 */
+ { 0, 0, 1,-1, 0, -5.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1, 2, 0, 1, 0, 3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-2, 1, 2, 0, 2, -7.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ { 1, 1, 0,-1, 1, 7.0, 0.0, 0.0, -4.0, 0.0, 0.0},
+ { 1, 0, 1,-2, 1, 0.0, 0.0, -12.0, 0.0, 0.0, -10.0},
+ { 0, 2, 0, 0, 2, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 1,-1, 2,-3, 1, 3.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ {-1, 1, 2,-1, 1, -3.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-2, 0, 4,-2, 2, -7.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ {-2, 0, 4,-2, 1, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+
+ /* 481-490 */
+ {-2,-2, 0, 2, 1, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ {-2, 0,-2, 4, 0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1, 2, 2,-4, 1, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ { 1, 1, 2,-4, 2, 7.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ {-1, 2, 2,-2, 1, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 2, 0, 0,-3, 1, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ {-1, 2, 0, 0, 1, -5.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ { 0, 0, 0,-2, 0, 5.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1,-1, 2,-2, 2, -5.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-1, 1, 0, 0, 2, 5.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+
+ /* 491-500 */
+ { 0, 0, 0,-1, 2, -8.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ {-2, 1, 0, 1, 0, 9.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1,-2, 0,-2, 1, 6.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 1, 0,-2, 0, 2, -5.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-3, 1, 0, 2, 0, 3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1, 1,-2, 2, 0, -7.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1,-1, 0, 0, 2, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ {-3, 0, 0, 2, 0, 5.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-3,-1, 0, 2, 0, 3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 2, 0, 2,-6, 1, -3.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+
+ /* 501-510 */
+ { 0, 1, 2,-4, 2, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 2, 0, 0,-4, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ {-2, 1, 2,-2, 1, -5.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 0,-1, 2,-4, 1, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 0, 1, 0,-2, 2, 9.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ {-1, 0, 0,-2, 0, 4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 2, 0,-2,-2, 1, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ {-4, 0, 2, 0, 1, -3.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-1,-1, 0,-1, 1, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 0, 0,-2, 0, 2, 9.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+
+ /* 511-520 */
+ {-3, 0, 0, 1, 0, -4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1, 0,-2, 1, 0, -4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-2, 0,-2, 2, 1, 3.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 0, 0,-4, 2, 0, 8.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-2,-1,-2, 2, 0, 3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1, 0, 2,-6, 1, -3.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-1, 0, 2,-4, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 1, 0, 0,-4, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 2, 1, 2,-4, 2, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ { 2, 1, 2,-4, 1, 6.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+
+ /* 521-530 */
+ { 0, 1, 4,-4, 4, 3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 1, 4,-4, 2, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ {-1,-1,-2, 4, 0, -7.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1,-3, 0, 2, 0, 9.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1, 0,-2, 4, 1, -3.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-2,-1, 0, 3, 0, -3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 0,-2, 3, 0, -4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-2, 0, 0, 3, 1, -5.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ { 0,-1, 0, 1, 0, -13.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-3, 0, 2, 2, 0, -7.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+
+ /* 531-540 */
+ { 1, 1,-2, 2, 0, 10.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1, 1, 0, 2, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 1,-2, 2,-2, 1, 10.0, 0.0, 13.0, 6.0, 0.0, -5.0},
+ { 0, 0, 1, 0, 2, 0.0, 0.0, 30.0, 0.0, 0.0, 14.0},
+ { 0, 0, 1, 0, 1, 0.0, 0.0, -162.0, 0.0, 0.0, -138.0},
+ { 0, 0, 1, 0, 0, 0.0, 0.0, 75.0, 0.0, 0.0, 0.0},
+ {-1, 2, 0, 2, 1, -7.0, 0.0, 0.0, 4.0, 0.0, 0.0},
+ { 0, 0, 2, 0, 2, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-2, 0, 2, 0, 2, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 2, 0, 0,-1, 1, 5.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+
+ /* 541-550 */
+ { 3, 0, 0,-2, 1, 5.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 1, 0, 2,-2, 3, -3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1, 2, 0, 0, 1, -3.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 2, 0, 2,-3, 2, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-1, 1, 4,-2, 2, -5.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-2,-2, 0, 4, 0, 6.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0,-3, 0, 2, 0, 9.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 0,-2, 4, 0, 5.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1,-1, 0, 3, 0, -7.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-2, 0, 0, 4, 2, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+
+ /* 551-560 */
+ {-1, 0, 0, 3, 1, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 2,-2, 0, 0, 0, 7.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1,-1, 0, 1, 0, -4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1, 0, 0, 2, 0, 4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0,-2, 2, 0, 1, -6.0, 0.0, -3.0, 3.0, 0.0, 1.0},
+ {-1, 0, 1, 2, 1, 0.0, 0.0, -3.0, 0.0, 0.0, -2.0},
+ {-1, 1, 0, 3, 0, 11.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1,-1, 2, 1, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 0,-1, 2, 0, 0, 11.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-2, 1, 2, 2, 1, -3.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+
+ /* 561-570 */
+ { 2,-2, 2,-2, 2, -1.0, 0.0, 3.0, 3.0, 0.0, -1.0},
+ { 1, 1, 0, 1, 1, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 1, 0, 1, 0, 1, 0.0, 0.0, -13.0, 0.0, 0.0, -11.0},
+ { 1, 0, 1, 0, 0, 3.0, 0.0, 6.0, 0.0, 0.0, 0.0},
+ { 0, 2, 0, 2, 0, -7.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 2,-1, 2,-2, 1, 5.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 0,-1, 4,-2, 1, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ { 0, 0, 4,-2, 3, 3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 1, 4,-2, 1, 5.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 4, 0, 2,-4, 2, -7.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+
+ /* 571-580 */
+ { 2, 2, 2,-2, 2, 8.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 2, 0, 4,-4, 2, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-1,-2, 0, 4, 0, 11.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1,-3, 2, 2, 2, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ {-3, 0, 2, 4, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ {-3, 0, 2,-2, 1, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-1,-1, 0,-2, 1, 8.0, 0.0, 0.0, -4.0, 0.0, 0.0},
+ {-3, 0, 0, 0, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ {-3, 0,-2, 2, 0, 11.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 1, 0,-4, 1, -6.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+
+ /* 581-590 */
+ {-2, 1, 0,-2, 1, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-4, 0, 0, 0, 1, -8.0, 0.0, 0.0, 4.0, 0.0, 0.0},
+ {-1, 0, 0,-4, 1, -7.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ {-3, 0, 0,-2, 1, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 0, 0, 0, 3, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ {-1, 1, 0, 4, 1, 6.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 1,-2, 2, 0, 1, -6.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ { 0, 1, 0, 3, 0, 6.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-1, 0, 2, 2, 3, 6.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 0, 0, 2, 2, 2, 5.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+
+ /* 591-600 */
+ {-2, 0, 2, 2, 2, -5.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-1, 1, 2, 2, 0, -4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 3, 0, 0, 0, 2, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 2, 1, 0, 1, 0, 4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 2,-1, 2,-1, 2, 6.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 0, 0, 2, 0, 1, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 0, 0, 3, 0, 3, 0.0, 0.0, -26.0, 0.0, 0.0, -11.0},
+ { 0, 0, 3, 0, 2, 0.0, 0.0, -10.0, 0.0, 0.0, -5.0},
+ {-1, 2, 2, 2, 1, 5.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ {-1, 0, 4, 0, 0, -13.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+
+ /* 601-610 */
+ { 1, 2, 2, 0, 1, 3.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 3, 1, 2,-2, 1, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 1, 1, 4,-2, 2, 7.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ {-2,-1, 0, 6, 0, 4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0,-2, 0, 4, 0, 5.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-2, 0, 0, 6, 1, -3.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-2,-2, 2, 4, 2, -6.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 0,-3, 2, 2, 2, -5.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 0, 0, 0, 4, 2, -7.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ {-1,-1, 2, 3, 2, 5.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+
+ /* 611-620 */
+ {-2, 0, 2, 4, 0, 13.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 2,-1, 0, 2, 1, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 1, 0, 0, 3, 0, -3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 1, 0, 4, 1, 5.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 0, 1, 0, 4, 0, -11.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1,-1, 2, 1, 2, 5.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 0, 0, 2, 2, 3, 4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1, 0, 2, 2, 2, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ {-1, 0, 2, 2, 2, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-2, 0, 4, 2, 1, 6.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+
+ /* 621-630 */
+ { 2, 1, 0, 2, 1, 3.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 2, 1, 0, 2, 0, -12.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 2,-1, 2, 0, 0, 4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1, 0, 2, 1, 0, -3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 1, 2, 2, 0, -4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 2, 0, 2, 0, 3, 3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 3, 0, 2, 0, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 1, 0, 2, 0, 2, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ { 1, 0, 3, 0, 3, 0.0, 0.0, -5.0, 0.0, 0.0, -2.0},
+ { 1, 1, 2, 1, 1, -7.0, 0.0, 0.0, 4.0, 0.0, 0.0},
+
+ /* 631-640 */
+ { 0, 2, 2, 2, 2, 6.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 2, 1, 2, 0, 0, -3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 2, 0, 4,-2, 1, 5.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 4, 1, 2,-2, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ {-1,-1, 0, 6, 0, 3.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ {-3,-1, 2, 6, 2, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ {-1, 0, 0, 6, 1, -5.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ {-3, 0, 2, 6, 1, -3.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 1,-1, 0, 4, 1, -3.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 1,-1, 0, 4, 0, 12.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+
+ /* 641-650 */
+ {-2, 0, 2, 5, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 1,-2, 2, 2, 1, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 3,-1, 0, 2, 0, 4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1,-1, 2, 2, 0, 6.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 0, 2, 3, 1, 5.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ {-1, 1, 2, 4, 1, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 0, 1, 2, 3, 2, -6.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ {-1, 0, 4, 2, 1, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 2, 0, 2, 1, 1, 6.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 5, 0, 0, 0, 0, 6.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+
+ /* 651-660 */
+ { 2, 1, 2, 1, 2, -6.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ { 1, 0, 4, 0, 1, 3.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 3, 1, 2, 0, 1, 7.0, 0.0, 0.0, -4.0, 0.0, 0.0},
+ { 3, 0, 4,-2, 2, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ {-2,-1, 2, 6, 2, -5.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 0, 0, 0, 6, 0, 5.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0,-2, 2, 4, 2, -6.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ {-2, 0, 2, 6, 1, -6.0, 0.0, 0.0, 3.0, 0.0, 0.0},
+ { 2, 0, 0, 4, 1, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 2, 0, 0, 4, 0, 10.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+
+ /* 661-670 */
+ { 2,-2, 2, 2, 2, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 0, 0, 2, 4, 0, 7.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 1, 0, 2, 3, 2, 7.0, 0.0, 0.0, -3.0, 0.0, 0.0},
+ { 4, 0, 0, 2, 0, 4.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 2, 0, 2, 2, 0, 11.0, 0.0, 0.0, 0.0, 0.0, 0.0},
+ { 0, 0, 4, 2, 2, 5.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 4,-1, 2, 0, 2, -6.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 3, 0, 2, 1, 2, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 2, 1, 2, 2, 1, 3.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 4, 1, 2, 0, 2, 5.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+
+ /* 671-678 */
+ {-1,-1, 2, 6, 2, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ {-1, 0, 2, 6, 1, -4.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 1,-1, 2, 4, 1, -3.0, 0.0, 0.0, 2.0, 0.0, 0.0},
+ { 1, 1, 2, 4, 2, 4.0, 0.0, 0.0, -2.0, 0.0, 0.0},
+ { 3, 1, 2, 2, 2, 3.0, 0.0, 0.0, -1.0, 0.0, 0.0},
+ { 5, 0, 2, 0, 1, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ { 2,-1, 2, 4, 2, -3.0, 0.0, 0.0, 1.0, 0.0, 0.0},
+ { 2, 0, 2, 4, 1, -3.0, 0.0, 0.0, 2.0, 0.0, 0.0}
+ };
+
+/* Number of terms in the luni-solar nutation model */
+ const int NLS = (int) (sizeof xls / sizeof xls[0]);
+
+/* ------------------------ */
+/* Planetary nutation model */
+/* ------------------------ */
+
+/* The units for the sine and cosine coefficients are */
+/* 0.1 microarcsecond */
+
+ static const struct {
+ int nl, /* coefficients of l, F, D and Omega */
+ nf,
+ nd,
+ nom,
+ nme, /* coefficients of planetary longitudes */
+ nve,
+ nea,
+ nma,
+ nju,
+ nsa,
+ nur,
+ nne,
+ npa; /* coefficient of general precession */
+ int sp,cp; /* longitude sin, cos coefficients */
+ int se,ce; /* obliquity sin, cos coefficients */
+ } xpl[] = {
+
+ /* 1-10 */
+ { 0, 0, 0, 0, 0, 0, 8,-16, 4, 5, 0, 0, 0, 1440, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -8, 16,-4,-5, 0, 0, 2, 56,-117, -42, -40},
+ { 0, 0, 0, 0, 0, 0, 8,-16, 4, 5, 0, 0, 2, 125, -43, 0, -54},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0,-1, 2, 2, 0, 5, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -4, 8,-1,-5, 0, 0, 2, 3, -7, -3, 0},
+ { 0, 0, 0, 0, 0, 0, 4, -8, 3, 0, 0, 0, 1, 3, 0, 0, -2},
+ { 0, 1,-1, 1, 0, 0, 3, -8, 3, 0, 0, 0, 0, -114, 0, 0, 61},
+ {-1, 0, 0, 0, 0, 10, -3, 0, 0, 0, 0, 0, 0, -219, 89, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 0, 0,-2, 6,-3, 0, 2, -3, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 4, -8, 3, 0, 0, 0, 0, -462,1604, 0, 0},
+
+ /* 11-20 */
+ { 0, 1,-1, 1, 0, 0, -5, 8,-3, 0, 0, 0, 0, 99, 0, 0, -53},
+ { 0, 0, 0, 0, 0, 0, -4, 8,-3, 0, 0, 0, 1, -3, 0, 0, 2},
+ { 0, 0, 0, 0, 0, 0, 4, -8, 1, 5, 0, 0, 2, 0, 6, 2, 0},
+ { 0, 0, 0, 0, 0, -5, 6, 4, 0, 0, 0, 0, 2, 3, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 2,-5, 0, 0, 2, -12, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 2,-5, 0, 0, 1, 14,-218, 117, 8},
+ { 0, 1,-1, 1, 0, 0, -1, 0, 2,-5, 0, 0, 0, 31,-481, -257, -17},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 2,-5, 0, 0, 0, -491, 128, 0, 0},
+ { 0, 1,-1, 1, 0, 0, -1, 0,-2, 5, 0, 0, 0,-3084,5123, 2735,1647},
+ { 0, 0, 0, 0, 0, 0, 0, 0,-2, 5, 0, 0, 1,-1444,2409,-1286,-771},
+
+ /* 21-30 */
+ { 0, 0, 0, 0, 0, 0, 0, 0,-2, 5, 0, 0, 2, 11, -24, -11, -9},
+ { 2,-1,-1, 0, 0, 0, 3, -7, 0, 0, 0, 0, 0, 26, -9, 0, 0},
+ { 1, 0,-2, 0, 0, 19,-21, 3, 0, 0, 0, 0, 0, 103, -60, 0, 0},
+ { 0, 1,-1, 1, 0, 2, -4, 0,-3, 0, 0, 0, 0, 0, -13, -7, 0},
+ { 1, 0,-1, 1, 0, 0, -1, 0, 2, 0, 0, 0, 0, -26, -29, -16, 14},
+ { 0, 1,-1, 1, 0, 0, -1, 0,-4,10, 0, 0, 0, 9, -27, -14, -5},
+ {-2, 0, 2, 1, 0, 0, 2, 0, 0,-5, 0, 0, 0, 12, 0, 0, -6},
+ { 0, 0, 0, 0, 0, 3, -7, 4, 0, 0, 0, 0, 0, -7, 0, 0, 0},
+ { 0,-1, 1, 0, 0, 0, 1, 0, 1,-1, 0, 0, 0, 0, 24, 0, 0},
+ {-2, 0, 2, 1, 0, 0, 2, 0,-2, 0, 0, 0, 0, 284, 0, 0,-151},
+
+ /* 31-40 */
+ {-1, 0, 0, 0, 0, 18,-16, 0, 0, 0, 0, 0, 0, 226, 101, 0, 0},
+ {-2, 1, 1, 2, 0, 0, 1, 0,-2, 0, 0, 0, 0, 0, -8, -2, 0},
+ {-1, 1,-1, 1, 0, 18,-17, 0, 0, 0, 0, 0, 0, 0, -6, -3, 0},
+ {-1, 0, 1, 1, 0, 0, 2, -2, 0, 0, 0, 0, 0, 5, 0, 0, -3},
+ { 0, 0, 0, 0, 0, -8, 13, 0, 0, 0, 0, 0, 2, -41, 175, 76, 17},
+ { 0, 2,-2, 2, 0, -8, 11, 0, 0, 0, 0, 0, 0, 0, 15, 6, 0},
+ { 0, 0, 0, 0, 0, -8, 13, 0, 0, 0, 0, 0, 1, 425, 212, -133, 269},
+ { 0, 1,-1, 1, 0, -8, 12, 0, 0, 0, 0, 0, 0, 1200, 598, 319,-641},
+ { 0, 0, 0, 0, 0, 8,-13, 0, 0, 0, 0, 0, 0, 235, 334, 0, 0},
+ { 0, 1,-1, 1, 0, 8,-14, 0, 0, 0, 0, 0, 0, 11, -12, -7, -6},
+
+ /* 41-50 */
+ { 0, 0, 0, 0, 0, 8,-13, 0, 0, 0, 0, 0, 1, 5, -6, 3, 3},
+ {-2, 0, 2, 1, 0, 0, 2, 0,-4, 5, 0, 0, 0, -5, 0, 0, 3},
+ {-2, 0, 2, 2, 0, 3, -3, 0, 0, 0, 0, 0, 0, 6, 0, 0, -3},
+ {-2, 0, 2, 0, 0, 0, 2, 0,-3, 1, 0, 0, 0, 15, 0, 0, 0},
+ { 0, 0, 0, 1, 0, 3, -5, 0, 2, 0, 0, 0, 0, 13, 0, 0, -7},
+ {-2, 0, 2, 0, 0, 0, 2, 0,-4, 3, 0, 0, 0, -6, -9, 0, 0},
+ { 0,-1, 1, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 266, -78, 0, 0},
+ { 0, 0, 0, 1, 0, 0, -1, 2, 0, 0, 0, 0, 0, -460,-435, -232, 246},
+ { 0, 1,-1, 2, 0, 0, -2, 2, 0, 0, 0, 0, 0, 0, 15, 7, 0},
+ {-1, 1, 0, 1, 0, 3, -5, 0, 0, 0, 0, 0, 0, -3, 0, 0, 2},
+
+ /* 51-60 */
+ {-1, 0, 1, 0, 0, 3, -4, 0, 0, 0, 0, 0, 0, 0, 131, 0, 0},
+ {-2, 0, 2, 0, 0, 0, 2, 0,-2,-2, 0, 0, 0, 4, 0, 0, 0},
+ {-2, 2, 0, 2, 0, 0, -5, 9, 0, 0, 0, 0, 0, 0, 3, 0, 0},
+ { 0, 1,-1, 1, 0, 0, -1, 0, 0, 0,-1, 0, 0, 0, 4, 2, 0},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 3, 0, 0},
+ { 0, 1,-1, 1, 0, 0, -1, 0, 0, 0, 0, 2, 0, -17, -19, -10, 9},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 1, -9, -11, 6, -5},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 2, -6, 0, 0, 3},
+ {-1, 0, 1, 0, 0, 0, 3, -4, 0, 0, 0, 0, 0, -16, 8, 0, 0},
+ { 0,-1, 1, 0, 0, 0, 1, 0, 0, 2, 0, 0, 0, 0, 3, 0, 0},
+
+ /* 61-70 */
+ { 0, 1,-1, 2, 0, 0, -1, 0, 0, 2, 0, 0, 0, 11, 24, 11, -5},
+ { 0, 0, 0, 1, 0, 0, -9, 17, 0, 0, 0, 0, 0, -3, -4, -2, 1},
+ { 0, 0, 0, 2, 0, -3, 5, 0, 0, 0, 0, 0, 0, 3, 0, 0, -1},
+ { 0, 1,-1, 1, 0, 0, -1, 0,-1, 2, 0, 0, 0, 0, -8, -4, 0},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 1,-2, 0, 0, 0, 0, 3, 0, 0},
+ { 1, 0,-2, 0, 0, 17,-16, 0,-2, 0, 0, 0, 0, 0, 5, 0, 0},
+ { 0, 1,-1, 1, 0, 0, -1, 0, 1,-3, 0, 0, 0, 0, 3, 2, 0},
+ {-2, 0, 2, 1, 0, 0, 5, -6, 0, 0, 0, 0, 0, -6, 4, 2, 3},
+ { 0,-2, 2, 0, 0, 0, 9,-13, 0, 0, 0, 0, 0, -3, -5, 0, 0},
+ { 0, 1,-1, 2, 0, 0, -1, 0, 0, 1, 0, 0, 0, -5, 0, 0, 2},
+
+ /* 71-80 */
+ { 0, 0, 0, 1, 0, 0, 0, 0, 0, 1, 0, 0, 0, 4, 24, 13, -2},
+ { 0,-1, 1, 0, 0, 0, 1, 0, 0, 1, 0, 0, 0, -42, 20, 0, 0},
+ { 0,-2, 2, 0, 0, 5, -6, 0, 0, 0, 0, 0, 0, -10, 233, 0, 0},
+ { 0,-1, 1, 1, 0, 5, -7, 0, 0, 0, 0, 0, 0, -3, 0, 0, 1},
+ {-2, 0, 2, 0, 0, 6, -8, 0, 0, 0, 0, 0, 0, 78, -18, 0, 0},
+ { 2, 1,-3, 1, 0, -6, 7, 0, 0, 0, 0, 0, 0, 0, 3, 1, 0},
+ { 0, 0, 0, 2, 0, 0, 0, 0, 1, 0, 0, 0, 0, 0, -3, -1, 0},
+ { 0,-1, 1, 1, 0, 0, 1, 0, 1, 0, 0, 0, 0, 0, -4, -2, 1},
+ { 0, 1,-1, 1, 0, 0, -1, 0, 0, 0, 2, 0, 0, 0, -8, -4, -1},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 1, 0, -5, 3, 0},
+
+ /* 81-90 */
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 2, -7, 0, 0, 3},
+ { 0, 0, 0, 0, 0, 0, -8, 15, 0, 0, 0, 0, 2, -14, 8, 3, 6},
+ { 0, 0, 0, 0, 0, 0, -8, 15, 0, 0, 0, 0, 1, 0, 8, -4, 0},
+ { 0, 1,-1, 1, 0, 0, -9, 15, 0, 0, 0, 0, 0, 0, 19, 10, 0},
+ { 0, 0, 0, 0, 0, 0, 8,-15, 0, 0, 0, 0, 0, 45, -22, 0, 0},
+ { 1,-1,-1, 0, 0, 0, 8,-15, 0, 0, 0, 0, 0, -3, 0, 0, 0},
+ { 2, 0,-2, 0, 0, 2, -5, 0, 0, 0, 0, 0, 0, 0, -3, 0, 0},
+ {-2, 0, 2, 0, 0, 0, 2, 0,-5, 5, 0, 0, 0, 0, 3, 0, 0},
+ { 2, 0,-2, 1, 0, 0, -6, 8, 0, 0, 0, 0, 0, 3, 5, 3, -2},
+ { 2, 0,-2, 1, 0, 0, -2, 0, 3, 0, 0, 0, 0, 89, -16, -9, -48},
+
+ /* 91-100 */
+ {-2, 1, 1, 0, 0, 0, 1, 0,-3, 0, 0, 0, 0, 0, 3, 0, 0},
+ {-2, 1, 1, 1, 0, 0, 1, 0,-3, 0, 0, 0, 0, -3, 7, 4, 2},
+ {-2, 0, 2, 0, 0, 0, 2, 0,-3, 0, 0, 0, 0, -349, -62, 0, 0},
+ {-2, 0, 2, 0, 0, 0, 6, -8, 0, 0, 0, 0, 0, -15, 22, 0, 0},
+ {-2, 0, 2, 0, 0, 0, 2, 0,-1,-5, 0, 0, 0, -3, 0, 0, 0},
+ {-1, 0, 1, 0, 0, 0, 1, 0,-1, 0, 0, 0, 0, -53, 0, 0, 0},
+ {-1, 1, 1, 1, 0,-20, 20, 0, 0, 0, 0, 0, 0, 5, 0, 0, -3},
+ { 1, 0,-2, 0, 0, 20,-21, 0, 0, 0, 0, 0, 0, 0, -8, 0, 0},
+ { 0, 0, 0, 1, 0, 0, 8,-15, 0, 0, 0, 0, 0, 15, -7, -4, -8},
+ { 0, 2,-2, 1, 0, 0,-10, 15, 0, 0, 0, 0, 0, -3, 0, 0, 1},
+
+ /* 101-110 */
+ { 0,-1, 1, 0, 0, 0, 1, 0, 1, 0, 0, 0, 0, -21, -78, 0, 0},
+ { 0, 0, 0, 1, 0, 0, 0, 0, 1, 0, 0, 0, 0, 20, -70, -37, -11},
+ { 0, 1,-1, 2, 0, 0, -1, 0, 1, 0, 0, 0, 0, 0, 6, 3, 0},
+ { 0, 1,-1, 1, 0, 0, -1, 0,-2, 4, 0, 0, 0, 5, 3, 2, -2},
+ { 2, 0,-2, 1, 0, -6, 8, 0, 0, 0, 0, 0, 0, -17, -4, -2, 9},
+ { 0,-2, 2, 1, 0, 5, -6, 0, 0, 0, 0, 0, 0, 0, 6, 3, 0},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0,-1, 0, 0, 1, 32, 15, -8, 17},
+ { 0, 1,-1, 1, 0, 0, -1, 0, 0,-1, 0, 0, 0, 174, 84, 45, -93},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 11, 56, 0, 0},
+ { 0, 1,-1, 1, 0, 0, -1, 0, 0, 1, 0, 0, 0, -66, -12, -6, 35},
+
+ /* 111-120 */
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 1, 47, 8, 4, -25},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 2, 0, 8, 4, 0},
+ { 0, 2,-2, 1, 0, 0, -9, 13, 0, 0, 0, 0, 0, 10, -22, -12, -5},
+ { 0, 0, 0, 1, 0, 0, 7,-13, 0, 0, 0, 0, 0, -3, 0, 0, 2},
+ {-2, 0, 2, 0, 0, 0, 5, -6, 0, 0, 0, 0, 0, -24, 12, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 9,-17, 0, 0, 0, 0, 0, 5, -6, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -9, 17, 0, 0, 0, 0, 2, 3, 0, 0, -2},
+ { 1, 0,-1, 1, 0, 0, -3, 4, 0, 0, 0, 0, 0, 4, 3, 1, -2},
+ { 1, 0,-1, 1, 0, -3, 4, 0, 0, 0, 0, 0, 0, 0, 29, 15, 0},
+ { 0, 0, 0, 2, 0, 0, -1, 2, 0, 0, 0, 0, 0, -5, -4, -2, 2},
+
+ /* 121-130 */
+ { 0,-1, 1, 1, 0, 0, 0, 2, 0, 0, 0, 0, 0, 8, -3, -1, -5},
+ { 0,-2, 2, 0, 1, 0, -2, 0, 0, 0, 0, 0, 0, 0, -3, 0, 0},
+ { 0, 0, 0, 0, 0, 3, -5, 0, 2, 0, 0, 0, 0, 10, 0, 0, 0},
+ {-2, 0, 2, 1, 0, 0, 2, 0,-3, 1, 0, 0, 0, 3, 0, 0, -2},
+ {-2, 0, 2, 1, 0, 3, -3, 0, 0, 0, 0, 0, 0, -5, 0, 0, 3},
+ { 0, 0, 0, 1, 0, 8,-13, 0, 0, 0, 0, 0, 0, 46, 66, 35, -25},
+ { 0,-1, 1, 0, 0, 8,-12, 0, 0, 0, 0, 0, 0, -14, 7, 0, 0},
+ { 0, 2,-2, 1, 0, -8, 11, 0, 0, 0, 0, 0, 0, 0, 3, 2, 0},
+ {-1, 0, 1, 0, 0, 0, 2, -2, 0, 0, 0, 0, 0, -5, 0, 0, 0},
+ {-1, 0, 0, 1, 0, 18,-16, 0, 0, 0, 0, 0, 0, -68, -34, -18, 36},
+
+ /* 131-140 */
+ { 0, 1,-1, 1, 0, 0, -1, 0,-1, 1, 0, 0, 0, 0, 14, 7, 0},
+ { 0, 0, 0, 1, 0, 3, -7, 4, 0, 0, 0, 0, 0, 10, -6, -3, -5},
+ {-2, 1, 1, 1, 0, 0, -3, 7, 0, 0, 0, 0, 0, -5, -4, -2, 3},
+ { 0, 1,-1, 2, 0, 0, -1, 0,-2, 5, 0, 0, 0, -3, 5, 2, 1},
+ { 0, 0, 0, 1, 0, 0, 0, 0,-2, 5, 0, 0, 0, 76, 17, 9, -41},
+ { 0, 0, 0, 1, 0, 0, -4, 8,-3, 0, 0, 0, 0, 84, 298, 159, -45},
+ { 1, 0, 0, 1, 0,-10, 3, 0, 0, 0, 0, 0, 0, 3, 0, 0, -1},
+ { 0, 2,-2, 1, 0, 0, -2, 0, 0, 0, 0, 0, 0, -3, 0, 0, 2},
+ {-1, 0, 0, 1, 0, 10, -3, 0, 0, 0, 0, 0, 0, -3, 0, 0, 1},
+ { 0, 0, 0, 1, 0, 0, 4, -8, 3, 0, 0, 0, 0, -82, 292, 156, 44},
+
+ /* 141-150 */
+ { 0, 0, 0, 1, 0, 0, 0, 0, 2,-5, 0, 0, 0, -73, 17, 9, 39},
+ { 0,-1, 1, 0, 0, 0, 1, 0, 2,-5, 0, 0, 0, -9, -16, 0, 0},
+ { 2,-1,-1, 1, 0, 0, 3, -7, 0, 0, 0, 0, 0, 3, 0, -1, -2},
+ {-2, 0, 2, 0, 0, 0, 2, 0, 0,-5, 0, 0, 0, -3, 0, 0, 0},
+ { 0, 0, 0, 1, 0, -3, 7, -4, 0, 0, 0, 0, 0, -9, -5, -3, 5},
+ {-2, 0, 2, 0, 0, 0, 2, 0,-2, 0, 0, 0, 0, -439, 0, 0, 0},
+ { 1, 0, 0, 1, 0,-18, 16, 0, 0, 0, 0, 0, 0, 57, -28, -15, -30},
+ {-2, 1, 1, 1, 0, 0, 1, 0,-2, 0, 0, 0, 0, 0, -6, -3, 0},
+ { 0, 1,-1, 2, 0, -8, 12, 0, 0, 0, 0, 0, 0, -4, 0, 0, 2},
+ { 0, 0, 0, 1, 0, -8, 13, 0, 0, 0, 0, 0, 0, -40, 57, 30, 21},
+
+ /* 151-160 */
+ { 0, 0, 0, 0, 0, 0, 1, -2, 0, 0, 0, 0, 1, 23, 7, 3, -13},
+ { 0, 1,-1, 1, 0, 0, 0, -2, 0, 0, 0, 0, 0, 273, 80, 43,-146},
+ { 0, 0, 0, 0, 0, 0, 1, -2, 0, 0, 0, 0, 0, -449, 430, 0, 0},
+ { 0, 1,-1, 1, 0, 0, -2, 2, 0, 0, 0, 0, 0, -8, -47, -25, 4},
+ { 0, 0, 0, 0, 0, 0, -1, 2, 0, 0, 0, 0, 1, 6, 47, 25, -3},
+ {-1, 0, 1, 1, 0, 3, -4, 0, 0, 0, 0, 0, 0, 0, 23, 13, 0},
+ {-1, 0, 1, 1, 0, 0, 3, -4, 0, 0, 0, 0, 0, -3, 0, 0, 2},
+ { 0, 1,-1, 1, 0, 0, -1, 0, 0,-2, 0, 0, 0, 3, -4, -2, -2},
+ { 0, 1,-1, 1, 0, 0, -1, 0, 0, 2, 0, 0, 0, -48,-110, -59, 26},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 1, 51, 114, 61, -27},
+
+ /* 161-170 */
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 2, -133, 0, 0, 57},
+ { 0, 1,-1, 0, 0, 3, -6, 0, 0, 0, 0, 0, 0, 0, 4, 0, 0},
+ { 0, 0, 0, 1, 0, -3, 5, 0, 0, 0, 0, 0, 0, -21, -6, -3, 11},
+ { 0, 1,-1, 2, 0, -3, 4, 0, 0, 0, 0, 0, 0, 0, -3, -1, 0},
+ { 0, 0, 0, 1, 0, 0, -2, 4, 0, 0, 0, 0, 0, -11, -21, -11, 6},
+ { 0, 2,-2, 1, 0, -5, 6, 0, 0, 0, 0, 0, 0, -18,-436, -233, 9},
+ { 0,-1, 1, 0, 0, 5, -7, 0, 0, 0, 0, 0, 0, 35, -7, 0, 0},
+ { 0, 0, 0, 1, 0, 5, -8, 0, 0, 0, 0, 0, 0, 0, 5, 3, 0},
+ {-2, 0, 2, 1, 0, 6, -8, 0, 0, 0, 0, 0, 0, 11, -3, -1, -6},
+ { 0, 0, 0, 1, 0, 0, -8, 15, 0, 0, 0, 0, 0, -5, -3, -1, 3},
+
+ /* 171-180 */
+ {-2, 0, 2, 1, 0, 0, 2, 0,-3, 0, 0, 0, 0, -53, -9, -5, 28},
+ {-2, 0, 2, 1, 0, 0, 6, -8, 0, 0, 0, 0, 0, 0, 3, 2, 1},
+ { 1, 0,-1, 1, 0, 0, -1, 0, 1, 0, 0, 0, 0, 4, 0, 0, -2},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 3,-5, 0, 0, 0, 0, -4, 0, 0},
+ { 0, 1,-1, 1, 0, 0, -1, 0,-1, 0, 0, 0, 0, -50, 194, 103, 27},
+ { 0, 0, 0, 0, 0, 0, 0, 0,-1, 0, 0, 0, 1, -13, 52, 28, 7},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 0, -91, 248, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 1, 6, 49, 26, -3},
+ { 0, 1,-1, 1, 0, 0, -1, 0, 1, 0, 0, 0, 0, -6, -47, -25, 3},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 1, 0, 5, 3, 0},
+
+ /* 181-190 */
+ { 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 2, 52, 23, 10, -23},
+ { 0, 1,-1, 2, 0, 0, -1, 0, 0,-1, 0, 0, 0, -3, 0, 0, 1},
+ { 0, 0, 0, 1, 0, 0, 0, 0, 0,-1, 0, 0, 0, 0, 5, 3, 0},
+ { 0,-1, 1, 0, 0, 0, 1, 0, 0,-1, 0, 0, 0, -4, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -7, 13, 0, 0, 0, 0, 2, -4, 8, 3, 2},
+ { 0, 0, 0, 0, 0, 0, 7,-13, 0, 0, 0, 0, 0, 10, 0, 0, 0},
+ { 2, 0,-2, 1, 0, 0, -5, 6, 0, 0, 0, 0, 0, 3, 0, 0, -2},
+ { 0, 2,-2, 1, 0, 0, -8, 11, 0, 0, 0, 0, 0, 0, 8, 4, 0},
+ { 0, 2,-2, 1,-1, 0, 2, 0, 0, 0, 0, 0, 0, 0, 8, 4, 1},
+ {-2, 0, 2, 0, 0, 0, 4, -4, 0, 0, 0, 0, 0, -4, 0, 0, 0},
+
+ /* 191-200 */
+ { 0, 0, 0, 0, 0, 0, 0, 0, 2,-2, 0, 0, 0, -4, 0, 0, 0},
+ { 0, 1,-1, 1, 0, 0, -1, 0, 0, 3, 0, 0, 0, -8, 4, 2, 4},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, 1, 8, -4, -2, -4},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, 2, 0, 15, 7, 0},
+ {-2, 0, 2, 0, 0, 3, -3, 0, 0, 0, 0, 0, 0, -138, 0, 0, 0},
+ { 0, 0, 0, 2, 0, 0, -4, 8,-3, 0, 0, 0, 0, 0, -7, -3, 0},
+ { 0, 0, 0, 2, 0, 0, 4, -8, 3, 0, 0, 0, 0, 0, -7, -3, 0},
+ { 2, 0,-2, 1, 0, 0, -2, 0, 2, 0, 0, 0, 0, 54, 0, 0, -29},
+ { 0, 1,-1, 2, 0, 0, -1, 0, 2, 0, 0, 0, 0, 0, 10, 4, 0},
+ { 0, 1,-1, 2, 0, 0, 0, -2, 0, 0, 0, 0, 0, -7, 0, 0, 3},
+
+ /* 201-210 */
+ { 0, 0, 0, 1, 0, 0, 1, -2, 0, 0, 0, 0, 0, -37, 35, 19, 20},
+ { 0,-1, 1, 0, 0, 0, 2, -2, 0, 0, 0, 0, 0, 0, 4, 0, 0},
+ { 0,-1, 1, 0, 0, 0, 1, 0, 0,-2, 0, 0, 0, -4, 9, 0, 0},
+ { 0, 2,-2, 1, 0, 0, -2, 0, 0, 2, 0, 0, 0, 8, 0, 0, -4},
+ { 0, 1,-1, 1, 0, 3, -6, 0, 0, 0, 0, 0, 0, -9, -14, -8, 5},
+ { 0, 0, 0, 0, 0, 3, -5, 0, 0, 0, 0, 0, 1, -3, -9, -5, 3},
+ { 0, 0, 0, 0, 0, 3, -5, 0, 0, 0, 0, 0, 0, -145, 47, 0, 0},
+ { 0, 1,-1, 1, 0, -3, 4, 0, 0, 0, 0, 0, 0, -10, 40, 21, 5},
+ { 0, 0, 0, 0, 0, -3, 5, 0, 0, 0, 0, 0, 1, 11, -49, -26, -7},
+ { 0, 0, 0, 0, 0, -3, 5, 0, 0, 0, 0, 0, 2,-2150, 0, 0, 932},
+
+ /* 211-220 */
+ { 0, 2,-2, 2, 0, -3, 3, 0, 0, 0, 0, 0, 0, -12, 0, 0, 5},
+ { 0, 0, 0, 0, 0, -3, 5, 0, 0, 0, 0, 0, 2, 85, 0, 0, -37},
+ { 0, 0, 0, 0, 0, 0, 2, -4, 0, 0, 0, 0, 1, 4, 0, 0, -2},
+ { 0, 1,-1, 1, 0, 0, 1, -4, 0, 0, 0, 0, 0, 3, 0, 0, -2},
+ { 0, 0, 0, 0, 0, 0, 2, -4, 0, 0, 0, 0, 0, -86, 153, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -2, 4, 0, 0, 0, 0, 1, -6, 9, 5, 3},
+ { 0, 1,-1, 1, 0, 0, -3, 4, 0, 0, 0, 0, 0, 9, -13, -7, -5},
+ { 0, 0, 0, 0, 0, 0, -2, 4, 0, 0, 0, 0, 1, -8, 12, 6, 4},
+ { 0, 0, 0, 0, 0, 0, -2, 4, 0, 0, 0, 0, 2, -51, 0, 0, 22},
+ { 0, 0, 0, 0, 0, -5, 8, 0, 0, 0, 0, 0, 2, -11,-268, -116, 5},
+
+ /* 221-230 */
+ { 0, 2,-2, 2, 0, -5, 6, 0, 0, 0, 0, 0, 0, 0, 12, 5, 0},
+ { 0, 0, 0, 0, 0, -5, 8, 0, 0, 0, 0, 0, 2, 0, 7, 3, 0},
+ { 0, 0, 0, 0, 0, -5, 8, 0, 0, 0, 0, 0, 1, 31, 6, 3, -17},
+ { 0, 1,-1, 1, 0, -5, 7, 0, 0, 0, 0, 0, 0, 140, 27, 14, -75},
+ { 0, 0, 0, 0, 0, -5, 8, 0, 0, 0, 0, 0, 1, 57, 11, 6, -30},
+ { 0, 0, 0, 0, 0, 5, -8, 0, 0, 0, 0, 0, 0, -14, -39, 0, 0},
+ { 0, 1,-1, 2, 0, 0, -1, 0,-1, 0, 0, 0, 0, 0, -6, -2, 0},
+ { 0, 0, 0, 1, 0, 0, 0, 0,-1, 0, 0, 0, 0, 4, 15, 8, -2},
+ { 0,-1, 1, 0, 0, 0, 1, 0,-1, 0, 0, 0, 0, 0, 4, 0, 0},
+ { 0, 2,-2, 1, 0, 0, -2, 0, 1, 0, 0, 0, 0, -3, 0, 0, 1},
+
+ /* 231-240 */
+ { 0, 0, 0, 0, 0, 0, -6, 11, 0, 0, 0, 0, 2, 0, 11, 5, 0},
+ { 0, 0, 0, 0, 0, 0, 6,-11, 0, 0, 0, 0, 0, 9, 6, 0, 0},
+ { 0, 0, 0, 0,-1, 0, 4, 0, 0, 0, 0, 0, 2, -4, 10, 4, 2},
+ { 0, 0, 0, 0, 1, 0, -4, 0, 0, 0, 0, 0, 0, 5, 3, 0, 0},
+ { 2, 0,-2, 1, 0, -3, 3, 0, 0, 0, 0, 0, 0, 16, 0, 0, -9},
+ {-2, 0, 2, 0, 0, 0, 2, 0, 0,-2, 0, 0, 0, -3, 0, 0, 0},
+ { 0, 2,-2, 1, 0, 0, -7, 9, 0, 0, 0, 0, 0, 0, 3, 2, -1},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 4,-5, 0, 0, 2, 7, 0, 0, -3},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, -25, 22, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 1, 42, 223, 119, -22},
+
+ /* 241-250 */
+ { 0, 1,-1, 1, 0, 0, -1, 0, 2, 0, 0, 0, 0, -27,-143, -77, 14},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 1, 9, 49, 26, -5},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 2,-1166, 0, 0, 505},
+ { 0, 2,-2, 2, 0, 0, -2, 0, 2, 0, 0, 0, 0, -5, 0, 0, 2},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 5, 0, 0, 2, -6, 0, 0, 3},
+ { 0, 0, 0, 1, 0, 3, -5, 0, 0, 0, 0, 0, 0, -8, 0, 1, 4},
+ { 0,-1, 1, 0, 0, 3, -4, 0, 0, 0, 0, 0, 0, 0, -4, 0, 0},
+ { 0, 2,-2, 1, 0, -3, 3, 0, 0, 0, 0, 0, 0, 117, 0, 0, -63},
+ { 0, 0, 0, 1, 0, 0, 2, -4, 0, 0, 0, 0, 0, -4, 8, 4, 2},
+ { 0, 2,-2, 1, 0, 0, -4, 4, 0, 0, 0, 0, 0, 3, 0, 0, -2},
+
+ /* 251-260 */
+ { 0, 1,-1, 2, 0, -5, 7, 0, 0, 0, 0, 0, 0, -5, 0, 0, 2},
+ { 0, 0, 0, 0, 0, 0, 3, -6, 0, 0, 0, 0, 0, 0, 31, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -3, 6, 0, 0, 0, 0, 1, -5, 0, 1, 3},
+ { 0, 1,-1, 1, 0, 0, -4, 6, 0, 0, 0, 0, 0, 4, 0, 0, -2},
+ { 0, 0, 0, 0, 0, 0, -3, 6, 0, 0, 0, 0, 1, -4, 0, 0, 2},
+ { 0, 0, 0, 0, 0, 0, -3, 6, 0, 0, 0, 0, 2, -24, -13, -6, 10},
+ { 0,-1, 1, 0, 0, 2, -2, 0, 0, 0, 0, 0, 0, 3, 0, 0, 0},
+ { 0, 0, 0, 1, 0, 2, -3, 0, 0, 0, 0, 0, 0, 0, -32, -17, 0},
+ { 0, 0, 0, 0, 0, 0, -5, 9, 0, 0, 0, 0, 2, 8, 12, 5, -3},
+ { 0, 0, 0, 0, 0, 0, -5, 9, 0, 0, 0, 0, 1, 3, 0, 0, -1},
+
+ /* 261-270 */
+ { 0, 0, 0, 0, 0, 0, 5, -9, 0, 0, 0, 0, 0, 7, 13, 0, 0},
+ { 0,-1, 1, 0, 0, 0, 1, 0,-2, 0, 0, 0, 0, -3, 16, 0, 0},
+ { 0, 2,-2, 1, 0, 0, -2, 0, 2, 0, 0, 0, 0, 50, 0, 0, -27},
+ {-2, 1, 1, 1, 0, 0, 1, 0, 0, 0, 0, 0, 0, 0, -5, -3, 0},
+ { 0,-2, 2, 0, 0, 3, -3, 0, 0, 0, 0, 0, 0, 13, 0, 0, 0},
+ { 0, 0, 0, 0, 0, -6, 10, 0, 0, 0, 0, 0, 1, 0, 5, 3, 1},
+ { 0, 0, 0, 0, 0, -6, 10, 0, 0, 0, 0, 0, 2, 24, 5, 2, -11},
+ { 0, 0, 0, 0, 0, -2, 3, 0, 0, 0, 0, 0, 2, 5, -11, -5, -2},
+ { 0, 0, 0, 0, 0, -2, 3, 0, 0, 0, 0, 0, 1, 30, -3, -2, -16},
+ { 0, 1,-1, 1, 0, -2, 2, 0, 0, 0, 0, 0, 0, 18, 0, 0, -9},
+
+ /* 271-280 */
+ { 0, 0, 0, 0, 0, 2, -3, 0, 0, 0, 0, 0, 0, 8, 614, 0, 0},
+ { 0, 0, 0, 0, 0, 2, -3, 0, 0, 0, 0, 0, 1, 3, -3, -1, -2},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, 0, 1, 6, 17, 9, -3},
+ { 0, 1,-1, 1, 0, 0, -1, 0, 3, 0, 0, 0, 0, -3, -9, -5, 2},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, 0, 1, 0, 6, 3, -1},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, 0, 2, -127, 21, 9, 55},
+ { 0, 0, 0, 0, 0, 0, 4, -8, 0, 0, 0, 0, 0, 3, 5, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -4, 8, 0, 0, 0, 0, 2, -6, -10, -4, 3},
+ { 0,-2, 2, 0, 0, 0, 2, 0,-2, 0, 0, 0, 0, 5, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -4, 7, 0, 0, 0, 0, 2, 16, 9, 4, -7},
+
+ /* 281-290 */
+ { 0, 0, 0, 0, 0, 0, -4, 7, 0, 0, 0, 0, 1, 3, 0, 0, -2},
+ { 0, 0, 0, 0, 0, 0, 4, -7, 0, 0, 0, 0, 0, 0, 22, 0, 0},
+ { 0, 0, 0, 1, 0, -2, 3, 0, 0, 0, 0, 0, 0, 0, 19, 10, 0},
+ { 0, 2,-2, 1, 0, 0, -2, 0, 3, 0, 0, 0, 0, 7, 0, 0, -4},
+ { 0, 0, 0, 0, 0, 0, -5, 10, 0, 0, 0, 0, 2, 0, -5, -2, 0},
+ { 0, 0, 0, 1, 0, -1, 2, 0, 0, 0, 0, 0, 0, 0, 3, 1, 0},
+ { 0, 0, 0, 0, 0, 0, 0, 0, 4, 0, 0, 0, 2, -9, 3, 1, 4},
+ { 0, 0, 0, 0, 0, 0, -3, 5, 0, 0, 0, 0, 2, 17, 0, 0, -7},
+ { 0, 0, 0, 0, 0, 0, -3, 5, 0, 0, 0, 0, 1, 0, -3, -2, -1},
+ { 0, 0, 0, 0, 0, 0, 3, -5, 0, 0, 0, 0, 0, -20, 34, 0, 0},
+
+ /* 291-300 */
+ { 0, 0, 0, 0, 0, 1, -2, 0, 0, 0, 0, 0, 1, -10, 0, 1, 5},
+ { 0, 1,-1, 1, 0, 1, -3, 0, 0, 0, 0, 0, 0, -4, 0, 0, 2},
+ { 0, 0, 0, 0, 0, 1, -2, 0, 0, 0, 0, 0, 0, 22, -87, 0, 0},
+ { 0, 0, 0, 0, 0, -1, 2, 0, 0, 0, 0, 0, 1, -4, 0, 0, 2},
+ { 0, 0, 0, 0, 0, -1, 2, 0, 0, 0, 0, 0, 2, -3, -6, -2, 1},
+ { 0, 0, 0, 0, 0, -7, 11, 0, 0, 0, 0, 0, 2, -16, -3, -1, 7},
+ { 0, 0, 0, 0, 0, -7, 11, 0, 0, 0, 0, 0, 1, 0, -3, -2, 0},
+ { 0,-2, 2, 0, 0, 4, -4, 0, 0, 0, 0, 0, 0, 4, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 2, -3, 0, 0, 0, 0, 0, -68, 39, 0, 0},
+ { 0, 2,-2, 1, 0, -4, 4, 0, 0, 0, 0, 0, 0, 27, 0, 0, -14},
+
+ /* 301-310 */
+ { 0,-1, 1, 0, 0, 4, -5, 0, 0, 0, 0, 0, 0, 0, -4, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 1, -1, 0, 0, 0, 0, 0, -25, 0, 0, 0},
+ { 0, 0, 0, 0, 0, -4, 7, 0, 0, 0, 0, 0, 1, -12, -3, -2, 6},
+ { 0, 1,-1, 1, 0, -4, 6, 0, 0, 0, 0, 0, 0, 3, 0, 0, -1},
+ { 0, 0, 0, 0, 0, -4, 7, 0, 0, 0, 0, 0, 2, 3, 66, 29, -1},
+ { 0, 0, 0, 0, 0, -4, 6, 0, 0, 0, 0, 0, 2, 490, 0, 0,-213},
+ { 0, 0, 0, 0, 0, -4, 6, 0, 0, 0, 0, 0, 1, -22, 93, 49, 12},
+ { 0, 1,-1, 1, 0, -4, 5, 0, 0, 0, 0, 0, 0, -7, 28, 15, 4},
+ { 0, 0, 0, 0, 0, -4, 6, 0, 0, 0, 0, 0, 1, -3, 13, 7, 2},
+ { 0, 0, 0, 0, 0, 4, -6, 0, 0, 0, 0, 0, 0, -46, 14, 0, 0},
+
+ /* 311-320 */
+ {-2, 0, 2, 0, 0, 2, -2, 0, 0, 0, 0, 0, 0, -5, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 0, 0, 2, 1, 0, 0},
+ { 0,-1, 1, 0, 0, 1, 0, 0, 0, 0, 0, 0, 0, 0, -3, 0, 0},
+ { 0, 0, 0, 1, 0, 1, -1, 0, 0, 0, 0, 0, 0, -28, 0, 0, 15},
+ { 0, 0, 0, 0, 0, 0, -1, 0, 5, 0, 0, 0, 2, 5, 0, 0, -2},
+ { 0, 0, 0, 0, 0, 0, 1, -3, 0, 0, 0, 0, 0, 0, 3, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -1, 3, 0, 0, 0, 0, 2, -11, 0, 0, 5},
+ { 0, 0, 0, 0, 0, 0, -7, 12, 0, 0, 0, 0, 2, 0, 3, 1, 0},
+ { 0, 0, 0, 0, 0, -1, 1, 0, 0, 0, 0, 0, 2, -3, 0, 0, 1},
+ { 0, 0, 0, 0, 0, -1, 1, 0, 0, 0, 0, 0, 1, 25, 106, 57, -13},
+
+ /* 321-330 */
+ { 0, 1,-1, 1, 0, -1, 0, 0, 0, 0, 0, 0, 0, 5, 21, 11, -3},
+ { 0, 0, 0, 0, 0, 1, -1, 0, 0, 0, 0, 0, 0, 1485, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 1, -1, 0, 0, 0, 0, 0, 1, -7, -32, -17, 4},
+ { 0, 1,-1, 1, 0, 1, -2, 0, 0, 0, 0, 0, 0, 0, 5, 3, 0},
+ { 0, 0, 0, 0, 0, 0, -2, 5, 0, 0, 0, 0, 2, -6, -3, -2, 3},
+ { 0, 0, 0, 0, 0, 0, -1, 0, 4, 0, 0, 0, 2, 30, -6, -2, -13},
+ { 0, 0, 0, 0, 0, 0, 1, 0,-4, 0, 0, 0, 0, -4, 4, 0, 0},
+ { 0, 0, 0, 1, 0, -1, 1, 0, 0, 0, 0, 0, 0, -19, 0, 0, 10},
+ { 0, 0, 0, 0, 0, 0, -6, 10, 0, 0, 0, 0, 2, 0, 4, 2, -1},
+ { 0, 0, 0, 0, 0, 0, -6, 10, 0, 0, 0, 0, 0, 0, 3, 0, 0},
+
+ /* 331-340 */
+ { 0, 2,-2, 1, 0, 0, -3, 0, 3, 0, 0, 0, 0, 4, 0, 0, -2},
+ { 0, 0, 0, 0, 0, 0, -3, 7, 0, 0, 0, 0, 2, 0, -3, -1, 0},
+ {-2, 0, 2, 0, 0, 4, -4, 0, 0, 0, 0, 0, 0, -3, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -5, 8, 0, 0, 0, 0, 2, 5, 3, 1, -2},
+ { 0, 0, 0, 0, 0, 0, 5, -8, 0, 0, 0, 0, 0, 0, 11, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -1, 0, 3, 0, 0, 0, 2, 118, 0, 0, -52},
+ { 0, 0, 0, 0, 0, 0, -1, 0, 3, 0, 0, 0, 1, 0, -5, -3, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 0,-3, 0, 0, 0, 0, -28, 36, 0, 0},
+ { 0, 0, 0, 0, 0, 2, -4, 0, 0, 0, 0, 0, 0, 5, -5, 0, 0},
+ { 0, 0, 0, 0, 0, -2, 4, 0, 0, 0, 0, 0, 1, 14, -59, -31, -8},
+
+ /* 341-350 */
+ { 0, 1,-1, 1, 0, -2, 3, 0, 0, 0, 0, 0, 0, 0, 9, 5, 1},
+ { 0, 0, 0, 0, 0, -2, 4, 0, 0, 0, 0, 0, 2, -458, 0, 0, 198},
+ { 0, 0, 0, 0, 0, -6, 9, 0, 0, 0, 0, 0, 2, 0, -45, -20, 0},
+ { 0, 0, 0, 0, 0, -6, 9, 0, 0, 0, 0, 0, 1, 9, 0, 0, -5},
+ { 0, 0, 0, 0, 0, 6, -9, 0, 0, 0, 0, 0, 0, 0, -3, 0, 0},
+ { 0, 0, 0, 1, 0, 0, 1, 0,-2, 0, 0, 0, 0, 0, -4, -2, -1},
+ { 0, 2,-2, 1, 0, -2, 2, 0, 0, 0, 0, 0, 0, 11, 0, 0, -6},
+ { 0, 0, 0, 0, 0, 0, -4, 6, 0, 0, 0, 0, 2, 6, 0, 0, -2},
+ { 0, 0, 0, 0, 0, 0, 4, -6, 0, 0, 0, 0, 0, -16, 23, 0, 0},
+ { 0, 0, 0, 1, 0, 3, -4, 0, 0, 0, 0, 0, 0, 0, -4, -2, 0},
+
+ /* 351-360 */
+ { 0, 0, 0, 0, 0, 0, -1, 0, 2, 0, 0, 0, 2, -5, 0, 0, 2},
+ { 0, 0, 0, 0, 0, 0, 1, 0,-2, 0, 0, 0, 0, -166, 269, 0, 0},
+ { 0, 0, 0, 1, 0, 0, 1, 0,-1, 0, 0, 0, 0, 15, 0, 0, -8},
+ { 0, 0, 0, 0, 0, -5, 9, 0, 0, 0, 0, 0, 2, 10, 0, 0, -4},
+ { 0, 0, 0, 0, 0, 0, 3, -4, 0, 0, 0, 0, 0, -78, 45, 0, 0},
+ { 0, 0, 0, 0, 0, -3, 4, 0, 0, 0, 0, 0, 2, 0, -5, -2, 0},
+ { 0, 0, 0, 0, 0, -3, 4, 0, 0, 0, 0, 0, 1, 7, 0, 0, -4},
+ { 0, 0, 0, 0, 0, 3, -4, 0, 0, 0, 0, 0, 0, -5, 328, 0, 0},
+ { 0, 0, 0, 0, 0, 3, -4, 0, 0, 0, 0, 0, 1, 3, 0, 0, -2},
+ { 0, 0, 0, 1, 0, 0, 2, -2, 0, 0, 0, 0, 0, 5, 0, 0, -2},
+
+ /* 361-370 */
+ { 0, 0, 0, 1, 0, 0, -1, 0, 2, 0, 0, 0, 0, 0, 3, 1, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 0, 0,-3, 0, 0, 0, -3, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 0, 1,-5, 0, 0, 0, -3, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -1, 0, 1, 0, 0, 0, 1, 0, -4, -2, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 0,-1, 0, 0, 0, 0,-1223, -26, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 0,-1, 0, 0, 0, 1, 0, 7, 3, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 0,-3, 5, 0, 0, 0, 3, 0, 0, 0},
+ { 0, 0, 0, 1, 0, -3, 4, 0, 0, 0, 0, 0, 0, 0, 3, 2, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 0, 0,-2, 0, 0, 0, -6, 20, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 2, -2, 0, 0, 0, 0, 0, -368, 0, 0, 0},
+
+ /* 371-380 */
+ { 0, 0, 0, 0, 0, 0, 1, 0, 0,-1, 0, 0, 0, -75, 0, 0, 0},
+ { 0, 0, 0, 1, 0, 0, -1, 0, 1, 0, 0, 0, 0, 11, 0, 0, -6},
+ { 0, 0, 0, 1, 0, 0, -2, 2, 0, 0, 0, 0, 0, 3, 0, 0, -2},
+ { 0, 0, 0, 0, 0, -8, 14, 0, 0, 0, 0, 0, 2, -3, 0, 0, 1},
+ { 0, 0, 0, 0, 0, 0, 1, 0, 2,-5, 0, 0, 0, -13, -30, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 5, -8, 3, 0, 0, 0, 0, 21, 3, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 5, -8, 3, 0, 0, 0, 2, -3, 0, 0, 1},
+ { 0, 0, 0, 0, 0, 0, -1, 0, 0, 0, 0, 0, 1, -4, 0, 0, 2},
+ { 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 0, 0, 0, 8, -27, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 3, -8, 3, 0, 0, 0, 0, -19, -11, 0, 0},
+
+ /* 381-390 */
+ { 0, 0, 0, 0, 0, 0, -3, 8,-3, 0, 0, 0, 2, -4, 0, 0, 2},
+ { 0, 0, 0, 0, 0, 0, 1, 0,-2, 5, 0, 0, 2, 0, 5, 2, 0},
+ { 0, 0, 0, 0, 0, -8, 12, 0, 0, 0, 0, 0, 2, -6, 0, 0, 2},
+ { 0, 0, 0, 0, 0, -8, 12, 0, 0, 0, 0, 0, 0, -8, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 0, 1,-2, 0, 0, 0, -1, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 0, 0, 1, 0, 0, 2, -14, 0, 0, 6},
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 6, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 2, -74, 0, 0, 32},
+ { 0, 0, 0, 0, 0, 0, 1, 0, 0, 2, 0, 0, 2, 0, -3, -1, 0},
+ { 0, 2,-2, 1, 0, -5, 5, 0, 0, 0, 0, 0, 0, 4, 0, 0, -2},
+
+ /* 391-400 */
+ { 0, 0, 0, 0, 0, 0, 1, 0, 1, 0, 0, 0, 0, 8, 11, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 0, 1, 0, 0, 0, 1, 0, 3, 2, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 0, 1, 0, 0, 0, 2, -262, 0, 0, 114},
+ { 0, 0, 0, 0, 0, 3, -6, 0, 0, 0, 0, 0, 0, 0, -4, 0, 0},
+ { 0, 0, 0, 0, 0, -3, 6, 0, 0, 0, 0, 0, 1, -7, 0, 0, 4},
+ { 0, 0, 0, 0, 0, -3, 6, 0, 0, 0, 0, 0, 2, 0, -27, -12, 0},
+ { 0, 0, 0, 0, 0, 0, -1, 4, 0, 0, 0, 0, 2, -19, -8, -4, 8},
+ { 0, 0, 0, 0, 0, -5, 7, 0, 0, 0, 0, 0, 2, 202, 0, 0, -87},
+ { 0, 0, 0, 0, 0, -5, 7, 0, 0, 0, 0, 0, 1, -8, 35, 19, 5},
+ { 0, 1,-1, 1, 0, -5, 6, 0, 0, 0, 0, 0, 0, 0, 4, 2, 0},
+
+ /* 401-410 */
+ { 0, 0, 0, 0, 0, 5, -7, 0, 0, 0, 0, 0, 0, 16, -5, 0, 0},
+ { 0, 2,-2, 1, 0, 0, -1, 0, 1, 0, 0, 0, 0, 5, 0, 0, -3},
+ { 0, 0, 0, 0, 0, 0, -1, 0, 1, 0, 0, 0, 0, 0, -3, 0, 0},
+ { 0, 0, 0, 0,-1, 0, 3, 0, 0, 0, 0, 0, 2, 1, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 0, 2, 0, 0, 0, 2, -35, -48, -21, 15},
+ { 0, 0, 0, 0, 0, 0, -2, 6, 0, 0, 0, 0, 2, -3, -5, -2, 1},
+ { 0, 0, 0, 1, 0, 2, -2, 0, 0, 0, 0, 0, 0, 6, 0, 0, -3},
+ { 0, 0, 0, 0, 0, 0, -6, 9, 0, 0, 0, 0, 2, 3, 0, 0, -1},
+ { 0, 0, 0, 0, 0, 0, 6, -9, 0, 0, 0, 0, 0, 0, -5, 0, 0},
+ { 0, 0, 0, 0, 0, -2, 2, 0, 0, 0, 0, 0, 1, 12, 55, 29, -6},
+
+ /* 411-420 */
+ { 0, 1,-1, 1, 0, -2, 1, 0, 0, 0, 0, 0, 0, 0, 5, 3, 0},
+ { 0, 0, 0, 0, 0, 2, -2, 0, 0, 0, 0, 0, 0, -598, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 2, -2, 0, 0, 0, 0, 0, 1, -3, -13, -7, 1},
+ { 0, 0, 0, 0, 0, 0, 1, 0, 3, 0, 0, 0, 2, -5, -7, -3, 2},
+ { 0, 0, 0, 0, 0, 0, -5, 7, 0, 0, 0, 0, 2, 3, 0, 0, -1},
+ { 0, 0, 0, 0, 0, 0, 5, -7, 0, 0, 0, 0, 0, 5, -7, 0, 0},
+ { 0, 0, 0, 1, 0, -2, 2, 0, 0, 0, 0, 0, 0, 4, 0, 0, -2},
+ { 0, 0, 0, 0, 0, 0, 4, -5, 0, 0, 0, 0, 0, 16, -6, 0, 0},
+ { 0, 0, 0, 0, 0, 1, -3, 0, 0, 0, 0, 0, 0, 8, -3, 0, 0},
+ { 0, 0, 0, 0, 0, -1, 3, 0, 0, 0, 0, 0, 1, 8, -31, -16, -4},
+
+ /* 421-430 */
+ { 0, 1,-1, 1, 0, -1, 2, 0, 0, 0, 0, 0, 0, 0, 3, 1, 0},
+ { 0, 0, 0, 0, 0, -1, 3, 0, 0, 0, 0, 0, 2, 113, 0, 0, -49},
+ { 0, 0, 0, 0, 0, -7, 10, 0, 0, 0, 0, 0, 2, 0, -24, -10, 0},
+ { 0, 0, 0, 0, 0, -7, 10, 0, 0, 0, 0, 0, 1, 4, 0, 0, -2},
+ { 0, 0, 0, 0, 0, 0, 3, -3, 0, 0, 0, 0, 0, 27, 0, 0, 0},
+ { 0, 0, 0, 0, 0, -4, 8, 0, 0, 0, 0, 0, 2, -3, 0, 0, 1},
+ { 0, 0, 0, 0, 0, -4, 5, 0, 0, 0, 0, 0, 2, 0, -4, -2, 0},
+ { 0, 0, 0, 0, 0, -4, 5, 0, 0, 0, 0, 0, 1, 5, 0, 0, -2},
+ { 0, 0, 0, 0, 0, 4, -5, 0, 0, 0, 0, 0, 0, 0, -3, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 1, 0, 0, 0, 0, 2, -13, 0, 0, 6},
+
+ /* 431-440 */
+ { 0, 0, 0, 0, 0, 0, -2, 0, 5, 0, 0, 0, 2, 5, 0, 0, -2},
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, 0, 0, 2, -18, -10, -4, 8},
+ { 0, 0, 0, 0, 0, 1, 0, 0, 0, 0, 0, 0, 0, -4, -28, 0, 0},
+ { 0, 0, 0, 0, 0, 1, 0, 0, 0, 0, 0, 0, 2, -5, 6, 3, 2},
+ { 0, 0, 0, 0, 0, -9, 13, 0, 0, 0, 0, 0, 2, -3, 0, 0, 1},
+ { 0, 0, 0, 0, 0, 0, -1, 5, 0, 0, 0, 0, 2, -5, -9, -4, 2},
+ { 0, 0, 0, 0, 0, 0, -2, 0, 4, 0, 0, 0, 2, 17, 0, 0, -7},
+ { 0, 0, 0, 0, 0, 0, 2, 0,-4, 0, 0, 0, 0, 11, 4, 0, 0},
+ { 0, 0, 0, 0, 0, 0, -2, 7, 0, 0, 0, 0, 2, 0, -6, -2, 0},
+ { 0, 0, 0, 0, 0, 0, 2, 0,-3, 0, 0, 0, 0, 83, 15, 0, 0},
+
+ /* 441-450 */
+ { 0, 0, 0, 0, 0, -2, 5, 0, 0, 0, 0, 0, 1, -4, 0, 0, 2},
+ { 0, 0, 0, 0, 0, -2, 5, 0, 0, 0, 0, 0, 2, 0,-114, -49, 0},
+ { 0, 0, 0, 0, 0, -6, 8, 0, 0, 0, 0, 0, 2, 117, 0, 0, -51},
+ { 0, 0, 0, 0, 0, -6, 8, 0, 0, 0, 0, 0, 1, -5, 19, 10, 2},
+ { 0, 0, 0, 0, 0, 6, -8, 0, 0, 0, 0, 0, 0, -3, 0, 0, 0},
+ { 0, 0, 0, 1, 0, 0, 2, 0,-2, 0, 0, 0, 0, -3, 0, 0, 2},
+ { 0, 0, 0, 0, 0, 0, -3, 9, 0, 0, 0, 0, 2, 0, -3, -1, 0},
+ { 0, 0, 0, 0, 0, 0, 5, -6, 0, 0, 0, 0, 0, 3, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 5, -6, 0, 0, 0, 0, 2, 0, -6, -2, 0},
+ { 0, 0, 0, 0, 0, 0, 2, 0,-2, 0, 0, 0, 0, 393, 3, 0, 0},
+
+ /* 451-460 */
+ { 0, 0, 0, 0, 0, 0, 2, 0,-2, 0, 0, 0, 1, -4, 21, 11, 2},
+ { 0, 0, 0, 0, 0, 0, 2, 0,-2, 0, 0, 0, 2, -6, 0, -1, 3},
+ { 0, 0, 0, 0, 0, -5, 10, 0, 0, 0, 0, 0, 2, -3, 8, 4, 1},
+ { 0, 0, 0, 0, 0, 0, 4, -4, 0, 0, 0, 0, 0, 8, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 4, -4, 0, 0, 0, 0, 2, 18, -29, -13, -8},
+ { 0, 0, 0, 0, 0, -3, 3, 0, 0, 0, 0, 0, 1, 8, 34, 18, -4},
+ { 0, 0, 0, 0, 0, 3, -3, 0, 0, 0, 0, 0, 0, 89, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 3, -3, 0, 0, 0, 0, 0, 1, 3, 12, 6, -1},
+ { 0, 0, 0, 0, 0, 3, -3, 0, 0, 0, 0, 0, 2, 54, -15, -7, -24},
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0,-3, 0, 0, 0, 0, 3, 0, 0},
+
+ /* 461-470 */
+ { 0, 0, 0, 0, 0, 0, -5, 13, 0, 0, 0, 0, 2, 3, 0, 0, -1},
+ { 0, 0, 0, 0, 0, 0, 2, 0,-1, 0, 0, 0, 0, 0, 35, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 2, 0,-1, 0, 0, 0, 2, -154, -30, -13, 67},
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0,-2, 0, 0, 0, 15, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0,-2, 0, 0, 1, 0, 4, 2, 0},
+ { 0, 0, 0, 0, 0, 0, 3, -2, 0, 0, 0, 0, 0, 0, 9, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 3, -2, 0, 0, 0, 0, 2, 80, -71, -31, -35},
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0,-1, 0, 0, 2, 0, -20, -9, 0},
+ { 0, 0, 0, 0, 0, 0, -6, 15, 0, 0, 0, 0, 2, 11, 5, 2, -5},
+ { 0, 0, 0, 0, 0, -8, 15, 0, 0, 0, 0, 0, 2, 61, -96, -42, -27},
+
+ /* 471-480 */
+ { 0, 0, 0, 0, 0, -3, 9, -4, 0, 0, 0, 0, 2, 14, 9, 4, -6},
+ { 0, 0, 0, 0, 0, 0, 2, 0, 2,-5, 0, 0, 2, -11, -6, -3, 5},
+ { 0, 0, 0, 0, 0, 0, -2, 8,-1,-5, 0, 0, 2, 0, -3, -1, 0},
+ { 0, 0, 0, 0, 0, 0, 6, -8, 3, 0, 0, 0, 2, 123,-415, -180, -53},
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 0, 0, 0, 0, -35},
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 0, -5, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 1, 7, -32, -17, -4},
+ { 0, 1,-1, 1, 0, 0, 1, 0, 0, 0, 0, 0, 0, 0, -9, -5, 0},
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 1, 0, -4, 2, 0},
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 2, -89, 0, 0, 38},
+
+ /* 481-490 */
+ { 0, 0, 0, 0, 0, 0, -6, 16,-4,-5, 0, 0, 2, 0, -86, -19, -6},
+ { 0, 0, 0, 0, 0, 0, -2, 8,-3, 0, 0, 0, 2, 0, 0, -19, 6},
+ { 0, 0, 0, 0, 0, 0, -2, 8,-3, 0, 0, 0, 2, -123,-416, -180, 53},
+ { 0, 0, 0, 0, 0, 0, 6, -8, 1, 5, 0, 0, 2, 0, -3, -1, 0},
+ { 0, 0, 0, 0, 0, 0, 2, 0,-2, 5, 0, 0, 2, 12, -6, -3, -5},
+ { 0, 0, 0, 0, 0, 3, -5, 4, 0, 0, 0, 0, 2, -13, 9, 4, 6},
+ { 0, 0, 0, 0, 0, -8, 11, 0, 0, 0, 0, 0, 2, 0, -15, -7, 0},
+ { 0, 0, 0, 0, 0, -8, 11, 0, 0, 0, 0, 0, 1, 3, 0, 0, -1},
+ { 0, 0, 0, 0, 0, -8, 11, 0, 0, 0, 0, 0, 2, -62, -97, -42, 27},
+ { 0, 0, 0, 0, 0, 0, 11, 0, 0, 0, 0, 0, 2, -11, 5, 2, 5},
+
+ /* 491-500 */
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0, 1, 0, 0, 2, 0, -19, -8, 0},
+ { 0, 0, 0, 0, 0, 3, -3, 0, 2, 0, 0, 0, 2, -3, 0, 0, 1},
+ { 0, 2,-2, 1, 0, 0, 4, -8, 3, 0, 0, 0, 0, 0, 4, 2, 0},
+ { 0, 1,-1, 0, 0, 0, 1, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0},
+ { 0, 2,-2, 1, 0, 0, -4, 8,-3, 0, 0, 0, 0, 0, 4, 2, 0},
+ { 0, 0, 0, 0, 0, 0, 1, 2, 0, 0, 0, 0, 2, -85, -70, -31, 37},
+ { 0, 0, 0, 0, 0, 0, 2, 0, 1, 0, 0, 0, 2, 163, -12, -5, -72},
+ { 0, 0, 0, 0, 0, -3, 7, 0, 0, 0, 0, 0, 2, -63, -16, -7, 28},
+ { 0, 0, 0, 0, 0, 0, 0, 4, 0, 0, 0, 0, 2, -21, -32, -14, 9},
+ { 0, 0, 0, 0, 0, -5, 6, 0, 0, 0, 0, 0, 2, 0, -3, -1, 0},
+
+ /* 501-510 */
+ { 0, 0, 0, 0, 0, -5, 6, 0, 0, 0, 0, 0, 1, 3, 0, 0, -2},
+ { 0, 0, 0, 0, 0, 5, -6, 0, 0, 0, 0, 0, 0, 0, 8, 0, 0},
+ { 0, 0, 0, 0, 0, 5, -6, 0, 0, 0, 0, 0, 2, 3, 10, 4, -1},
+ { 0, 0, 0, 0, 0, 0, 2, 0, 2, 0, 0, 0, 2, 3, 0, 0, -1},
+ { 0, 0, 0, 0, 0, 0, -1, 6, 0, 0, 0, 0, 2, 0, -7, -3, 0},
+ { 0, 0, 0, 0, 0, 0, 7, -9, 0, 0, 0, 0, 2, 0, -4, -2, 0},
+ { 0, 0, 0, 0, 0, 2, -1, 0, 0, 0, 0, 0, 0, 6, 19, 0, 0},
+ { 0, 0, 0, 0, 0, 2, -1, 0, 0, 0, 0, 0, 2, 5,-173, -75, -2},
+ { 0, 0, 0, 0, 0, 0, 6, -7, 0, 0, 0, 0, 2, 0, -7, -3, 0},
+ { 0, 0, 0, 0, 0, 0, 5, -5, 0, 0, 0, 0, 2, 7, -12, -5, -3},
+
+ /* 511-520 */
+ { 0, 0, 0, 0, 0, -1, 4, 0, 0, 0, 0, 0, 1, -3, 0, 0, 2},
+ { 0, 0, 0, 0, 0, -1, 4, 0, 0, 0, 0, 0, 2, 3, -4, -2, -1},
+ { 0, 0, 0, 0, 0, -7, 9, 0, 0, 0, 0, 0, 2, 74, 0, 0, -32},
+ { 0, 0, 0, 0, 0, -7, 9, 0, 0, 0, 0, 0, 1, -3, 12, 6, 2},
+ { 0, 0, 0, 0, 0, 0, 4, -3, 0, 0, 0, 0, 2, 26, -14, -6, -11},
+ { 0, 0, 0, 0, 0, 0, 3, -1, 0, 0, 0, 0, 2, 19, 0, 0, -8},
+ { 0, 0, 0, 0, 0, -4, 4, 0, 0, 0, 0, 0, 1, 6, 24, 13, -3},
+ { 0, 0, 0, 0, 0, 4, -4, 0, 0, 0, 0, 0, 0, 83, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 4, -4, 0, 0, 0, 0, 0, 1, 0, -10, -5, 0},
+ { 0, 0, 0, 0, 0, 4, -4, 0, 0, 0, 0, 0, 2, 11, -3, -1, -5},
+
+ /* 521-530 */
+ { 0, 0, 0, 0, 0, 0, 2, 1, 0, 0, 0, 0, 2, 3, 0, 1, -1},
+ { 0, 0, 0, 0, 0, 0, -3, 0, 5, 0, 0, 0, 2, 3, 0, 0, -1},
+ { 0, 0, 0, 0, 0, 1, 1, 0, 0, 0, 0, 0, 0, -4, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 1, 1, 0, 0, 0, 0, 0, 1, 5, -23, -12, -3},
+ { 0, 0, 0, 0, 0, 1, 1, 0, 0, 0, 0, 0, 2, -339, 0, 0, 147},
+ { 0, 0, 0, 0, 0, -9, 12, 0, 0, 0, 0, 0, 2, 0, -10, -5, 0},
+ { 0, 0, 0, 0, 0, 0, 3, 0,-4, 0, 0, 0, 0, 5, 0, 0, 0},
+ { 0, 2,-2, 1, 0, 1, -1, 0, 0, 0, 0, 0, 0, 3, 0, 0, -1},
+ { 0, 0, 0, 0, 0, 0, 7, -8, 0, 0, 0, 0, 2, 0, -4, -2, 0},
+ { 0, 0, 0, 0, 0, 0, 3, 0,-3, 0, 0, 0, 0, 18, -3, 0, 0},
+
+ /* 531-540 */
+ { 0, 0, 0, 0, 0, 0, 3, 0,-3, 0, 0, 0, 2, 9, -11, -5, -4},
+ { 0, 0, 0, 0, 0, -2, 6, 0, 0, 0, 0, 0, 2, -8, 0, 0, 4},
+ { 0, 0, 0, 0, 0, -6, 7, 0, 0, 0, 0, 0, 1, 3, 0, 0, -1},
+ { 0, 0, 0, 0, 0, 6, -7, 0, 0, 0, 0, 0, 0, 0, 9, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 6, -6, 0, 0, 0, 0, 2, 6, -9, -4, -2},
+ { 0, 0, 0, 0, 0, 0, 3, 0,-2, 0, 0, 0, 0, -4, -12, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 3, 0,-2, 0, 0, 0, 2, 67, -91, -39, -29},
+ { 0, 0, 0, 0, 0, 0, 5, -4, 0, 0, 0, 0, 2, 30, -18, -8, -13},
+ { 0, 0, 0, 0, 0, 3, -2, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 3, -2, 0, 0, 0, 0, 0, 2, 0,-114, -50, 0},
+
+ /* 541-550 */
+ { 0, 0, 0, 0, 0, 0, 3, 0,-1, 0, 0, 0, 2, 0, 0, 0, 23},
+ { 0, 0, 0, 0, 0, 0, 3, 0,-1, 0, 0, 0, 2, 517, 16, 7,-224},
+ { 0, 0, 0, 0, 0, 0, 3, 0, 0,-2, 0, 0, 2, 0, -7, -3, 0},
+ { 0, 0, 0, 0, 0, 0, 4, -2, 0, 0, 0, 0, 2, 143, -3, -1, -62},
+ { 0, 0, 0, 0, 0, 0, 3, 0, 0,-1, 0, 0, 2, 29, 0, 0, -13},
+ { 0, 2,-2, 1, 0, 0, 1, 0,-1, 0, 0, 0, 0, -4, 0, 0, 2},
+ { 0, 0, 0, 0, 0, -8, 16, 0, 0, 0, 0, 0, 2, -6, 0, 0, 3},
+ { 0, 0, 0, 0, 0, 0, 3, 0, 2,-5, 0, 0, 2, 5, 12, 5, -2},
+ { 0, 0, 0, 0, 0, 0, 7, -8, 3, 0, 0, 0, 2, -25, 0, 0, 11},
+ { 0, 0, 0, 0, 0, 0, -5, 16,-4,-5, 0, 0, 2, -3, 0, 0, 1},
+
+ /* 551-560 */
+ { 0, 0, 0, 0, 0, 0, 3, 0, 0, 0, 0, 0, 2, 0, 4, 2, 0},
+ { 0, 0, 0, 0, 0, 0, -1, 8,-3, 0, 0, 0, 2, -22, 12, 5, 10},
+ { 0, 0, 0, 0, 0, -8, 10, 0, 0, 0, 0, 0, 2, 50, 0, 0, -22},
+ { 0, 0, 0, 0, 0, -8, 10, 0, 0, 0, 0, 0, 1, 0, 7, 4, 0},
+ { 0, 0, 0, 0, 0, -8, 10, 0, 0, 0, 0, 0, 2, 0, 3, 1, 0},
+ { 0, 0, 0, 0, 0, 0, 2, 2, 0, 0, 0, 0, 2, -4, 4, 2, 2},
+ { 0, 0, 0, 0, 0, 0, 3, 0, 1, 0, 0, 0, 2, -5, -11, -5, 2},
+ { 0, 0, 0, 0, 0, -3, 8, 0, 0, 0, 0, 0, 2, 0, 4, 2, 0},
+ { 0, 0, 0, 0, 0, -5, 5, 0, 0, 0, 0, 0, 1, 4, 17, 9, -2},
+ { 0, 0, 0, 0, 0, 5, -5, 0, 0, 0, 0, 0, 0, 59, 0, 0, 0},
+
+ /* 561-570 */
+ { 0, 0, 0, 0, 0, 5, -5, 0, 0, 0, 0, 0, 1, 0, -4, -2, 0},
+ { 0, 0, 0, 0, 0, 5, -5, 0, 0, 0, 0, 0, 2, -8, 0, 0, 4},
+ { 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 0, 0, -3, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 0, 1, 4, -15, -8, -2},
+ { 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 0, 2, 370, -8, 0,-160},
+ { 0, 0, 0, 0, 0, 0, 7, -7, 0, 0, 0, 0, 2, 0, 0, -3, 0},
+ { 0, 0, 0, 0, 0, 0, 7, -7, 0, 0, 0, 0, 2, 0, 3, 1, 0},
+ { 0, 0, 0, 0, 0, 0, 6, -5, 0, 0, 0, 0, 2, -6, 3, 1, 3},
+ { 0, 0, 0, 0, 0, 7, -8, 0, 0, 0, 0, 0, 0, 0, 6, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 5, -3, 0, 0, 0, 0, 2, -10, 0, 0, 4},
+
+ /* 571-580 */
+ { 0, 0, 0, 0, 0, 4, -3, 0, 0, 0, 0, 0, 2, 0, 9, 4, 0},
+ { 0, 0, 0, 0, 0, 1, 2, 0, 0, 0, 0, 0, 2, 4, 17, 7, -2},
+ { 0, 0, 0, 0, 0, -9, 11, 0, 0, 0, 0, 0, 2, 34, 0, 0, -15},
+ { 0, 0, 0, 0, 0, -9, 11, 0, 0, 0, 0, 0, 1, 0, 5, 3, 0},
+ { 0, 0, 0, 0, 0, 0, 4, 0,-4, 0, 0, 0, 2, -5, 0, 0, 2},
+ { 0, 0, 0, 0, 0, 0, 4, 0,-3, 0, 0, 0, 2, -37, -7, -3, 16},
+ { 0, 0, 0, 0, 0, -6, 6, 0, 0, 0, 0, 0, 1, 3, 13, 7, -2},
+ { 0, 0, 0, 0, 0, 6, -6, 0, 0, 0, 0, 0, 0, 40, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 6, -6, 0, 0, 0, 0, 0, 1, 0, -3, -2, 0},
+ { 0, 0, 0, 0, 0, 0, 4, 0,-2, 0, 0, 0, 2, -184, -3, -1, 80},
+
+ /* 581-590 */
+ { 0, 0, 0, 0, 0, 0, 6, -4, 0, 0, 0, 0, 2, -3, 0, 0, 1},
+ { 0, 0, 0, 0, 0, 3, -1, 0, 0, 0, 0, 0, 0, -3, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 3, -1, 0, 0, 0, 0, 0, 1, 0, -10, -6, -1},
+ { 0, 0, 0, 0, 0, 3, -1, 0, 0, 0, 0, 0, 2, 31, -6, 0, -13},
+ { 0, 0, 0, 0, 0, 0, 4, 0,-1, 0, 0, 0, 2, -3, -32, -14, 1},
+ { 0, 0, 0, 0, 0, 0, 4, 0, 0,-2, 0, 0, 2, -7, 0, 0, 3},
+ { 0, 0, 0, 0, 0, 0, 5, -2, 0, 0, 0, 0, 2, 0, -8, -4, 0},
+ { 0, 0, 0, 0, 0, 0, 4, 0, 0, 0, 0, 0, 0, 3, -4, 0, 0},
+ { 0, 0, 0, 0, 0, 8, -9, 0, 0, 0, 0, 0, 0, 0, 4, 0, 0},
+ { 0, 0, 0, 0, 0, 5, -4, 0, 0, 0, 0, 0, 2, 0, 3, 1, 0},
+
+ /* 591-600 */
+ { 0, 0, 0, 0, 0, 2, 1, 0, 0, 0, 0, 0, 2, 19, -23, -10, 2},
+ { 0, 0, 0, 0, 0, 2, 1, 0, 0, 0, 0, 0, 1, 0, 0, 0, -10},
+ { 0, 0, 0, 0, 0, 2, 1, 0, 0, 0, 0, 0, 1, 0, 3, 2, 0},
+ { 0, 0, 0, 0, 0, -7, 7, 0, 0, 0, 0, 0, 1, 0, 9, 5, -1},
+ { 0, 0, 0, 0, 0, 7, -7, 0, 0, 0, 0, 0, 0, 28, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 4, -2, 0, 0, 0, 0, 0, 1, 0, -7, -4, 0},
+ { 0, 0, 0, 0, 0, 4, -2, 0, 0, 0, 0, 0, 2, 8, -4, 0, -4},
+ { 0, 0, 0, 0, 0, 4, -2, 0, 0, 0, 0, 0, 0, 0, 0, -2, 0},
+ { 0, 0, 0, 0, 0, 4, -2, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 5, 0,-4, 0, 0, 0, 2, -3, 0, 0, 1},
+
+ /* 601-610 */
+ { 0, 0, 0, 0, 0, 0, 5, 0,-3, 0, 0, 0, 2, -9, 0, 1, 4},
+ { 0, 0, 0, 0, 0, 0, 5, 0,-2, 0, 0, 0, 2, 3, 12, 5, -1},
+ { 0, 0, 0, 0, 0, 3, 0, 0, 0, 0, 0, 0, 2, 17, -3, -1, 0},
+ { 0, 0, 0, 0, 0, -8, 8, 0, 0, 0, 0, 0, 1, 0, 7, 4, 0},
+ { 0, 0, 0, 0, 0, 8, -8, 0, 0, 0, 0, 0, 0, 19, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 5, -3, 0, 0, 0, 0, 0, 1, 0, -5, -3, 0},
+ { 0, 0, 0, 0, 0, 5, -3, 0, 0, 0, 0, 0, 2, 14, -3, 0, -1},
+ { 0, 0, 0, 0, 0, -9, 9, 0, 0, 0, 0, 0, 1, 0, 0, -1, 0},
+ { 0, 0, 0, 0, 0, -9, 9, 0, 0, 0, 0, 0, 1, 0, 0, 0, -5},
+ { 0, 0, 0, 0, 0, -9, 9, 0, 0, 0, 0, 0, 1, 0, 5, 3, 0},
+
+ /* 611-620 */
+ { 0, 0, 0, 0, 0, 9, -9, 0, 0, 0, 0, 0, 0, 13, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 6, -4, 0, 0, 0, 0, 0, 1, 0, -3, -2, 0},
+ { 0, 0, 0, 0, 0, 0, 6, 0, 0, 0, 0, 0, 2, 2, 9, 4, 3},
+ { 0, 0, 0, 0, 0, 0, 6, 0, 0, 0, 0, 0, 0, 0, 0, 0, -4},
+ { 0, 0, 0, 0, 0, 0, 6, 0, 0, 0, 0, 0, 0, 8, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 6, 0, 0, 0, 0, 0, 1, 0, 4, 2, 0},
+ { 0, 0, 0, 0, 0, 0, 6, 0, 0, 0, 0, 0, 2, 6, 0, 0, -3},
+ { 0, 0, 0, 0, 0, 0, 6, 0, 0, 0, 0, 0, 0, 6, 0, 0, 0},
+ { 0, 0, 0, 0, 0, 0, 6, 0, 0, 0, 0, 0, 1, 0, 3, 1, 0},
+ { 0, 0, 0, 0, 0, 0, 6, 0, 0, 0, 0, 0, 2, 5, 0, 0, -2},
+
+ /* 621-630 */
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 3, 0, 0, -1},
+ { 1, 0,-2, 0, 0, 0, 2, 0,-2, 0, 0, 0, 0, -3, 0, 0, 0},
+ { 1, 0,-2, 0, 0, 2, -2, 0, 0, 0, 0, 0, 0, 6, 0, 0, 0},
+ { 1, 0,-2, 0, 0, 0, 1, 0,-1, 0, 0, 0, 0, 7, 0, 0, 0},
+ { 1, 0,-2, 0, 0, 1, -1, 0, 0, 0, 0, 0, 0, -4, 0, 0, 0},
+ {-1, 0, 0, 0, 0, 3, -3, 0, 0, 0, 0, 0, 0, 4, 0, 0, 0},
+ {-1, 0, 0, 0, 0, 0, 2, 0,-2, 0, 0, 0, 0, 6, 0, 0, 0},
+ {-1, 0, 2, 0, 0, 0, 4, -8, 3, 0, 0, 0, 0, 0, -4, 0, 0},
+ { 1, 0,-2, 0, 0, 0, 4, -8, 3, 0, 0, 0, 0, 0, -4, 0, 0},
+ {-2, 0, 2, 0, 0, 0, 4, -8, 3, 0, 0, 0, 0, 5, 0, 0, 0},
+
+ /* 631-640 */
+ {-1, 0, 0, 0, 0, 0, 2, 0,-3, 0, 0, 0, 0, -3, 0, 0, 0},
+ {-1, 0, 0, 0, 0, 0, 1, 0,-1, 0, 0, 0, 0, 4, 0, 0, 0},
+ {-1, 0, 0, 0, 0, 1, -1, 0, 0, 0, 0, 0, 0, -5, 0, 0, 0},
+ {-1, 0, 2, 0, 0, 2, -2, 0, 0, 0, 0, 0, 0, 4, 0, 0, 0},
+ { 1,-1, 1, 0, 0, 0, 1, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0},
+ {-1, 0, 2, 0, 0, 0, 2, 0,-3, 0, 0, 0, 0, 13, 0, 0, 0},
+ {-2, 0, 0, 0, 0, 0, 2, 0,-3, 0, 0, 0, 0, 21, 11, 0, 0},
+ { 1, 0, 0, 0, 0, 0, 4, -8, 3, 0, 0, 0, 0, 0, -5, 0, 0},
+ {-1, 1,-1, 1, 0, 0, -1, 0, 0, 0, 0, 0, 0, 0, -5, -2, 0},
+ { 1, 1,-1, 1, 0, 0, -1, 0, 0, 0, 0, 0, 0, 0, 5, 3, 0},
+
+ /* 641-650 */
+ {-1, 0, 0, 0, 0, 0, 4, -8, 3, 0, 0, 0, 0, 0, -5, 0, 0},
+ {-1, 0, 2, 1, 0, 0, 2, 0,-2, 0, 0, 0, 0, -3, 0, 0, 2},
+ { 0, 0, 0, 0, 0, 0, 2, 0,-2, 0, 0, 0, 0, 20, 10, 0, 0},
+ {-1, 0, 2, 0, 0, 0, 2, 0,-2, 0, 0, 0, 0, -34, 0, 0, 0},
+ {-1, 0, 2, 0, 0, 3, -3, 0, 0, 0, 0, 0, 0, -19, 0, 0, 0},
+ { 1, 0,-2, 1, 0, 0, -2, 0, 2, 0, 0, 0, 0, 3, 0, 0, -2},
+ { 1, 2,-2, 2, 0, -3, 3, 0, 0, 0, 0, 0, 0, -3, 0, 0, 1},
+ { 1, 2,-2, 2, 0, 0, -2, 0, 2, 0, 0, 0, 0, -6, 0, 0, 3},
+ { 1, 0, 0, 0, 0, 1, -1, 0, 0, 0, 0, 0, 0, -4, 0, 0, 0},
+ { 1, 0, 0, 0, 0, 0, 1, 0,-1, 0, 0, 0, 0, 3, 0, 0, 0},
+
+ /* 651-660 */
+ { 0, 0,-2, 0, 0, 2, -2, 0, 0, 0, 0, 0, 0, 3, 0, 0, 0},
+ { 0, 0,-2, 0, 0, 0, 1, 0,-1, 0, 0, 0, 0, 4, 0, 0, 0},
+ { 0, 2, 0, 2, 0, -2, 2, 0, 0, 0, 0, 0, 0, 3, 0, 0, -1},
+ { 0, 2, 0, 2, 0, 0, -1, 0, 1, 0, 0, 0, 0, 6, 0, 0, -3},
+ { 0, 2, 0, 2, 0, -1, 1, 0, 0, 0, 0, 0, 0, -8, 0, 0, 3},
+ { 0, 2, 0, 2, 0, -2, 3, 0, 0, 0, 0, 0, 0, 0, 3, 1, 0},
+ { 0, 0, 2, 0, 0, 0, 2, 0,-2, 0, 0, 0, 0, -3, 0, 0, 0},
+ { 0, 1, 1, 2, 0, 0, 1, 0, 0, 0, 0, 0, 0, 0, -3, -2, 0},
+ { 1, 2, 0, 2, 0, 0, 1, 0, 0, 0, 0, 0, 0, 126, -63, -27, -55},
+ {-1, 2, 0, 2, 0, 10, -3, 0, 0, 0, 0, 0, 0, -5, 0, 1, 2},
+
+ /* 661-670 */
+ { 0, 1, 1, 1, 0, 0, 1, 0, 0, 0, 0, 0, 0, -3, 28, 15, 2},
+ { 1, 2, 0, 2, 0, 0, 1, 0, 0, 0, 0, 0, 0, 5, 0, 1, -2},
+ { 0, 2, 0, 2, 0, 0, 4, -8, 3, 0, 0, 0, 0, 0, 9, 4, 1},
+ { 0, 2, 0, 2, 0, 0, -4, 8,-3, 0, 0, 0, 0, 0, 9, 4, -1},
+ {-1, 2, 0, 2, 0, 0, -4, 8,-3, 0, 0, 0, 0, -126, -63, -27, 55},
+ { 2, 2,-2, 2, 0, 0, -2, 0, 3, 0, 0, 0, 0, 3, 0, 0, -1},
+ { 1, 2, 0, 1, 0, 0, -2, 0, 3, 0, 0, 0, 0, 21, -11, -6, -11},
+ { 0, 1, 1, 0, 0, 0, 1, 0, 0, 0, 0, 0, 0, 0, -4, 0, 0},
+ {-1, 2, 0, 1, 0, 0, 1, 0, 0, 0, 0, 0, 0, -21, -11, -6, 11},
+ {-2, 2, 2, 2, 0, 0, 2, 0,-2, 0, 0, 0, 0, -3, 0, 0, 1},
+
+ /* 671-680 */
+ { 0, 2, 0, 2, 0, 2, -3, 0, 0, 0, 0, 0, 0, 0, 3, 1, 0},
+ { 0, 2, 0, 2, 0, 1, -1, 0, 0, 0, 0, 0, 0, 8, 0, 0, -4},
+ { 0, 2, 0, 2, 0, 0, 1, 0,-1, 0, 0, 0, 0, -6, 0, 0, 3},
+ { 0, 2, 0, 2, 0, 2, -2, 0, 0, 0, 0, 0, 0, -3, 0, 0, 1},
+ {-1, 2, 2, 2, 0, 0, -1, 0, 1, 0, 0, 0, 0, 3, 0, 0, -1},
+ { 1, 2, 0, 2, 0, -1, 1, 0, 0, 0, 0, 0, 0, -3, 0, 0, 1},
+ {-1, 2, 2, 2, 0, 0, 2, 0,-3, 0, 0, 0, 0, -5, 0, 0, 2},
+ { 2, 2, 0, 2, 0, 0, 2, 0,-3, 0, 0, 0, 0, 24, -12, -5, -11},
+ { 1, 2, 0, 2, 0, 0, -4, 8,-3, 0, 0, 0, 0, 0, 3, 1, 0},
+ { 1, 2, 0, 2, 0, 0, 4, -8, 3, 0, 0, 0, 0, 0, 3, 1, 0},
+
+ /* 681-687 */
+ { 1, 1, 1, 1, 0, 0, 1, 0, 0, 0, 0, 0, 0, 0, 3, 2, 0},
+ { 0, 2, 0, 2, 0, 0, 1, 0, 0, 0, 0, 0, 0, -24, -12, -5, 10},
+ { 2, 2, 0, 1, 0, 0, 1, 0, 0, 0, 0, 0, 0, 4, 0, -1, -2},
+ {-1, 2, 2, 2, 0, 0, 2, 0,-2, 0, 0, 0, 0, 13, 0, 0, -6},
+ {-1, 2, 2, 2, 0, 3, -3, 0, 0, 0, 0, 0, 0, 7, 0, 0, -3},
+ { 1, 2, 0, 2, 0, 1, -1, 0, 0, 0, 0, 0, 0, 3, 0, 0, -1},
+ { 0, 2, 2, 2, 0, 0, 2, 0,-2, 0, 0, 0, 0, 3, 0, 0, -1}
+ };
+
+/* Number of terms in the planetary nutation model */
+ const int NPL = (int) (sizeof xpl / sizeof xpl[0]);
+
+/*--------------------------------------------------------------------*/
+
+/* Interval between fundamental date J2000.0 and given date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* ------------------- */
+/* LUNI-SOLAR NUTATION */
+/* ------------------- */
+
+/* Fundamental (Delaunay) arguments */
+
+/* Mean anomaly of the Moon (IERS 2003). */
+ el = iauFal03(t);
+
+/* Mean anomaly of the Sun (MHB2000). */
+ elp = fmod(1287104.79305 +
+ t * (129596581.0481 +
+ t * (-0.5532 +
+ t * (0.000136 +
+ t * (-0.00001149)))), TURNAS) * DAS2R;
+
+/* Mean longitude of the Moon minus that of the ascending node */
+/* (IERS 2003. */
+ f = iauFaf03(t);
+
+/* Mean elongation of the Moon from the Sun (MHB2000). */
+ d = fmod(1072260.70369 +
+ t * (1602961601.2090 +
+ t * (-6.3706 +
+ t * (0.006593 +
+ t * (-0.00003169)))), TURNAS) * DAS2R;
+
+/* Mean longitude of the ascending node of the Moon (IERS 2003). */
+ om = iauFaom03(t);
+
+/* Initialize the nutation values. */
+ dp = 0.0;
+ de = 0.0;
+
+/* Summation of luni-solar nutation series (in reverse order). */
+ for (i = NLS-1; i >= 0; i--) {
+
+ /* Argument and functions. */
+ arg = fmod((double)xls[i].nl * el +
+ (double)xls[i].nlp * elp +
+ (double)xls[i].nf * f +
+ (double)xls[i].nd * d +
+ (double)xls[i].nom * om, D2PI);
+ sarg = sin(arg);
+ carg = cos(arg);
+
+ /* Term. */
+ dp += (xls[i].sp + xls[i].spt * t) * sarg + xls[i].cp * carg;
+ de += (xls[i].ce + xls[i].cet * t) * carg + xls[i].se * sarg;
+ }
+
+/* Convert from 0.1 microarcsec units to radians. */
+ dpsils = dp * U2R;
+ depsls = de * U2R;
+
+/* ------------------ */
+/* PLANETARY NUTATION */
+/* ------------------ */
+
+/* n.b. The MHB2000 code computes the luni-solar and planetary nutation */
+/* in different functions, using slightly different Delaunay */
+/* arguments in the two cases. This behaviour is faithfully */
+/* reproduced here. Use of the IERS 2003 expressions for both */
+/* cases leads to negligible changes, well below */
+/* 0.1 microarcsecond. */
+
+/* Mean anomaly of the Moon (MHB2000). */
+ al = fmod(2.35555598 + 8328.6914269554 * t, D2PI);
+
+/* Mean longitude of the Moon minus that of the ascending node */
+/*(MHB2000). */
+ af = fmod(1.627905234 + 8433.466158131 * t, D2PI);
+
+/* Mean elongation of the Moon from the Sun (MHB2000). */
+ ad = fmod(5.198466741 + 7771.3771468121 * t, D2PI);
+
+/* Mean longitude of the ascending node of the Moon (MHB2000). */
+ aom = fmod(2.18243920 - 33.757045 * t, D2PI);
+
+/* General accumulated precession in longitude (IERS 2003). */
+ apa = iauFapa03(t);
+
+/* Planetary longitudes, Mercury through Uranus (IERS 2003). */
+ alme = iauFame03(t);
+ alve = iauFave03(t);
+ alea = iauFae03(t);
+ alma = iauFama03(t);
+ alju = iauFaju03(t);
+ alsa = iauFasa03(t);
+ alur = iauFaur03(t);
+
+/* Neptune longitude (MHB2000). */
+ alne = fmod(5.321159000 + 3.8127774000 * t, D2PI);
+
+/* Initialize the nutation values. */
+ dp = 0.0;
+ de = 0.0;
+
+/* Summation of planetary nutation series (in reverse order). */
+ for (i = NPL-1; i >= 0; i--) {
+
+ /* Argument and functions. */
+ arg = fmod((double)xpl[i].nl * al +
+ (double)xpl[i].nf * af +
+ (double)xpl[i].nd * ad +
+ (double)xpl[i].nom * aom +
+ (double)xpl[i].nme * alme +
+ (double)xpl[i].nve * alve +
+ (double)xpl[i].nea * alea +
+ (double)xpl[i].nma * alma +
+ (double)xpl[i].nju * alju +
+ (double)xpl[i].nsa * alsa +
+ (double)xpl[i].nur * alur +
+ (double)xpl[i].nne * alne +
+ (double)xpl[i].npa * apa, D2PI);
+ sarg = sin(arg);
+ carg = cos(arg);
+
+ /* Term. */
+ dp += (double)xpl[i].sp * sarg + (double)xpl[i].cp * carg;
+ de += (double)xpl[i].se * sarg + (double)xpl[i].ce * carg;
+
+ }
+
+/* Convert from 0.1 microarcsec units to radians. */
+ dpsipl = dp * U2R;
+ depspl = de * U2R;
+
+/* ------- */
+/* RESULTS */
+/* ------- */
+
+/* Add luni-solar and planetary components. */
+ *dpsi = dpsils + dpsipl;
+ *deps = depsls + depspl;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/nut00b.c b/sofa/nut00b.c
new file mode 100644
index 0000000..6dd89e5
--- /dev/null
+++ b/sofa/nut00b.c
@@ -0,0 +1,422 @@
+#include "sofam.h"
+
+void iauNut00b(double date1, double date2, double *dpsi, double *deps)
+/*
+** - - - - - - - - - -
+** i a u N u t 0 0 b
+** - - - - - - - - - -
+**
+** Nutation, IAU 2000B model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** dpsi,deps double nutation, luni-solar + planetary (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The nutation components in longitude and obliquity are in radians
+** and with respect to the equinox and ecliptic of date. The
+** obliquity at J2000.0 is assumed to be the Lieske et al. (1977)
+** value of 84381.448 arcsec. (The errors that result from using
+** this function with the IAU 2006 value of 84381.406 arcsec can be
+** neglected.)
+**
+** The nutation model consists only of luni-solar terms, but
+** includes also a fixed offset which compensates for certain long-
+** period planetary terms (Note 7).
+**
+** 3) This function is an implementation of the IAU 2000B abridged
+** nutation model formally adopted by the IAU General Assembly in
+** 2000. The function computes the MHB_2000_SHORT luni-solar
+** nutation series (Luzum 2001), but without the associated
+** corrections for the precession rate adjustments and the offset
+** between the GCRS and J2000.0 mean poles.
+**
+** 4) The full IAU 2000A (MHB2000) nutation model contains nearly 1400
+** terms. The IAU 2000B model (McCarthy & Luzum 2003) contains only
+** 77 terms, plus additional simplifications, yet still delivers
+** results of 1 mas accuracy at present epochs. This combination of
+** accuracy and size makes the IAU 2000B abridged nutation model
+** suitable for most practical applications.
+**
+** The function delivers a pole accurate to 1 mas from 1900 to 2100
+** (usually better than 1 mas, very occasionally just outside
+** 1 mas). The full IAU 2000A model, which is implemented in the
+** function iauNut00a (q.v.), delivers considerably greater accuracy
+** at current dates; however, to realize this improved accuracy,
+** corrections for the essentially unpredictable free-core-nutation
+** (FCN) must also be included.
+**
+** 5) The present function provides classical nutation. The
+** MHB_2000_SHORT algorithm, from which it is adapted, deals also
+** with (i) the offsets between the GCRS and mean poles and (ii) the
+** adjustments in longitude and obliquity due to the changed
+** precession rates. These additional functions, namely frame bias
+** and precession adjustments, are supported by the SOFA functions
+** iauBi00 and iauPr00.
+**
+** 6) The MHB_2000_SHORT algorithm also provides "total" nutations,
+** comprising the arithmetic sum of the frame bias, precession
+** adjustments, and nutation (luni-solar + planetary). These total
+** nutations can be used in combination with an existing IAU 1976
+** precession implementation, such as iauPmat76, to deliver GCRS-
+** to-true predictions of mas accuracy at current epochs. However,
+** for symmetry with the iauNut00a function (q.v. for the reasons),
+** the SOFA functions do not generate the "total nutations"
+** directly. Should they be required, they could of course easily
+** be generated by calling iauBi00, iauPr00 and the present function
+** and adding the results.
+**
+** 7) The IAU 2000B model includes "planetary bias" terms that are
+** fixed in size but compensate for long-period nutations. The
+** amplitudes quoted in McCarthy & Luzum (2003), namely
+** Dpsi = -1.5835 mas and Depsilon = +1.6339 mas, are optimized for
+** the "total nutations" method described in Note 6. The Luzum
+** (2001) values used in this SOFA implementation, namely -0.135 mas
+** and +0.388 mas, are optimized for the "rigorous" method, where
+** frame bias, precession and nutation are applied separately and in
+** that order. During the interval 1995-2050, the SOFA
+** implementation delivers a maximum error of 1.001 mas (not
+** including FCN).
+**
+** References:
+**
+** Lieske, J.H., Lederle, T., Fricke, W., Morando, B., "Expressions
+** for the precession quantities based upon the IAU /1976/ system of
+** astronomical constants", Astron.Astrophys. 58, 1-2, 1-16. (1977)
+**
+** Luzum, B., private communication, 2001 (Fortran code
+** MHB_2000_SHORT)
+**
+** McCarthy, D.D. & Luzum, B.J., "An abridged model of the
+** precession-nutation of the celestial pole", Cel.Mech.Dyn.Astron.
+** 85, 37-49 (2003)
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J., Astron.Astrophys. 282, 663-683 (1994)
+**
+** This revision: 2010 September 4
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t, el, elp, f, d, om, arg, dp, de, sarg, carg,
+ dpsils, depsls, dpsipl, depspl;
+ int i;
+
+/* Units of 0.1 microarcsecond to radians */
+ static const double U2R = DAS2R / 1e7;
+
+/* ---------------------------------------- */
+/* Fixed offsets in lieu of planetary terms */
+/* ---------------------------------------- */
+
+ static const double DPPLAN = -0.135 * DMAS2R;
+ static const double DEPLAN = 0.388 * DMAS2R;
+
+/* --------------------------------------------------- */
+/* Luni-solar nutation: argument and term coefficients */
+/* --------------------------------------------------- */
+
+/* The units for the sine and cosine coefficients are */
+/* 0.1 microarcsec and the same per Julian century */
+
+ static const struct {
+ int nl,nlp,nf,nd,nom; /* coefficients of l,l',F,D,Om */
+ double ps,pst,pc; /* longitude sin, t*sin, cos coefficients */
+ double ec,ect,es; /* obliquity cos, t*cos, sin coefficients */
+
+ } x[] = {
+
+ /* 1-10 */
+ { 0, 0, 0, 0,1,
+ -172064161.0, -174666.0, 33386.0, 92052331.0, 9086.0, 15377.0},
+ { 0, 0, 2,-2,2,
+ -13170906.0, -1675.0, -13696.0, 5730336.0, -3015.0, -4587.0},
+ { 0, 0, 2, 0,2,-2276413.0,-234.0, 2796.0, 978459.0,-485.0,1374.0},
+ { 0, 0, 0, 0,2,2074554.0, 207.0, -698.0,-897492.0, 470.0,-291.0},
+ { 0, 1, 0, 0,0,1475877.0,-3633.0,11817.0, 73871.0,-184.0,-1924.0},
+ { 0, 1, 2,-2,2,-516821.0, 1226.0, -524.0, 224386.0,-677.0,-174.0},
+ { 1, 0, 0, 0,0, 711159.0, 73.0, -872.0, -6750.0, 0.0, 358.0},
+ { 0, 0, 2, 0,1,-387298.0, -367.0, 380.0, 200728.0, 18.0, 318.0},
+ { 1, 0, 2, 0,2,-301461.0, -36.0, 816.0, 129025.0, -63.0, 367.0},
+ { 0,-1, 2,-2,2, 215829.0, -494.0, 111.0, -95929.0, 299.0, 132.0},
+
+ /* 11-20 */
+ { 0, 0, 2,-2,1, 128227.0, 137.0, 181.0, -68982.0, -9.0, 39.0},
+ {-1, 0, 2, 0,2, 123457.0, 11.0, 19.0, -53311.0, 32.0, -4.0},
+ {-1, 0, 0, 2,0, 156994.0, 10.0, -168.0, -1235.0, 0.0, 82.0},
+ { 1, 0, 0, 0,1, 63110.0, 63.0, 27.0, -33228.0, 0.0, -9.0},
+ {-1, 0, 0, 0,1, -57976.0, -63.0, -189.0, 31429.0, 0.0, -75.0},
+ {-1, 0, 2, 2,2, -59641.0, -11.0, 149.0, 25543.0, -11.0, 66.0},
+ { 1, 0, 2, 0,1, -51613.0, -42.0, 129.0, 26366.0, 0.0, 78.0},
+ {-2, 0, 2, 0,1, 45893.0, 50.0, 31.0, -24236.0, -10.0, 20.0},
+ { 0, 0, 0, 2,0, 63384.0, 11.0, -150.0, -1220.0, 0.0, 29.0},
+ { 0, 0, 2, 2,2, -38571.0, -1.0, 158.0, 16452.0, -11.0, 68.0},
+
+ /* 21-30 */
+ { 0,-2, 2,-2,2, 32481.0, 0.0, 0.0, -13870.0, 0.0, 0.0},
+ {-2, 0, 0, 2,0, -47722.0, 0.0, -18.0, 477.0, 0.0, -25.0},
+ { 2, 0, 2, 0,2, -31046.0, -1.0, 131.0, 13238.0, -11.0, 59.0},
+ { 1, 0, 2,-2,2, 28593.0, 0.0, -1.0, -12338.0, 10.0, -3.0},
+ {-1, 0, 2, 0,1, 20441.0, 21.0, 10.0, -10758.0, 0.0, -3.0},
+ { 2, 0, 0, 0,0, 29243.0, 0.0, -74.0, -609.0, 0.0, 13.0},
+ { 0, 0, 2, 0,0, 25887.0, 0.0, -66.0, -550.0, 0.0, 11.0},
+ { 0, 1, 0, 0,1, -14053.0, -25.0, 79.0, 8551.0, -2.0, -45.0},
+ {-1, 0, 0, 2,1, 15164.0, 10.0, 11.0, -8001.0, 0.0, -1.0},
+ { 0, 2, 2,-2,2, -15794.0, 72.0, -16.0, 6850.0, -42.0, -5.0},
+
+ /* 31-40 */
+ { 0, 0,-2, 2,0, 21783.0, 0.0, 13.0, -167.0, 0.0, 13.0},
+ { 1, 0, 0,-2,1, -12873.0, -10.0, -37.0, 6953.0, 0.0, -14.0},
+ { 0,-1, 0, 0,1, -12654.0, 11.0, 63.0, 6415.0, 0.0, 26.0},
+ {-1, 0, 2, 2,1, -10204.0, 0.0, 25.0, 5222.0, 0.0, 15.0},
+ { 0, 2, 0, 0,0, 16707.0, -85.0, -10.0, 168.0, -1.0, 10.0},
+ { 1, 0, 2, 2,2, -7691.0, 0.0, 44.0, 3268.0, 0.0, 19.0},
+ {-2, 0, 2, 0,0, -11024.0, 0.0, -14.0, 104.0, 0.0, 2.0},
+ { 0, 1, 2, 0,2, 7566.0, -21.0, -11.0, -3250.0, 0.0, -5.0},
+ { 0, 0, 2, 2,1, -6637.0, -11.0, 25.0, 3353.0, 0.0, 14.0},
+ { 0,-1, 2, 0,2, -7141.0, 21.0, 8.0, 3070.0, 0.0, 4.0},
+
+ /* 41-50 */
+ { 0, 0, 0, 2,1, -6302.0, -11.0, 2.0, 3272.0, 0.0, 4.0},
+ { 1, 0, 2,-2,1, 5800.0, 10.0, 2.0, -3045.0, 0.0, -1.0},
+ { 2, 0, 2,-2,2, 6443.0, 0.0, -7.0, -2768.0, 0.0, -4.0},
+ {-2, 0, 0, 2,1, -5774.0, -11.0, -15.0, 3041.0, 0.0, -5.0},
+ { 2, 0, 2, 0,1, -5350.0, 0.0, 21.0, 2695.0, 0.0, 12.0},
+ { 0,-1, 2,-2,1, -4752.0, -11.0, -3.0, 2719.0, 0.0, -3.0},
+ { 0, 0, 0,-2,1, -4940.0, -11.0, -21.0, 2720.0, 0.0, -9.0},
+ {-1,-1, 0, 2,0, 7350.0, 0.0, -8.0, -51.0, 0.0, 4.0},
+ { 2, 0, 0,-2,1, 4065.0, 0.0, 6.0, -2206.0, 0.0, 1.0},
+ { 1, 0, 0, 2,0, 6579.0, 0.0, -24.0, -199.0, 0.0, 2.0},
+
+ /* 51-60 */
+ { 0, 1, 2,-2,1, 3579.0, 0.0, 5.0, -1900.0, 0.0, 1.0},
+ { 1,-1, 0, 0,0, 4725.0, 0.0, -6.0, -41.0, 0.0, 3.0},
+ {-2, 0, 2, 0,2, -3075.0, 0.0, -2.0, 1313.0, 0.0, -1.0},
+ { 3, 0, 2, 0,2, -2904.0, 0.0, 15.0, 1233.0, 0.0, 7.0},
+ { 0,-1, 0, 2,0, 4348.0, 0.0, -10.0, -81.0, 0.0, 2.0},
+ { 1,-1, 2, 0,2, -2878.0, 0.0, 8.0, 1232.0, 0.0, 4.0},
+ { 0, 0, 0, 1,0, -4230.0, 0.0, 5.0, -20.0, 0.0, -2.0},
+ {-1,-1, 2, 2,2, -2819.0, 0.0, 7.0, 1207.0, 0.0, 3.0},
+ {-1, 0, 2, 0,0, -4056.0, 0.0, 5.0, 40.0, 0.0, -2.0},
+ { 0,-1, 2, 2,2, -2647.0, 0.0, 11.0, 1129.0, 0.0, 5.0},
+
+ /* 61-70 */
+ {-2, 0, 0, 0,1, -2294.0, 0.0, -10.0, 1266.0, 0.0, -4.0},
+ { 1, 1, 2, 0,2, 2481.0, 0.0, -7.0, -1062.0, 0.0, -3.0},
+ { 2, 0, 0, 0,1, 2179.0, 0.0, -2.0, -1129.0, 0.0, -2.0},
+ {-1, 1, 0, 1,0, 3276.0, 0.0, 1.0, -9.0, 0.0, 0.0},
+ { 1, 1, 0, 0,0, -3389.0, 0.0, 5.0, 35.0, 0.0, -2.0},
+ { 1, 0, 2, 0,0, 3339.0, 0.0, -13.0, -107.0, 0.0, 1.0},
+ {-1, 0, 2,-2,1, -1987.0, 0.0, -6.0, 1073.0, 0.0, -2.0},
+ { 1, 0, 0, 0,2, -1981.0, 0.0, 0.0, 854.0, 0.0, 0.0},
+ {-1, 0, 0, 1,0, 4026.0, 0.0, -353.0, -553.0, 0.0,-139.0},
+ { 0, 0, 2, 1,2, 1660.0, 0.0, -5.0, -710.0, 0.0, -2.0},
+
+ /* 71-77 */
+ {-1, 0, 2, 4,2, -1521.0, 0.0, 9.0, 647.0, 0.0, 4.0},
+ {-1, 1, 0, 1,1, 1314.0, 0.0, 0.0, -700.0, 0.0, 0.0},
+ { 0,-2, 2,-2,1, -1283.0, 0.0, 0.0, 672.0, 0.0, 0.0},
+ { 1, 0, 2, 2,1, -1331.0, 0.0, 8.0, 663.0, 0.0, 4.0},
+ {-2, 0, 2, 2,2, 1383.0, 0.0, -2.0, -594.0, 0.0, -2.0},
+ {-1, 0, 0, 0,2, 1405.0, 0.0, 4.0, -610.0, 0.0, 2.0},
+ { 1, 1, 2,-2,2, 1290.0, 0.0, 0.0, -556.0, 0.0, 0.0}
+ };
+
+/* Number of terms in the series */
+ const int NLS = (int) (sizeof x / sizeof x[0]);
+
+/*--------------------------------------------------------------------*/
+
+/* Interval between fundamental epoch J2000.0 and given date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* --------------------*/
+/* LUNI-SOLAR NUTATION */
+/* --------------------*/
+
+/* Fundamental (Delaunay) arguments from Simon et al. (1994) */
+
+/* Mean anomaly of the Moon. */
+ el = fmod(485868.249036 + (1717915923.2178) * t, TURNAS) * DAS2R;
+
+/* Mean anomaly of the Sun. */
+ elp = fmod(1287104.79305 + (129596581.0481) * t, TURNAS) * DAS2R;
+
+/* Mean argument of the latitude of the Moon. */
+ f = fmod(335779.526232 + (1739527262.8478) * t, TURNAS) * DAS2R;
+
+/* Mean elongation of the Moon from the Sun. */
+ d = fmod(1072260.70369 + (1602961601.2090) * t, TURNAS) * DAS2R;
+
+/* Mean longitude of the ascending node of the Moon. */
+ om = fmod(450160.398036 + (-6962890.5431) * t, TURNAS) * DAS2R;
+
+/* Initialize the nutation values. */
+ dp = 0.0;
+ de = 0.0;
+
+/* Summation of luni-solar nutation series (smallest terms first). */
+ for (i = NLS-1; i >= 0; i--) {
+
+ /* Argument and functions. */
+ arg = fmod( (double)x[i].nl * el +
+ (double)x[i].nlp * elp +
+ (double)x[i].nf * f +
+ (double)x[i].nd * d +
+ (double)x[i].nom * om, D2PI );
+ sarg = sin(arg);
+ carg = cos(arg);
+
+ /* Term. */
+ dp += (x[i].ps + x[i].pst * t) * sarg + x[i].pc * carg;
+ de += (x[i].ec + x[i].ect * t) * carg + x[i].es * sarg;
+ }
+
+/* Convert from 0.1 microarcsec units to radians. */
+ dpsils = dp * U2R;
+ depsls = de * U2R;
+
+/* ------------------------------*/
+/* IN LIEU OF PLANETARY NUTATION */
+/* ------------------------------*/
+
+/* Fixed offset to correct for missing terms in truncated series. */
+ dpsipl = DPPLAN;
+ depspl = DEPLAN;
+
+/* --------*/
+/* RESULTS */
+/* --------*/
+
+/* Add luni-solar and planetary components. */
+ *dpsi = dpsils + dpsipl;
+ *deps = depsls + depspl;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/nut06a.c b/sofa/nut06a.c
new file mode 100644
index 0000000..2dfe939
--- /dev/null
+++ b/sofa/nut06a.c
@@ -0,0 +1,200 @@
+#include "sofam.h"
+
+void iauNut06a(double date1, double date2, double *dpsi, double *deps)
+/*
+** - - - - - - - - - -
+** i a u N u t 0 6 a
+** - - - - - - - - - -
+**
+** IAU 2000A nutation with adjustments to match the IAU 2006
+** precession.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** dpsi,deps double nutation, luni-solar + planetary (Note 2)
+**
+** Status: canonical model.
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The nutation components in longitude and obliquity are in radians
+** and with respect to the mean equinox and ecliptic of date,
+** IAU 2006 precession model (Hilton et al. 2006, Capitaine et al.
+** 2005).
+**
+** 3) The function first computes the IAU 2000A nutation, then applies
+** adjustments for (i) the consequences of the change in obliquity
+** from the IAU 1980 ecliptic to the IAU 2006 ecliptic and (ii) the
+** secular variation in the Earth's dynamical form factor J2.
+**
+** 4) The present function provides classical nutation, complementing
+** the IAU 2000 frame bias and IAU 2006 precession. It delivers a
+** pole which is at current epochs accurate to a few tens of
+** microarcseconds, apart from the free core nutation.
+**
+** Called:
+** iauNut00a nutation, IAU 2000A
+**
+** References:
+**
+** Chapront, J., Chapront-Touze, M. & Francou, G. 2002,
+** Astron.Astrophys. 387, 700
+**
+** Lieske, J.H., Lederle, T., Fricke, W. & Morando, B. 1977,
+** Astron.Astrophys. 58, 1-16
+**
+** Mathews, P.M., Herring, T.A., Buffet, B.A. 2002, J.Geophys.Res.
+** 107, B4. The MHB_2000 code itself was obtained on 9th September
+** 2002 from ftp//maia.usno.navy.mil/conv2000/chapter5/IAU2000A.
+**
+** Simon, J.-L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G., Laskar, J. 1994, Astron.Astrophys. 282, 663-683
+**
+** Souchay, J., Loysel, B., Kinoshita, H., Folgueira, M. 1999,
+** Astron.Astrophys.Supp.Ser. 135, 111
+**
+** Wallace, P.T., "Software for Implementing the IAU 2000
+** Resolutions", in IERS Workshop 5.1 (2002)
+**
+** This revision: 2011 April 3
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t, fj2, dp, de;
+
+
+/* Interval between fundamental date J2000.0 and given date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* Factor correcting for secular variation of J2. */
+ fj2 = -2.7774e-6 * t;
+
+/* Obtain IAU 2000A nutation. */
+ iauNut00a(date1, date2, &dp, &de);
+
+/* Apply P03 adjustments (Wallace & Capitaine, 2006, Eqs.5). */
+ *dpsi = dp + dp * (0.4697e-6 + fj2);
+ *deps = de + de * fj2;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/nut80.c b/sofa/nut80.c
new file mode 100644
index 0000000..510c71e
--- /dev/null
+++ b/sofa/nut80.c
@@ -0,0 +1,375 @@
+#include "sofam.h"
+
+void iauNut80(double date1, double date2, double *dpsi, double *deps)
+/*
+** - - - - - - - - -
+** i a u N u t 8 0
+** - - - - - - - - -
+**
+** Nutation, IAU 1980 model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** dpsi double nutation in longitude (radians)
+** deps double nutation in obliquity (radians)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The nutation components are with respect to the ecliptic of
+** date.
+**
+** Called:
+** iauAnpm normalize angle into range +/- pi
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992),
+** Section 3.222 (p111).
+**
+** This revision: 2008 September 30
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t, el, elp, f, d, om, dp, de, arg, s, c;
+ int j;
+
+/* Units of 0.1 milliarcsecond to radians */
+ const double U2R = DAS2R / 1e4;
+
+/* ------------------------------------------------ */
+/* Table of multiples of arguments and coefficients */
+/* ------------------------------------------------ */
+
+/* The units for the sine and cosine coefficients are 0.1 mas and */
+/* the same per Julian century */
+
+ static const struct {
+ int nl,nlp,nf,nd,nom; /* coefficients of l,l',F,D,Om */
+ double sp,spt; /* longitude sine, 1 and t coefficients */
+ double ce,cet; /* obliquity cosine, 1 and t coefficients */
+ } x[] = {
+
+ /* 1-10 */
+ { 0, 0, 0, 0, 1, -171996.0, -174.2, 92025.0, 8.9 },
+ { 0, 0, 0, 0, 2, 2062.0, 0.2, -895.0, 0.5 },
+ { -2, 0, 2, 0, 1, 46.0, 0.0, -24.0, 0.0 },
+ { 2, 0, -2, 0, 0, 11.0, 0.0, 0.0, 0.0 },
+ { -2, 0, 2, 0, 2, -3.0, 0.0, 1.0, 0.0 },
+ { 1, -1, 0, -1, 0, -3.0, 0.0, 0.0, 0.0 },
+ { 0, -2, 2, -2, 1, -2.0, 0.0, 1.0, 0.0 },
+ { 2, 0, -2, 0, 1, 1.0, 0.0, 0.0, 0.0 },
+ { 0, 0, 2, -2, 2, -13187.0, -1.6, 5736.0, -3.1 },
+ { 0, 1, 0, 0, 0, 1426.0, -3.4, 54.0, -0.1 },
+
+ /* 11-20 */
+ { 0, 1, 2, -2, 2, -517.0, 1.2, 224.0, -0.6 },
+ { 0, -1, 2, -2, 2, 217.0, -0.5, -95.0, 0.3 },
+ { 0, 0, 2, -2, 1, 129.0, 0.1, -70.0, 0.0 },
+ { 2, 0, 0, -2, 0, 48.0, 0.0, 1.0, 0.0 },
+ { 0, 0, 2, -2, 0, -22.0, 0.0, 0.0, 0.0 },
+ { 0, 2, 0, 0, 0, 17.0, -0.1, 0.0, 0.0 },
+ { 0, 1, 0, 0, 1, -15.0, 0.0, 9.0, 0.0 },
+ { 0, 2, 2, -2, 2, -16.0, 0.1, 7.0, 0.0 },
+ { 0, -1, 0, 0, 1, -12.0, 0.0, 6.0, 0.0 },
+ { -2, 0, 0, 2, 1, -6.0, 0.0, 3.0, 0.0 },
+
+ /* 21-30 */
+ { 0, -1, 2, -2, 1, -5.0, 0.0, 3.0, 0.0 },
+ { 2, 0, 0, -2, 1, 4.0, 0.0, -2.0, 0.0 },
+ { 0, 1, 2, -2, 1, 4.0, 0.0, -2.0, 0.0 },
+ { 1, 0, 0, -1, 0, -4.0, 0.0, 0.0, 0.0 },
+ { 2, 1, 0, -2, 0, 1.0, 0.0, 0.0, 0.0 },
+ { 0, 0, -2, 2, 1, 1.0, 0.0, 0.0, 0.0 },
+ { 0, 1, -2, 2, 0, -1.0, 0.0, 0.0, 0.0 },
+ { 0, 1, 0, 0, 2, 1.0, 0.0, 0.0, 0.0 },
+ { -1, 0, 0, 1, 1, 1.0, 0.0, 0.0, 0.0 },
+ { 0, 1, 2, -2, 0, -1.0, 0.0, 0.0, 0.0 },
+
+ /* 31-40 */
+ { 0, 0, 2, 0, 2, -2274.0, -0.2, 977.0, -0.5 },
+ { 1, 0, 0, 0, 0, 712.0, 0.1, -7.0, 0.0 },
+ { 0, 0, 2, 0, 1, -386.0, -0.4, 200.0, 0.0 },
+ { 1, 0, 2, 0, 2, -301.0, 0.0, 129.0, -0.1 },
+ { 1, 0, 0, -2, 0, -158.0, 0.0, -1.0, 0.0 },
+ { -1, 0, 2, 0, 2, 123.0, 0.0, -53.0, 0.0 },
+ { 0, 0, 0, 2, 0, 63.0, 0.0, -2.0, 0.0 },
+ { 1, 0, 0, 0, 1, 63.0, 0.1, -33.0, 0.0 },
+ { -1, 0, 0, 0, 1, -58.0, -0.1, 32.0, 0.0 },
+ { -1, 0, 2, 2, 2, -59.0, 0.0, 26.0, 0.0 },
+
+ /* 41-50 */
+ { 1, 0, 2, 0, 1, -51.0, 0.0, 27.0, 0.0 },
+ { 0, 0, 2, 2, 2, -38.0, 0.0, 16.0, 0.0 },
+ { 2, 0, 0, 0, 0, 29.0, 0.0, -1.0, 0.0 },
+ { 1, 0, 2, -2, 2, 29.0, 0.0, -12.0, 0.0 },
+ { 2, 0, 2, 0, 2, -31.0, 0.0, 13.0, 0.0 },
+ { 0, 0, 2, 0, 0, 26.0, 0.0, -1.0, 0.0 },
+ { -1, 0, 2, 0, 1, 21.0, 0.0, -10.0, 0.0 },
+ { -1, 0, 0, 2, 1, 16.0, 0.0, -8.0, 0.0 },
+ { 1, 0, 0, -2, 1, -13.0, 0.0, 7.0, 0.0 },
+ { -1, 0, 2, 2, 1, -10.0, 0.0, 5.0, 0.0 },
+
+ /* 51-60 */
+ { 1, 1, 0, -2, 0, -7.0, 0.0, 0.0, 0.0 },
+ { 0, 1, 2, 0, 2, 7.0, 0.0, -3.0, 0.0 },
+ { 0, -1, 2, 0, 2, -7.0, 0.0, 3.0, 0.0 },
+ { 1, 0, 2, 2, 2, -8.0, 0.0, 3.0, 0.0 },
+ { 1, 0, 0, 2, 0, 6.0, 0.0, 0.0, 0.0 },
+ { 2, 0, 2, -2, 2, 6.0, 0.0, -3.0, 0.0 },
+ { 0, 0, 0, 2, 1, -6.0, 0.0, 3.0, 0.0 },
+ { 0, 0, 2, 2, 1, -7.0, 0.0, 3.0, 0.0 },
+ { 1, 0, 2, -2, 1, 6.0, 0.0, -3.0, 0.0 },
+ { 0, 0, 0, -2, 1, -5.0, 0.0, 3.0, 0.0 },
+
+ /* 61-70 */
+ { 1, -1, 0, 0, 0, 5.0, 0.0, 0.0, 0.0 },
+ { 2, 0, 2, 0, 1, -5.0, 0.0, 3.0, 0.0 },
+ { 0, 1, 0, -2, 0, -4.0, 0.0, 0.0, 0.0 },
+ { 1, 0, -2, 0, 0, 4.0, 0.0, 0.0, 0.0 },
+ { 0, 0, 0, 1, 0, -4.0, 0.0, 0.0, 0.0 },
+ { 1, 1, 0, 0, 0, -3.0, 0.0, 0.0, 0.0 },
+ { 1, 0, 2, 0, 0, 3.0, 0.0, 0.0, 0.0 },
+ { 1, -1, 2, 0, 2, -3.0, 0.0, 1.0, 0.0 },
+ { -1, -1, 2, 2, 2, -3.0, 0.0, 1.0, 0.0 },
+ { -2, 0, 0, 0, 1, -2.0, 0.0, 1.0, 0.0 },
+
+ /* 71-80 */
+ { 3, 0, 2, 0, 2, -3.0, 0.0, 1.0, 0.0 },
+ { 0, -1, 2, 2, 2, -3.0, 0.0, 1.0, 0.0 },
+ { 1, 1, 2, 0, 2, 2.0, 0.0, -1.0, 0.0 },
+ { -1, 0, 2, -2, 1, -2.0, 0.0, 1.0, 0.0 },
+ { 2, 0, 0, 0, 1, 2.0, 0.0, -1.0, 0.0 },
+ { 1, 0, 0, 0, 2, -2.0, 0.0, 1.0, 0.0 },
+ { 3, 0, 0, 0, 0, 2.0, 0.0, 0.0, 0.0 },
+ { 0, 0, 2, 1, 2, 2.0, 0.0, -1.0, 0.0 },
+ { -1, 0, 0, 0, 2, 1.0, 0.0, -1.0, 0.0 },
+ { 1, 0, 0, -4, 0, -1.0, 0.0, 0.0, 0.0 },
+
+ /* 81-90 */
+ { -2, 0, 2, 2, 2, 1.0, 0.0, -1.0, 0.0 },
+ { -1, 0, 2, 4, 2, -2.0, 0.0, 1.0, 0.0 },
+ { 2, 0, 0, -4, 0, -1.0, 0.0, 0.0, 0.0 },
+ { 1, 1, 2, -2, 2, 1.0, 0.0, -1.0, 0.0 },
+ { 1, 0, 2, 2, 1, -1.0, 0.0, 1.0, 0.0 },
+ { -2, 0, 2, 4, 2, -1.0, 0.0, 1.0, 0.0 },
+ { -1, 0, 4, 0, 2, 1.0, 0.0, 0.0, 0.0 },
+ { 1, -1, 0, -2, 0, 1.0, 0.0, 0.0, 0.0 },
+ { 2, 0, 2, -2, 1, 1.0, 0.0, -1.0, 0.0 },
+ { 2, 0, 2, 2, 2, -1.0, 0.0, 0.0, 0.0 },
+
+ /* 91-100 */
+ { 1, 0, 0, 2, 1, -1.0, 0.0, 0.0, 0.0 },
+ { 0, 0, 4, -2, 2, 1.0, 0.0, 0.0, 0.0 },
+ { 3, 0, 2, -2, 2, 1.0, 0.0, 0.0, 0.0 },
+ { 1, 0, 2, -2, 0, -1.0, 0.0, 0.0, 0.0 },
+ { 0, 1, 2, 0, 1, 1.0, 0.0, 0.0, 0.0 },
+ { -1, -1, 0, 2, 1, 1.0, 0.0, 0.0, 0.0 },
+ { 0, 0, -2, 0, 1, -1.0, 0.0, 0.0, 0.0 },
+ { 0, 0, 2, -1, 2, -1.0, 0.0, 0.0, 0.0 },
+ { 0, 1, 0, 2, 0, -1.0, 0.0, 0.0, 0.0 },
+ { 1, 0, -2, -2, 0, -1.0, 0.0, 0.0, 0.0 },
+
+ /* 101-106 */
+ { 0, -1, 2, 0, 1, -1.0, 0.0, 0.0, 0.0 },
+ { 1, 1, 0, -2, 1, -1.0, 0.0, 0.0, 0.0 },
+ { 1, 0, -2, 2, 0, -1.0, 0.0, 0.0, 0.0 },
+ { 2, 0, 0, 2, 0, 1.0, 0.0, 0.0, 0.0 },
+ { 0, 0, 2, 4, 2, -1.0, 0.0, 0.0, 0.0 },
+ { 0, 1, 0, 1, 0, 1.0, 0.0, 0.0, 0.0 }
+ };
+
+/* Number of terms in the series */
+ const int NT = (int) (sizeof x / sizeof x[0]);
+
+/*--------------------------------------------------------------------*/
+
+/* Interval between fundamental epoch J2000.0 and given date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* --------------------- */
+/* Fundamental arguments */
+/* --------------------- */
+
+/* Mean longitude of Moon minus mean longitude of Moon's perigee. */
+ el = iauAnpm(
+ (485866.733 + (715922.633 + (31.310 + 0.064 * t) * t) * t)
+ * DAS2R + fmod(1325.0 * t, 1.0) * D2PI);
+
+/* Mean longitude of Sun minus mean longitude of Sun's perigee. */
+ elp = iauAnpm(
+ (1287099.804 + (1292581.224 + (-0.577 - 0.012 * t) * t) * t)
+ * DAS2R + fmod(99.0 * t, 1.0) * D2PI);
+
+/* Mean longitude of Moon minus mean longitude of Moon's node. */
+ f = iauAnpm(
+ (335778.877 + (295263.137 + (-13.257 + 0.011 * t) * t) * t)
+ * DAS2R + fmod(1342.0 * t, 1.0) * D2PI);
+
+/* Mean elongation of Moon from Sun. */
+ d = iauAnpm(
+ (1072261.307 + (1105601.328 + (-6.891 + 0.019 * t) * t) * t)
+ * DAS2R + fmod(1236.0 * t, 1.0) * D2PI);
+
+/* Longitude of the mean ascending node of the lunar orbit on the */
+/* ecliptic, measured from the mean equinox of date. */
+ om = iauAnpm(
+ (450160.280 + (-482890.539 + (7.455 + 0.008 * t) * t) * t)
+ * DAS2R + fmod(-5.0 * t, 1.0) * D2PI);
+
+/* --------------- */
+/* Nutation series */
+/* --------------- */
+
+/* Initialize nutation components. */
+ dp = 0.0;
+ de = 0.0;
+
+/* Sum the nutation terms, ending with the biggest. */
+ for (j = NT-1; j >= 0; j--) {
+
+ /* Form argument for current term. */
+ arg = (double)x[j].nl * el
+ + (double)x[j].nlp * elp
+ + (double)x[j].nf * f
+ + (double)x[j].nd * d
+ + (double)x[j].nom * om;
+
+ /* Accumulate current nutation term. */
+ s = x[j].sp + x[j].spt * t;
+ c = x[j].ce + x[j].cet * t;
+ if (s != 0.0) dp += s * sin(arg);
+ if (c != 0.0) de += c * cos(arg);
+ }
+
+/* Convert results from 0.1 mas units to radians. */
+ *dpsi = dp * U2R;
+ *deps = de * U2R;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/nutm80.c b/sofa/nutm80.c
new file mode 100644
index 0000000..baee06e
--- /dev/null
+++ b/sofa/nutm80.c
@@ -0,0 +1,167 @@
+#include "sofam.h"
+
+void iauNutm80(double date1, double date2, double rmatn[3][3])
+/*
+** - - - - - - - - - -
+** i a u N u t m 8 0
+** - - - - - - - - - -
+**
+** Form the matrix of nutation for a given date, IAU 1980 model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TDB date (Note 1)
+**
+** Returned:
+** rmatn double[3][3] nutation matrix
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix operates in the sense V(true) = rmatn * V(mean),
+** where the p-vector V(true) is with respect to the true
+** equatorial triad of date and the p-vector V(mean) is with
+** respect to the mean equatorial triad of date.
+**
+** Called:
+** iauNut80 nutation, IAU 1980
+** iauObl80 mean obliquity, IAU 1980
+** iauNumat form nutation matrix
+**
+** This revision: 2008 May 12
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dpsi, deps, epsa;
+
+
+/* Nutation components and mean obliquity. */
+ iauNut80(date1, date2, &dpsi, &deps);
+ epsa = iauObl80(date1, date2);
+
+/* Build the rotation matrix. */
+ iauNumat(epsa, dpsi, deps, rmatn);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/obl06.c b/sofa/obl06.c
new file mode 100644
index 0000000..f94acf8
--- /dev/null
+++ b/sofa/obl06.c
@@ -0,0 +1,168 @@
+#include "sofam.h"
+
+double iauObl06(double date1, double date2)
+/*
+** - - - - - - - - -
+** i a u O b l 0 6
+** - - - - - - - - -
+**
+** Mean obliquity of the ecliptic, IAU 2006 precession model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned (function value):
+** double obliquity of the ecliptic (radians, Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The result is the angle between the ecliptic and mean equator of
+** date date1+date2.
+**
+** Reference:
+**
+** Hilton, J. et al., 2006, Celest.Mech.Dyn.Astron. 94, 351
+**
+** This revision: 2009 March 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t, eps0;
+
+
+/* Interval between fundamental date J2000.0 and given date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* Mean obliquity. */
+ eps0 = (84381.406 +
+ (-46.836769 +
+ ( -0.0001831 +
+ ( 0.00200340 +
+ ( -0.000000576 +
+ ( -0.0000000434) * t) * t) * t) * t) * t) * DAS2R;
+
+ return eps0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/obl80.c b/sofa/obl80.c
new file mode 100644
index 0000000..27ea3c7
--- /dev/null
+++ b/sofa/obl80.c
@@ -0,0 +1,168 @@
+#include "sofam.h"
+
+double iauObl80(double date1, double date2)
+/*
+** - - - - - - - - -
+** i a u O b l 8 0
+** - - - - - - - - -
+**
+** Mean obliquity of the ecliptic, IAU 1980 model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned (function value):
+** double obliquity of the ecliptic (radians, Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The result is the angle between the ecliptic and mean equator of
+** date date1+date2.
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992),
+** Expression 3.222-1 (p114).
+**
+** This revision: 2009 March 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t, eps0;
+
+
+/* Interval between fundamental epoch J2000.0 and given date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* Mean obliquity of date. */
+ eps0 = DAS2R * (84381.448 +
+ (-46.8150 +
+ (-0.00059 +
+ ( 0.001813) * t) * t) * t);
+
+ return eps0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/p06e.c b/sofa/p06e.c
new file mode 100644
index 0000000..5b6f8cb
--- /dev/null
+++ b/sofa/p06e.c
@@ -0,0 +1,371 @@
+#include "sofam.h"
+
+void iauP06e(double date1, double date2,
+ double *eps0, double *psia, double *oma, double *bpa,
+ double *bqa, double *pia, double *bpia,
+ double *epsa, double *chia, double *za, double *zetaa,
+ double *thetaa, double *pa,
+ double *gam, double *phi, double *psi)
+/*
+** - - - - - - - -
+** i a u P 0 6 e
+** - - - - - - - -
+**
+** Precession angles, IAU 2006, equinox based.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical models.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned (see Note 2):
+** eps0 double epsilon_0
+** psia double psi_A
+** oma double omega_A
+** bpa double P_A
+** bqa double Q_A
+** pia double pi_A
+** bpia double Pi_A
+** epsa double obliquity epsilon_A
+** chia double chi_A
+** za double z_A
+** zetaa double zeta_A
+** thetaa double theta_A
+** pa double p_A
+** gam double F-W angle gamma_J2000
+** phi double F-W angle phi_J2000
+** psi double F-W angle psi_J2000
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) This function returns the set of equinox based angles for the
+** Capitaine et al. "P03" precession theory, adopted by the IAU in
+** 2006. The angles are set out in Table 1 of Hilton et al. (2006):
+**
+** eps0 epsilon_0 obliquity at J2000.0
+** psia psi_A luni-solar precession
+** oma omega_A inclination of equator wrt J2000.0 ecliptic
+** bpa P_A ecliptic pole x, J2000.0 ecliptic triad
+** bqa Q_A ecliptic pole -y, J2000.0 ecliptic triad
+** pia pi_A angle between moving and J2000.0 ecliptics
+** bpia Pi_A longitude of ascending node of the ecliptic
+** epsa epsilon_A obliquity of the ecliptic
+** chia chi_A planetary precession
+** za z_A equatorial precession: -3rd 323 Euler angle
+** zetaa zeta_A equatorial precession: -1st 323 Euler angle
+** thetaa theta_A equatorial precession: 2nd 323 Euler angle
+** pa p_A general precession
+** gam gamma_J2000 J2000.0 RA difference of ecliptic poles
+** phi phi_J2000 J2000.0 codeclination of ecliptic pole
+** psi psi_J2000 longitude difference of equator poles, J2000.0
+**
+** The returned values are all radians.
+**
+** 3) Hilton et al. (2006) Table 1 also contains angles that depend on
+** models distinct from the P03 precession theory itself, namely the
+** IAU 2000A frame bias and nutation. The quoted polynomials are
+** used in other SOFA functions:
+**
+** . iauXy06 contains the polynomial parts of the X and Y series.
+**
+** . iauS06 contains the polynomial part of the s+XY/2 series.
+**
+** . iauPfw06 implements the series for the Fukushima-Williams
+** angles that are with respect to the GCRS pole (i.e. the variants
+** that include frame bias).
+**
+** 4) The IAU resolution stipulated that the choice of parameterization
+** was left to the user, and so an IAU compliant precession
+** implementation can be constructed using various combinations of
+** the angles returned by the present function.
+**
+** 5) The parameterization used by SOFA is the version of the Fukushima-
+** Williams angles that refers directly to the GCRS pole. These
+** angles may be calculated by calling the function iauPfw06. SOFA
+** also supports the direct computation of the CIP GCRS X,Y by
+** series, available by calling iauXy06.
+**
+** 6) The agreement between the different parameterizations is at the
+** 1 microarcsecond level in the present era.
+**
+** 7) When constructing a precession formulation that refers to the GCRS
+** pole rather than the dynamical pole, it may (depending on the
+** choice of angles) be necessary to introduce the frame bias
+** explicitly.
+**
+** 8) It is permissible to re-use the same variable in the returned
+** arguments. The quantities are stored in the stated order.
+**
+** Reference:
+**
+** Hilton, J. et al., 2006, Celest.Mech.Dyn.Astron. 94, 351
+**
+** Called:
+** iauObl06 mean obliquity, IAU 2006
+**
+** This revision: 2011 December 6
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t;
+
+
+/* Interval between fundamental date J2000.0 and given date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* Obliquity at J2000.0. */
+
+ *eps0 = 84381.406 * DAS2R;
+
+/* Luni-solar precession. */
+
+ *psia = ( 5038.481507 +
+ ( -1.0790069 +
+ ( -0.00114045 +
+ ( 0.000132851 +
+ ( -0.0000000951 )
+ * t) * t) * t) * t) * t * DAS2R;
+
+/* Inclination of mean equator with respect to the J2000.0 ecliptic. */
+
+ *oma = *eps0 + ( -0.025754 +
+ ( 0.0512623 +
+ ( -0.00772503 +
+ ( -0.000000467 +
+ ( 0.0000003337 )
+ * t) * t) * t) * t) * t * DAS2R;
+
+/* Ecliptic pole x, J2000.0 ecliptic triad. */
+
+ *bpa = ( 4.199094 +
+ ( 0.1939873 +
+ ( -0.00022466 +
+ ( -0.000000912 +
+ ( 0.0000000120 )
+ * t) * t) * t) * t) * t * DAS2R;
+
+/* Ecliptic pole -y, J2000.0 ecliptic triad. */
+
+ *bqa = ( -46.811015 +
+ ( 0.0510283 +
+ ( 0.00052413 +
+ ( -0.000000646 +
+ ( -0.0000000172 )
+ * t) * t) * t) * t) * t * DAS2R;
+
+/* Angle between moving and J2000.0 ecliptics. */
+
+ *pia = ( 46.998973 +
+ ( -0.0334926 +
+ ( -0.00012559 +
+ ( 0.000000113 +
+ ( -0.0000000022 )
+ * t) * t) * t) * t) * t * DAS2R;
+
+/* Longitude of ascending node of the moving ecliptic. */
+
+ *bpia = ( 629546.7936 +
+ ( -867.95758 +
+ ( 0.157992 +
+ ( -0.0005371 +
+ ( -0.00004797 +
+ ( 0.000000072 )
+ * t) * t) * t) * t) * t) * DAS2R;
+
+/* Mean obliquity of the ecliptic. */
+
+ *epsa = iauObl06(date1, date2);
+
+/* Planetary precession. */
+
+ *chia = ( 10.556403 +
+ ( -2.3814292 +
+ ( -0.00121197 +
+ ( 0.000170663 +
+ ( -0.0000000560 )
+ * t) * t) * t) * t) * t * DAS2R;
+
+/* Equatorial precession: minus the third of the 323 Euler angles. */
+
+ *za = ( -2.650545 +
+ ( 2306.077181 +
+ ( 1.0927348 +
+ ( 0.01826837 +
+ ( -0.000028596 +
+ ( -0.0000002904 )
+ * t) * t) * t) * t) * t) * DAS2R;
+
+/* Equatorial precession: minus the first of the 323 Euler angles. */
+
+ *zetaa = ( 2.650545 +
+ ( 2306.083227 +
+ ( 0.2988499 +
+ ( 0.01801828 +
+ ( -0.000005971 +
+ ( -0.0000003173 )
+ * t) * t) * t) * t) * t) * DAS2R;
+
+/* Equatorial precession: second of the 323 Euler angles. */
+
+ *thetaa = ( 2004.191903 +
+ ( -0.4294934 +
+ ( -0.04182264 +
+ ( -0.000007089 +
+ ( -0.0000001274 )
+ * t) * t) * t) * t) * t * DAS2R;
+
+/* General precession. */
+
+ *pa = ( 5028.796195 +
+ ( 1.1054348 +
+ ( 0.00007964 +
+ ( -0.000023857 +
+ ( 0.0000000383 )
+ * t) * t) * t) * t) * t * DAS2R;
+
+/* Fukushima-Williams angles for precession. */
+
+ *gam = ( 10.556403 +
+ ( 0.4932044 +
+ ( -0.00031238 +
+ ( -0.000002788 +
+ ( 0.0000000260 )
+ * t) * t) * t) * t) * t * DAS2R;
+
+ *phi = *eps0 + ( -46.811015 +
+ ( 0.0511269 +
+ ( 0.00053289 +
+ ( -0.000000440 +
+ ( -0.0000000176 )
+ * t) * t) * t) * t) * t * DAS2R;
+
+ *psi = ( 5038.481507 +
+ ( 1.5584176 +
+ ( -0.00018522 +
+ ( -0.000026452 +
+ ( -0.0000000148 )
+ * t) * t) * t) * t) * t * DAS2R;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/p2pv.c b/sofa/p2pv.c
new file mode 100644
index 0000000..39b14ac
--- /dev/null
+++ b/sofa/p2pv.c
@@ -0,0 +1,133 @@
+#include "sofam.h"
+
+void iauP2pv(double p[3], double pv[2][3])
+/*
+** - - - - - - - -
+** i a u P 2 p v
+** - - - - - - - -
+**
+** Extend a p-vector to a pv-vector by appending a zero velocity.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** p double[3] p-vector
+**
+** Returned:
+** pv double[2][3] pv-vector
+**
+** Called:
+** iauCp copy p-vector
+** iauZp zero p-vector
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauCp(p, pv[0]);
+ iauZp(pv[1]);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/p2s.c b/sofa/p2s.c
new file mode 100644
index 0000000..2cd4157
--- /dev/null
+++ b/sofa/p2s.c
@@ -0,0 +1,141 @@
+#include "sofam.h"
+
+void iauP2s(double p[3], double *theta, double *phi, double *r)
+/*
+** - - - - - - -
+** i a u P 2 s
+** - - - - - - -
+**
+** P-vector to spherical polar coordinates.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** p double[3] p-vector
+**
+** Returned:
+** theta double longitude angle (radians)
+** phi double latitude angle (radians)
+** r double radial distance
+**
+** Notes:
+**
+** 1) If P is null, zero theta, phi and r are returned.
+**
+** 2) At either pole, zero theta is returned.
+**
+** Called:
+** iauC2s p-vector to spherical
+** iauPm modulus of p-vector
+**
+** This revision: 2008 May 22
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauC2s(p, theta, phi);
+ *r = iauPm(p);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pap.c b/sofa/pap.c
new file mode 100644
index 0000000..aca9e96
--- /dev/null
+++ b/sofa/pap.c
@@ -0,0 +1,189 @@
+#include "sofam.h"
+
+double iauPap(double a[3], double b[3])
+/*
+** - - - - - - -
+** i a u P a p
+** - - - - - - -
+**
+** Position-angle from two p-vectors.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double[3] direction of reference point
+** b double[3] direction of point whose PA is required
+**
+** Returned (function value):
+** double position angle of b with respect to a (radians)
+**
+** Notes:
+**
+** 1) The result is the position angle, in radians, of direction b with
+** respect to direction a. It is in the range -pi to +pi. The
+** sense is such that if b is a small distance "north" of a the
+** position angle is approximately zero, and if b is a small
+** distance "east" of a the position angle is approximately +pi/2.
+**
+** 2) The vectors a and b need not be of unit length.
+**
+** 3) Zero is returned if the two directions are the same or if either
+** vector is null.
+**
+** 4) If vector a is at a pole, the result is ill-defined.
+**
+** Called:
+** iauPn decompose p-vector into modulus and direction
+** iauPm modulus of p-vector
+** iauPxp vector product of two p-vectors
+** iauPmp p-vector minus p-vector
+** iauPdp scalar product of two p-vectors
+**
+** This revision: 2008 May 25
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double am, au[3], bm, st, ct, xa, ya, za, eta[3], xi[3], a2b[3], pa;
+
+
+/* Modulus and direction of the a vector. */
+ iauPn(a, &am, au);
+
+/* Modulus of the b vector. */
+ bm = iauPm(b);
+
+/* Deal with the case of a null vector. */
+ if ((am == 0.0) || (bm == 0.0)) {
+ st = 0.0;
+ ct = 1.0;
+ } else {
+
+ /* The "north" axis tangential from a (arbitrary length). */
+ xa = a[0];
+ ya = a[1];
+ za = a[2];
+ eta[0] = -xa * za;
+ eta[1] = -ya * za;
+ eta[2] = xa*xa + ya*ya;
+
+ /* The "east" axis tangential from a (same length). */
+ iauPxp(eta, au, xi);
+
+ /* The vector from a to b. */
+ iauPmp(b, a, a2b);
+
+ /* Resolve into components along the north and east axes. */
+ st = iauPdp(a2b, xi);
+ ct = iauPdp(a2b, eta);
+
+ /* Deal with degenerate cases. */
+ if ((st == 0.0) && (ct == 0.0)) ct = 1.0;
+ }
+
+/* Position angle. */
+ pa = atan2(st, ct);
+
+ return pa;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pas.c b/sofa/pas.c
new file mode 100644
index 0000000..bfc744a
--- /dev/null
+++ b/sofa/pas.c
@@ -0,0 +1,146 @@
+#include "sofam.h"
+
+double iauPas(double al, double ap, double bl, double bp)
+/*
+** - - - - - - -
+** i a u P a s
+** - - - - - - -
+**
+** Position-angle from spherical coordinates.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** al double longitude of point A (e.g. RA) in radians
+** ap double latitude of point A (e.g. Dec) in radians
+** bl double longitude of point B
+** bp double latitude of point B
+**
+** Returned (function value):
+** double position angle of B with respect to A
+**
+** Notes:
+**
+** 1) The result is the bearing (position angle), in radians, of point
+** B with respect to point A. It is in the range -pi to +pi. The
+** sense is such that if B is a small distance "east" of point A,
+** the bearing is approximately +pi/2.
+**
+** 2) Zero is returned if the two points are coincident.
+**
+** This revision: 2008 May 22
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dl, x, y, pa;
+
+
+ dl = bl - al;
+ y = sin(dl) * cos(bp);
+ x = sin(bp) * cos(ap) - cos(bp) * sin(ap) * cos(dl);
+ pa = ((x != 0.0) || (y != 0.0)) ? atan2(y, x) : 0.0;
+
+ return pa;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pb06.c b/sofa/pb06.c
new file mode 100644
index 0000000..4f84af6
--- /dev/null
+++ b/sofa/pb06.c
@@ -0,0 +1,194 @@
+#include "sofam.h"
+
+void iauPb06(double date1, double date2,
+ double *bzeta, double *bz, double *btheta)
+/*
+** - - - - - - - -
+** i a u P b 0 6
+** - - - - - - - -
+**
+** This function forms three Euler angles which implement general
+** precession from epoch J2000.0, using the IAU 2006 model. Frame
+** bias (the offset between ICRS and mean J2000.0) is included.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** bzeta double 1st rotation: radians cw around z
+** bz double 3rd rotation: radians cw around z
+** btheta double 2nd rotation: radians ccw around y
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The traditional accumulated precession angles zeta_A, z_A,
+** theta_A cannot be obtained in the usual way, namely through
+** polynomial expressions, because of the frame bias. The latter
+** means that two of the angles undergo rapid changes near this
+** date. They are instead the results of decomposing the
+** precession-bias matrix obtained by using the Fukushima-Williams
+** method, which does not suffer from the problem. The
+** decomposition returns values which can be used in the
+** conventional formulation and which include frame bias.
+**
+** 3) The three angles are returned in the conventional order, which
+** is not the same as the order of the corresponding Euler
+** rotations. The precession-bias matrix is
+** R_3(-z) x R_2(+theta) x R_3(-zeta).
+**
+** 4) Should zeta_A, z_A, theta_A angles be required that do not
+** contain frame bias, they are available by calling the SOFA
+** function iauP06e.
+**
+** Called:
+** iauPmat06 PB matrix, IAU 2006
+** iauRz rotate around Z-axis
+**
+** This revision: 2008 May 26
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double r[3][3], r31, r32;
+
+
+/* Precession matrix via Fukushima-Williams angles. */
+ iauPmat06(date1, date2, r);
+
+/* Solve for z. */
+ *bz = atan2(r[1][2], r[0][2]);
+
+/* Remove it from the matrix. */
+ iauRz(*bz, r);
+
+/* Solve for the remaining two angles. */
+ *bzeta = atan2 (r[1][0], r[1][1]);
+ r31 = r[2][0];
+ r32 = r[2][1];
+ *btheta = atan2(-dsign(sqrt(r31 * r31 + r32 * r32), r[0][2]),
+ r[2][2]);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pdp.c b/sofa/pdp.c
new file mode 100644
index 0000000..0a34948
--- /dev/null
+++ b/sofa/pdp.c
@@ -0,0 +1,134 @@
+#include "sofam.h"
+
+double iauPdp(double a[3], double b[3])
+/*
+** - - - - - - -
+** i a u P d p
+** - - - - - - -
+**
+** p-vector inner (=scalar=dot) product.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double[3] first p-vector
+** b double[3] second p-vector
+**
+** Returned (function value):
+** double a . b
+**
+** This revision: 2008 May 22
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double w;
+
+
+ w = a[0] * b[0]
+ + a[1] * b[1]
+ + a[2] * b[2];
+
+ return w;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pfw06.c b/sofa/pfw06.c
new file mode 100644
index 0000000..b842627
--- /dev/null
+++ b/sofa/pfw06.c
@@ -0,0 +1,215 @@
+#include "sofam.h"
+
+void iauPfw06(double date1, double date2,
+ double *gamb, double *phib, double *psib, double *epsa)
+/*
+** - - - - - - - - -
+** i a u P f w 0 6
+** - - - - - - - - -
+**
+** Precession angles, IAU 2006 (Fukushima-Williams 4-angle formulation).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** gamb double F-W angle gamma_bar (radians)
+** phib double F-W angle phi_bar (radians)
+** psib double F-W angle psi_bar (radians)
+** epsa double F-W angle epsilon_A (radians)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) Naming the following points:
+**
+** e = J2000.0 ecliptic pole,
+** p = GCRS pole,
+** E = mean ecliptic pole of date,
+** and P = mean pole of date,
+**
+** the four Fukushima-Williams angles are as follows:
+**
+** gamb = gamma_bar = epE
+** phib = phi_bar = pE
+** psib = psi_bar = pEP
+** epsa = epsilon_A = EP
+**
+** 3) The matrix representing the combined effects of frame bias and
+** precession is:
+**
+** PxB = R_1(-epsa).R_3(-psib).R_1(phib).R_3(gamb)
+**
+** 4) The matrix representing the combined effects of frame bias,
+** precession and nutation is simply:
+**
+** NxPxB = R_1(-epsa-dE).R_3(-psib-dP).R_1(phib).R_3(gamb)
+**
+** where dP and dE are the nutation components with respect to the
+** ecliptic of date.
+**
+** Reference:
+**
+** Hilton, J. et al., 2006, Celest.Mech.Dyn.Astron. 94, 351
+**
+** Called:
+** iauObl06 mean obliquity, IAU 2006
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t;
+
+
+/* Interval between fundamental date J2000.0 and given date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* P03 bias+precession angles. */
+ *gamb = ( -0.052928 +
+ ( 10.556378 +
+ ( 0.4932044 +
+ ( -0.00031238 +
+ ( -0.000002788 +
+ ( 0.0000000260 )
+ * t) * t) * t) * t) * t) * DAS2R;
+ *phib = ( 84381.412819 +
+ ( -46.811016 +
+ ( 0.0511268 +
+ ( 0.00053289 +
+ ( -0.000000440 +
+ ( -0.0000000176 )
+ * t) * t) * t) * t) * t) * DAS2R;
+ *psib = ( -0.041775 +
+ ( 5038.481484 +
+ ( 1.5584175 +
+ ( -0.00018522 +
+ ( -0.000026452 +
+ ( -0.0000000148 )
+ * t) * t) * t) * t) * t) * DAS2R;
+ *epsa = iauObl06(date1, date2);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/plan94.c b/sofa/plan94.c
new file mode 100644
index 0000000..916bc10
--- /dev/null
+++ b/sofa/plan94.c
@@ -0,0 +1,564 @@
+#include "sofam.h"
+
+int iauPlan94(double date1, double date2, int np, double pv[2][3])
+/*
+** - - - - - - - - - -
+** i a u P l a n 9 4
+** - - - - - - - - - -
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Approximate heliocentric position and velocity of a nominated major
+** planet: Mercury, Venus, EMB, Mars, Jupiter, Saturn, Uranus or
+** Neptune (but not the Earth itself).
+**
+** Given:
+** date1 double TDB date part A (Note 1)
+** date2 double TDB date part B (Note 1)
+** np int planet (1=Mercury, 2=Venus, 3=EMB, 4=Mars,
+** 5=Jupiter, 6=Saturn, 7=Uranus, 8=Neptune)
+**
+** Returned (argument):
+** pv double[3][2] planet p,v (heliocentric, J2000.0, AU,AU/d)
+**
+** Returned (function value):
+** int status: -1 = illegal NP (outside 1-8)
+** 0 = OK
+** +1 = warning: year outside 1000-3000
+** +2 = warning: failed to converge
+**
+** Notes:
+**
+** 1) The date date1+date2 is in the TDB time scale (in practice TT can
+** be used) and is a Julian Date, apportioned in any convenient way
+** between the two arguments. For example, JD(TDB)=2450123.7 could
+** be expressed in any of these ways, among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in cases
+** where the loss of several decimal digits of resolution is
+** acceptable. The J2000 method is best matched to the way the
+** argument is handled internally and will deliver the optimum
+** resolution. The MJD method and the date & time methods are both
+** good compromises between resolution and convenience. The limited
+** accuracy of the present algorithm is such that any of the methods
+** is satisfactory.
+**
+** 2) If an np value outside the range 1-8 is supplied, an error status
+** (function value -1) is returned and the pv vector set to zeroes.
+**
+** 3) For np=3 the result is for the Earth-Moon Barycenter. To obtain
+** the heliocentric position and velocity of the Earth, use instead
+** the SOFA function iauEpv00.
+**
+** 4) On successful return, the array pv contains the following:
+**
+** pv[0][0] x }
+** pv[1][0] y } heliocentric position, AU
+** pv[2][0] z }
+**
+** pv[0][1] xdot }
+** pv[1][1] ydot } heliocentric velocity, AU/d
+** pv[2][1] zdot }
+**
+** The reference frame is equatorial and is with respect to the
+** mean equator and equinox of epoch J2000.0.
+**
+** 5) The algorithm is due to J.L. Simon, P. Bretagnon, J. Chapront,
+** M. Chapront-Touze, G. Francou and J. Laskar (Bureau des
+** Longitudes, Paris, France). From comparisons with JPL
+** ephemeris DE102, they quote the following maximum errors
+** over the interval 1800-2050:
+**
+** L (arcsec) B (arcsec) R (km)
+**
+** Mercury 4 1 300
+** Venus 5 1 800
+** EMB 6 1 1000
+** Mars 17 1 7700
+** Jupiter 71 5 76000
+** Saturn 81 13 267000
+** Uranus 86 7 712000
+** Neptune 11 1 253000
+**
+** Over the interval 1000-3000, they report that the accuracy is no
+** worse than 1.5 times that over 1800-2050. Outside 1000-3000 the
+** accuracy declines.
+**
+** Comparisons of the present function with the JPL DE200 ephemeris
+** give the following RMS errors over the interval 1960-2025:
+**
+** position (km) velocity (m/s)
+**
+** Mercury 334 0.437
+** Venus 1060 0.855
+** EMB 2010 0.815
+** Mars 7690 1.98
+** Jupiter 71700 7.70
+** Saturn 199000 19.4
+** Uranus 564000 16.4
+** Neptune 158000 14.4
+**
+** Comparisons against DE200 over the interval 1800-2100 gave the
+** following maximum absolute differences. (The results using
+** DE406 were essentially the same.)
+**
+** L (arcsec) B (arcsec) R (km) Rdot (m/s)
+**
+** Mercury 7 1 500 0.7
+** Venus 7 1 1100 0.9
+** EMB 9 1 1300 1.0
+** Mars 26 1 9000 2.5
+** Jupiter 78 6 82000 8.2
+** Saturn 87 14 263000 24.6
+** Uranus 86 7 661000 27.4
+** Neptune 11 2 248000 21.4
+**
+** 6) The present SOFA re-implementation of the original Simon et al.
+** Fortran code differs from the original in the following respects:
+**
+** * C instead of Fortran.
+**
+** * The date is supplied in two parts.
+**
+** * The result is returned only in equatorial Cartesian form;
+** the ecliptic longitude, latitude and radius vector are not
+** returned.
+**
+** * The result is in the J2000.0 equatorial frame, not ecliptic.
+**
+** * More is done in-line: there are fewer calls to subroutines.
+**
+** * Different error/warning status values are used.
+**
+** * A different Kepler's-equation-solver is used (avoiding
+** use of double precision complex).
+**
+** * Polynomials in t are nested to minimize rounding errors.
+**
+** * Explicit double constants are used to avoid mixed-mode
+** expressions.
+**
+** None of the above changes affects the result significantly.
+**
+** 7) The returned status indicates the most serious condition
+** encountered during execution of the function. Illegal np is
+** considered the most serious, overriding failure to converge,
+** which in turn takes precedence over the remote date warning.
+**
+** Called:
+** iauAnp normalize angle into range 0 to 2pi
+**
+** Reference: Simon, J.L, Bretagnon, P., Chapront, J.,
+** Chapront-Touze, M., Francou, G., and Laskar, J.,
+** Astron. Astrophys. 282, 663 (1994).
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Gaussian constant */
+ static const double GK = 0.017202098950;
+
+/* Sin and cos of J2000.0 mean obliquity (IAU 1976) */
+ static const double SINEPS = 0.3977771559319137;
+ static const double COSEPS = 0.9174820620691818;
+
+/* Maximum number of iterations allowed to solve Kepler's equation */
+ static const int KMAX = 10;
+
+ int jstat, i, k;
+ double t, da, dl, de, dp, di, dom, dmu, arga, argl, am,
+ ae, dae, ae2, at, r, v, si2, xq, xp, tl, xsw,
+ xcw, xm2, xf, ci2, xms, xmc, xpxq2, x, y, z;
+
+/* Planetary inverse masses */
+ static const double amas[] = { 6023600.0, /* Mercury */
+ 408523.5, /* Venus */
+ 328900.5, /* EMB */
+ 3098710.0, /* Mars */
+ 1047.355, /* Jupiter */
+ 3498.5, /* Saturn */
+ 22869.0, /* Uranus */
+ 19314.0 }; /* Neptune */
+
+/*
+** Tables giving the mean Keplerian elements, limited to t^2 terms:
+**
+** a semi-major axis (AU)
+** dlm mean longitude (degree and arcsecond)
+** e eccentricity
+** pi longitude of the perihelion (degree and arcsecond)
+** dinc inclination (degree and arcsecond)
+** omega longitude of the ascending node (degree and arcsecond)
+*/
+
+ static const double a[][3] = {
+ { 0.3870983098, 0.0, 0.0 }, /* Mercury */
+ { 0.7233298200, 0.0, 0.0 }, /* Venus */
+ { 1.0000010178, 0.0, 0.0 }, /* EMB */
+ { 1.5236793419, 3e-10, 0.0 }, /* Mars */
+ { 5.2026032092, 19132e-10, -39e-10 }, /* Jupiter */
+ { 9.5549091915, -0.0000213896, 444e-10 }, /* Saturn */
+ { 19.2184460618, -3716e-10, 979e-10 }, /* Uranus */
+ { 30.1103868694, -16635e-10, 686e-10 } /* Neptune */
+ };
+
+ static const double dlm[][3] = {
+ { 252.25090552, 5381016286.88982, -1.92789 },
+ { 181.97980085, 2106641364.33548, 0.59381 },
+ { 100.46645683, 1295977422.83429, -2.04411 },
+ { 355.43299958, 689050774.93988, 0.94264 },
+ { 34.35151874, 109256603.77991, -30.60378 },
+ { 50.07744430, 43996098.55732, 75.61614 },
+ { 314.05500511, 15424811.93933, -1.75083 },
+ { 304.34866548, 7865503.20744, 0.21103 }
+ };
+
+ static const double e[][3] = {
+ { 0.2056317526, 0.0002040653, -28349e-10 },
+ { 0.0067719164, -0.0004776521, 98127e-10 },
+ { 0.0167086342, -0.0004203654, -0.0000126734 },
+ { 0.0934006477, 0.0009048438, -80641e-10 },
+ { 0.0484979255, 0.0016322542, -0.0000471366 },
+ { 0.0555481426, -0.0034664062, -0.0000643639 },
+ { 0.0463812221, -0.0002729293, 0.0000078913 },
+ { 0.0094557470, 0.0000603263, 0.0 }
+ };
+
+ static const double pi[][3] = {
+ { 77.45611904, 5719.11590, -4.83016 },
+ { 131.56370300, 175.48640, -498.48184 },
+ { 102.93734808, 11612.35290, 53.27577 },
+ { 336.06023395, 15980.45908, -62.32800 },
+ { 14.33120687, 7758.75163, 259.95938 },
+ { 93.05723748, 20395.49439, 190.25952 },
+ { 173.00529106, 3215.56238, -34.09288 },
+ { 48.12027554, 1050.71912, 27.39717 }
+ };
+
+ static const double dinc[][3] = {
+ { 7.00498625, -214.25629, 0.28977 },
+ { 3.39466189, -30.84437, -11.67836 },
+ { 0.0, 469.97289, -3.35053 },
+ { 1.84972648, -293.31722, -8.11830 },
+ { 1.30326698, -71.55890, 11.95297 },
+ { 2.48887878, 91.85195, -17.66225 },
+ { 0.77319689, -60.72723, 1.25759 },
+ { 1.76995259, 8.12333, 0.08135 }
+ };
+
+ static const double omega[][3] = {
+ { 48.33089304, -4515.21727, -31.79892 },
+ { 76.67992019, -10008.48154, -51.32614 },
+ { 174.87317577, -8679.27034, 15.34191 },
+ { 49.55809321, -10620.90088, -230.57416 },
+ { 100.46440702, 6362.03561, 326.52178 },
+ { 113.66550252, -9240.19942, -66.23743 },
+ { 74.00595701, 2669.15033, 145.93964 },
+ { 131.78405702, -221.94322, -0.78728 }
+ };
+
+/* Tables for trigonometric terms to be added to the mean elements of */
+/* the semi-major axes */
+
+ static const double kp[][9] = {
+ { 69613, 75645, 88306, 59899, 15746, 71087, 142173, 3086, 0 },
+ { 21863, 32794, 26934, 10931, 26250, 43725, 53867, 28939, 0 },
+ { 16002, 21863, 32004, 10931, 14529, 16368, 15318, 32794, 0 },
+ { 6345, 7818, 15636, 7077, 8184, 14163, 1107, 4872, 0 },
+ { 1760, 1454, 1167, 880, 287, 2640, 19, 2047, 1454 },
+ { 574, 0, 880, 287, 19, 1760, 1167, 306, 574 },
+ { 204, 0, 177, 1265, 4, 385, 200, 208, 204 },
+ { 0, 102, 106, 4, 98, 1367, 487, 204, 0 }
+ };
+
+ static const double ca[][9] = {
+ { 4, -13, 11, -9, -9, -3, -1, 4, 0 },
+ { -156, 59, -42, 6, 19, -20, -10, -12, 0 },
+ { 64, -152, 62, -8, 32, -41, 19, -11, 0 },
+ { 124, 621, -145, 208, 54, -57, 30, 15, 0 },
+ { -23437, -2634, 6601, 6259, -1507,-1821, 2620, -2115, -1489 },
+ { 62911,-119919, 79336,17814,-24241,12068, 8306, -4893, 8902 },
+ { 389061,-262125,-44088, 8387,-22976,-2093, -615, -9720, 6633 },
+ { -412235,-157046,-31430,37817, -9740, -13, -7449, 9644, 0 }
+ };
+
+ static const double sa[][9] = {
+ { -29, -1, 9, 6, -6, 5, 4, 0, 0 },
+ { -48, -125, -26, -37, 18, -13, -20, -2, 0 },
+ { -150, -46, 68, 54, 14, 24, -28, 22, 0 },
+ { -621, 532, -694, -20, 192, -94, 71, -73, 0 },
+ { -14614,-19828, -5869, 1881, -4372, -2255, 782, 930, 913 },
+ { 139737, 0, 24667, 51123, -5102, 7429, -4095, -1976, -9566 },
+ { -138081, 0, 37205,-49039,-41901,-33872,-27037,-12474, 18797 },
+ { 0, 28492,133236, 69654, 52322,-49577,-26430, -3593, 0 }
+ };
+
+/* Tables giving the trigonometric terms to be added to the mean */
+/* elements of the mean longitudes */
+
+ static const double kq[][10] = {
+ { 3086,15746,69613,59899,75645,88306, 12661, 2658, 0, 0 },
+ { 21863,32794,10931, 73, 4387,26934, 1473, 2157, 0, 0 },
+ { 10,16002,21863,10931, 1473,32004, 4387, 73, 0, 0 },
+ { 10, 6345, 7818, 1107,15636, 7077, 8184, 532, 10, 0 },
+ { 19, 1760, 1454, 287, 1167, 880, 574, 2640, 19, 1454 },
+ { 19, 574, 287, 306, 1760, 12, 31, 38, 19, 574 },
+ { 4, 204, 177, 8, 31, 200, 1265, 102, 4, 204 },
+ { 4, 102, 106, 8, 98, 1367, 487, 204, 4, 102 }
+ };
+
+ static const double cl[][10] = {
+ { 21, -95, -157, 41, -5, 42, 23, 30, 0, 0 },
+ { -160, -313, -235, 60, -74, -76, -27, 34, 0, 0 },
+ { -325, -322, -79, 232, -52, 97, 55, -41, 0, 0 },
+ { 2268, -979, 802, 602, -668, -33, 345, 201, -55, 0 },
+ { 7610, -4997,-7689,-5841,-2617, 1115,-748,-607, 6074, 354 },
+ { -18549, 30125,20012, -730, 824, 23,1289,-352, -14767, -2062 },
+ { -135245,-14594, 4197,-4030,-5630,-2898,2540,-306, 2939, 1986 },
+ { 89948, 2103, 8963, 2695, 3682, 1648, 866,-154, -1963, -283 }
+ };
+
+ static const double sl[][10] = {
+ { -342, 136, -23, 62, 66, -52, -33, 17, 0, 0 },
+ { 524, -149, -35, 117, 151, 122, -71, -62, 0, 0 },
+ { -105, -137, 258, 35, -116, -88,-112, -80, 0, 0 },
+ { 854, -205, -936, -240, 140, -341, -97, -232, 536, 0 },
+ { -56980, 8016, 1012, 1448,-3024,-3710, 318, 503, 3767, 577 },
+ { 138606,-13478,-4964, 1441,-1319,-1482, 427, 1236, -9167, -1918 },
+ { 71234,-41116, 5334,-4935,-1848, 66, 434, -1748, 3780, -701 },
+ { -47645, 11647, 2166, 3194, 679, 0,-244, -419, -2531, 48 }
+ };
+
+/*--------------------------------------------------------------------*/
+
+/* Validate the planet number. */
+ if ((np < 1) || (np > 8)) {
+ jstat = -1;
+
+ /* Reset the result in case of failure. */
+ for (k = 0; k < 2; k++) {
+ for (i = 0; i < 3; i++) {
+ pv[k][i] = 0.0;
+ }
+ }
+
+ } else {
+
+ /* Decrement the planet number to start at zero. */
+ np--;
+
+ /* Time: Julian millennia since J2000.0. */
+ t = ((date1 - DJ00) + date2) / DJM;
+
+ /* OK status unless remote date. */
+ jstat = fabs(t) <= 1.0 ? 0 : 1;
+
+ /* Compute the mean elements. */
+ da = a[np][0] +
+ (a[np][1] +
+ a[np][2] * t) * t;
+ dl = (3600.0 * dlm[np][0] +
+ (dlm[np][1] +
+ dlm[np][2] * t) * t) * DAS2R;
+ de = e[np][0] +
+ ( e[np][1] +
+ e[np][2] * t) * t;
+ dp = iauAnpm((3600.0 * pi[np][0] +
+ (pi[np][1] +
+ pi[np][2] * t) * t) * DAS2R);
+ di = (3600.0 * dinc[np][0] +
+ (dinc[np][1] +
+ dinc[np][2] * t) * t) * DAS2R;
+ dom = iauAnpm((3600.0 * omega[np][0] +
+ (omega[np][1] +
+ omega[np][2] * t) * t) * DAS2R);
+
+ /* Apply the trigonometric terms. */
+ dmu = 0.35953620 * t;
+ for (k = 0; k < 8; k++) {
+ arga = kp[np][k] * dmu;
+ argl = kq[np][k] * dmu;
+ da += (ca[np][k] * cos(arga) +
+ sa[np][k] * sin(arga)) * 1e-7;
+ dl += (cl[np][k] * cos(argl) +
+ sl[np][k] * sin(argl)) * 1e-7;
+ }
+ arga = kp[np][8] * dmu;
+ da += t * (ca[np][8] * cos(arga) +
+ sa[np][8] * sin(arga)) * 1e-7;
+ for (k = 8; k < 10; k++) {
+ argl = kq[np][k] * dmu;
+ dl += t * (cl[np][k] * cos(argl) +
+ sl[np][k] * sin(argl)) * 1e-7;
+ }
+ dl = fmod(dl, D2PI);
+
+ /* Iterative soln. of Kepler's equation to get eccentric anomaly. */
+ am = dl - dp;
+ ae = am + de * sin(am);
+ k = 0;
+ dae = 1.0;
+ while (k < KMAX && fabs(dae) > 1e-12) {
+ dae = (am - ae + de * sin(ae)) / (1.0 - de * cos(ae));
+ ae += dae;
+ k++;
+ if (k == KMAX-1) jstat = 2;
+ }
+
+ /* True anomaly. */
+ ae2 = ae / 2.0;
+ at = 2.0 * atan2(sqrt((1.0 + de) / (1.0 - de)) * sin(ae2),
+ cos(ae2));
+
+ /* Distance (AU) and speed (radians per day). */
+ r = da * (1.0 - de * cos(ae));
+ v = GK * sqrt((1.0 + 1.0 / amas[np]) / (da * da * da));
+
+ si2 = sin(di / 2.0);
+ xq = si2 * cos(dom);
+ xp = si2 * sin(dom);
+ tl = at + dp;
+ xsw = sin(tl);
+ xcw = cos(tl);
+ xm2 = 2.0 * (xp * xcw - xq * xsw);
+ xf = da / sqrt(1 - de * de);
+ ci2 = cos(di / 2.0);
+ xms = (de * sin(dp) + xsw) * xf;
+ xmc = (de * cos(dp) + xcw) * xf;
+ xpxq2 = 2 * xp * xq;
+
+ /* Position (J2000.0 ecliptic x,y,z in AU). */
+ x = r * (xcw - xm2 * xp);
+ y = r * (xsw + xm2 * xq);
+ z = r * (-xm2 * ci2);
+
+ /* Rotate to equatorial. */
+ pv[0][0] = x;
+ pv[0][1] = y * COSEPS - z * SINEPS;
+ pv[0][2] = y * SINEPS + z * COSEPS;
+
+ /* Velocity (J2000.0 ecliptic xdot,ydot,zdot in AU/d). */
+ x = v * (( -1.0 + 2.0 * xp * xp) * xms + xpxq2 * xmc);
+ y = v * (( 1.0 - 2.0 * xq * xq) * xmc - xpxq2 * xms);
+ z = v * (2.0 * ci2 * (xp * xms + xq * xmc));
+
+ /* Rotate to equatorial. */
+ pv[1][0] = x;
+ pv[1][1] = y * COSEPS - z * SINEPS;
+ pv[1][2] = y * SINEPS + z * COSEPS;
+
+ }
+
+/* Return the status. */
+ return jstat;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pm.c b/sofa/pm.c
new file mode 100644
index 0000000..23c06dd
--- /dev/null
+++ b/sofa/pm.c
@@ -0,0 +1,133 @@
+#include "sofam.h"
+
+double iauPm(double p[3])
+/*
+** - - - - - -
+** i a u P m
+** - - - - - -
+**
+** Modulus of p-vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** p double[3] p-vector
+**
+** Returned (function value):
+** double modulus
+**
+** This revision: 2008 May 22
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double w;
+
+
+ w = sqrt( p[0] * p[0]
+ + p[1] * p[1]
+ + p[2] * p[2] );
+
+ return w;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pmat00.c b/sofa/pmat00.c
new file mode 100644
index 0000000..f63f0f8
--- /dev/null
+++ b/sofa/pmat00.c
@@ -0,0 +1,168 @@
+#include "sofam.h"
+
+void iauPmat00(double date1, double date2, double rbp[3][3])
+/*
+** - - - - - - - - - -
+** i a u P m a t 0 0
+** - - - - - - - - - -
+**
+** Precession matrix (including frame bias) from GCRS to a specified
+** date, IAU 2000 model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rbp double[3][3] bias-precession matrix (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix operates in the sense V(date) = rbp * V(GCRS), where
+** the p-vector V(GCRS) is with respect to the Geocentric Celestial
+** Reference System (IAU, 2000) and the p-vector V(date) is with
+** respect to the mean equatorial triad of the given date.
+**
+** Called:
+** iauBp00 frame bias and precession matrices, IAU 2000
+**
+** Reference:
+**
+** IAU: Trans. International Astronomical Union, Vol. XXIVB; Proc.
+** 24th General Assembly, Manchester, UK. Resolutions B1.3, B1.6.
+** (2000)
+**
+** This revision: 2009 December 21
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rb[3][3], rp[3][3];
+
+
+/* Obtain the required matrix (discarding others). */
+ iauBp00(date1, date2, rb, rp, rbp);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pmat06.c b/sofa/pmat06.c
new file mode 100644
index 0000000..ecb9d97
--- /dev/null
+++ b/sofa/pmat06.c
@@ -0,0 +1,172 @@
+#include "sofam.h"
+
+void iauPmat06(double date1, double date2, double rbp[3][3])
+/*
+** - - - - - - - - - -
+** i a u P m a t 0 6
+** - - - - - - - - - -
+**
+** Precession matrix (including frame bias) from GCRS to a specified
+** date, IAU 2006 model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rbp double[3][3] bias-precession matrix (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix operates in the sense V(date) = rbp * V(GCRS), where
+** the p-vector V(GCRS) is with respect to the Geocentric Celestial
+** Reference System (IAU, 2000) and the p-vector V(date) is with
+** respect to the mean equatorial triad of the given date.
+**
+** Called:
+** iauPfw06 bias-precession F-W angles, IAU 2006
+** iauFw2m F-W angles to r-matrix
+**
+** References:
+**
+** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855
+**
+** Wallace, P.T. & Capitaine, N., 2006, Astron.Astrophys. 459, 981
+**
+** This revision: 2009 December 21
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double gamb, phib, psib, epsa;
+
+
+/* Bias-precession Fukushima-Williams angles. */
+ iauPfw06(date1, date2, &gamb, &phib, &psib, &epsa);
+
+/* Form the matrix. */
+ iauFw2m(gamb, phib, psib, epsa, rbp);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pmat76.c b/sofa/pmat76.c
new file mode 100644
index 0000000..304c6d6
--- /dev/null
+++ b/sofa/pmat76.c
@@ -0,0 +1,191 @@
+#include "sofam.h"
+
+void iauPmat76(double date1, double date2, double rmatp[3][3])
+/*
+** - - - - - - - - - -
+** i a u P m a t 7 6
+** - - - - - - - - - -
+**
+** Precession matrix from J2000.0 to a specified date, IAU 1976 model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double ending date, TT (Note 1)
+**
+** Returned:
+** rmatp double[3][3] precession matrix, J2000.0 -> date1+date2
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix operates in the sense V(date) = RMATP * V(J2000),
+** where the p-vector V(J2000) is with respect to the mean
+** equatorial triad of epoch J2000.0 and the p-vector V(date)
+** is with respect to the mean equatorial triad of the given
+** date.
+**
+** 3) Though the matrix method itself is rigorous, the precession
+** angles are expressed through canonical polynomials which are
+** valid only for a limited time span. In addition, the IAU 1976
+** precession rate is known to be imperfect. The absolute accuracy
+** of the present formulation is better than 0.1 arcsec from
+** 1960AD to 2040AD, better than 1 arcsec from 1640AD to 2360AD,
+** and remains below 3 arcsec for the whole of the period
+** 500BC to 3000AD. The errors exceed 10 arcsec outside the
+** range 1200BC to 3900AD, exceed 100 arcsec outside 4200BC to
+** 5600AD and exceed 1000 arcsec outside 6800BC to 8200AD.
+**
+** Called:
+** iauPrec76 accumulated precession angles, IAU 1976
+** iauIr initialize r-matrix to identity
+** iauRz rotate around Z-axis
+** iauRy rotate around Y-axis
+** iauCr copy r-matrix
+**
+** References:
+**
+** Lieske, J.H., 1979, Astron.Astrophys. 73, 282.
+** equations (6) & (7), p283.
+**
+** Kaplan,G.H., 1981. USNO circular no. 163, pA2.
+**
+** This revision: 2009 December 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double zeta, z, theta, wmat[3][3];
+
+
+/* Precession Euler angles, J2000.0 to specified date. */
+ iauPrec76(DJ00, 0.0, date1, date2, &zeta, &z, &theta);
+
+/* Form the rotation matrix. */
+ iauIr( wmat);
+ iauRz( -zeta, wmat);
+ iauRy( theta, wmat);
+ iauRz( -z, wmat);
+ iauCr( wmat, rmatp);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pmp.c b/sofa/pmp.c
new file mode 100644
index 0000000..b691cd9
--- /dev/null
+++ b/sofa/pmp.c
@@ -0,0 +1,135 @@
+#include "sofam.h"
+
+void iauPmp(double a[3], double b[3], double amb[3])
+/*
+** - - - - - - -
+** i a u P m p
+** - - - - - - -
+**
+** P-vector subtraction.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double[3] first p-vector
+** b double[3] second p-vector
+**
+** Returned:
+** amb double[3] a - b
+**
+** Note:
+** It is permissible to re-use the same array for any of the
+** arguments.
+**
+** This revision: 2008 November 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ amb[0] = a[0] - b[0];
+ amb[1] = a[1] - b[1];
+ amb[2] = a[2] - b[2];
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pn.c b/sofa/pn.c
new file mode 100644
index 0000000..37401f7
--- /dev/null
+++ b/sofa/pn.c
@@ -0,0 +1,159 @@
+#include "sofam.h"
+
+void iauPn(double p[3], double *r, double u[3])
+/*
+** - - - - - -
+** i a u P n
+** - - - - - -
+**
+** Convert a p-vector into modulus and unit vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** p double[3] p-vector
+**
+** Returned:
+** r double modulus
+** u double[3] unit vector
+**
+** Notes:
+**
+** 1) If p is null, the result is null. Otherwise the result is a unit
+** vector.
+**
+** 2) It is permissible to re-use the same array for any of the
+** arguments.
+**
+** Called:
+** iauPm modulus of p-vector
+** iauZp zero p-vector
+** iauSxp multiply p-vector by scalar
+**
+** This revision: 2008 November 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double w;
+
+
+/* Obtain the modulus and test for zero. */
+ w = iauPm(p);
+ if (w == 0.0) {
+
+ /* Null vector. */
+ iauZp(u);
+
+ } else {
+
+ /* Unit vector. */
+ iauSxp(1.0/w, p, u);
+ }
+
+/* Return the modulus. */
+ *r = w;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pn00.c b/sofa/pn00.c
new file mode 100644
index 0000000..6ae880c
--- /dev/null
+++ b/sofa/pn00.c
@@ -0,0 +1,227 @@
+#include "sofam.h"
+
+void iauPn00(double date1, double date2, double dpsi, double deps,
+ double *epsa,
+ double rb[3][3], double rp[3][3], double rbp[3][3],
+ double rn[3][3], double rbpn[3][3])
+/*
+** - - - - - - - -
+** i a u P n 0 0
+** - - - - - - - -
+**
+** Precession-nutation, IAU 2000 model: a multi-purpose function,
+** supporting classical (equinox-based) use directly and CIO-based
+** use indirectly.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+** dpsi,deps double nutation (Note 2)
+**
+** Returned:
+** epsa double mean obliquity (Note 3)
+** rb double[3][3] frame bias matrix (Note 4)
+** rp double[3][3] precession matrix (Note 5)
+** rbp double[3][3] bias-precession matrix (Note 6)
+** rn double[3][3] nutation matrix (Note 7)
+** rbpn double[3][3] GCRS-to-true matrix (Note 8)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The caller is responsible for providing the nutation components;
+** they are in longitude and obliquity, in radians and are with
+** respect to the equinox and ecliptic of date. For high-accuracy
+** applications, free core nutation should be included as well as
+** any other relevant corrections to the position of the CIP.
+**
+** 3) The returned mean obliquity is consistent with the IAU 2000
+** precession-nutation models.
+**
+** 4) The matrix rb transforms vectors from GCRS to J2000.0 mean
+** equator and equinox by applying frame bias.
+**
+** 5) The matrix rp transforms vectors from J2000.0 mean equator and
+** equinox to mean equator and equinox of date by applying
+** precession.
+**
+** 6) The matrix rbp transforms vectors from GCRS to mean equator and
+** equinox of date by applying frame bias then precession. It is
+** the product rp x rb.
+**
+** 7) The matrix rn transforms vectors from mean equator and equinox of
+** date to true equator and equinox of date by applying the nutation
+** (luni-solar + planetary).
+**
+** 8) The matrix rbpn transforms vectors from GCRS to true equator and
+** equinox of date. It is the product rn x rbp, applying frame
+** bias, precession and nutation in that order.
+**
+** 9) It is permissible to re-use the same array in the returned
+** arguments. The arrays are filled in the order given.
+**
+** Called:
+** iauPr00 IAU 2000 precession adjustments
+** iauObl80 mean obliquity, IAU 1980
+** iauBp00 frame bias and precession matrices, IAU 2000
+** iauCr copy r-matrix
+** iauNumat form nutation matrix
+** iauRxr product of two r-matrices
+**
+** Reference:
+**
+** Capitaine, N., Chapront, J., Lambert, S. and Wallace, P.,
+** "Expressions for the Celestial Intermediate Pole and Celestial
+** Ephemeris Origin consistent with the IAU 2000A precession-
+** nutation model", Astron.Astrophys. 400, 1145-1154 (2003)
+**
+** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
+** intermediate origin" (CIO) by IAU 2006 Resolution 2.
+**
+** This revision: 2010 January 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dpsipr, depspr, rbpw[3][3], rnw[3][3];
+
+
+/* IAU 2000 precession-rate adjustments. */
+ iauPr00(date1, date2, &dpsipr, &depspr);
+
+/* Mean obliquity, consistent with IAU 2000 precession-nutation. */
+ *epsa = iauObl80(date1, date2) + depspr;
+
+/* Frame bias and precession matrices and their product. */
+ iauBp00(date1, date2, rb, rp, rbpw);
+ iauCr(rbpw, rbp);
+
+/* Nutation matrix. */
+ iauNumat(*epsa, dpsi, deps, rnw);
+ iauCr(rnw, rn);
+
+/* Bias-precession-nutation matrix (classical). */
+ iauRxr(rnw, rbpw, rbpn);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pn00a.c b/sofa/pn00a.c
new file mode 100644
index 0000000..0245962
--- /dev/null
+++ b/sofa/pn00a.c
@@ -0,0 +1,212 @@
+#include "sofam.h"
+
+void iauPn00a(double date1, double date2,
+ double *dpsi, double *deps, double *epsa,
+ double rb[3][3], double rp[3][3], double rbp[3][3],
+ double rn[3][3], double rbpn[3][3])
+/*
+** - - - - - - - - -
+** i a u P n 0 0 a
+** - - - - - - - - -
+**
+** Precession-nutation, IAU 2000A model: a multi-purpose function,
+** supporting classical (equinox-based) use directly and CIO-based
+** use indirectly.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** dpsi,deps double nutation (Note 2)
+** epsa double mean obliquity (Note 3)
+** rb double[3][3] frame bias matrix (Note 4)
+** rp double[3][3] precession matrix (Note 5)
+** rbp double[3][3] bias-precession matrix (Note 6)
+** rn double[3][3] nutation matrix (Note 7)
+** rbpn double[3][3] GCRS-to-true matrix (Notes 8,9)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The nutation components (luni-solar + planetary, IAU 2000A) in
+** longitude and obliquity are in radians and with respect to the
+** equinox and ecliptic of date. Free core nutation is omitted;
+** for the utmost accuracy, use the iauPn00 function, where the
+** nutation components are caller-specified. For faster but
+** slightly less accurate results, use the iauPn00b function.
+**
+** 3) The mean obliquity is consistent with the IAU 2000 precession.
+**
+** 4) The matrix rb transforms vectors from GCRS to J2000.0 mean
+** equator and equinox by applying frame bias.
+**
+** 5) The matrix rp transforms vectors from J2000.0 mean equator and
+** equinox to mean equator and equinox of date by applying
+** precession.
+**
+** 6) The matrix rbp transforms vectors from GCRS to mean equator and
+** equinox of date by applying frame bias then precession. It is
+** the product rp x rb.
+**
+** 7) The matrix rn transforms vectors from mean equator and equinox
+** of date to true equator and equinox of date by applying the
+** nutation (luni-solar + planetary).
+**
+** 8) The matrix rbpn transforms vectors from GCRS to true equator and
+** equinox of date. It is the product rn x rbp, applying frame
+** bias, precession and nutation in that order.
+**
+** 9) The X,Y,Z coordinates of the IAU 2000B Celestial Intermediate
+** Pole are elements (3,1-3) of the matrix rbpn.
+**
+** 10) It is permissible to re-use the same array in the returned
+** arguments. The arrays are filled in the order given.
+**
+** Called:
+** iauNut00a nutation, IAU 2000A
+** iauPn00 bias/precession/nutation results, IAU 2000
+**
+** Reference:
+**
+** Capitaine, N., Chapront, J., Lambert, S. and Wallace, P.,
+** "Expressions for the Celestial Intermediate Pole and Celestial
+** Ephemeris Origin consistent with the IAU 2000A precession-
+** nutation model", Astron.Astrophys. 400, 1145-1154 (2003)
+**
+** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
+** intermediate origin" (CIO) by IAU 2006 Resolution 2.
+**
+** This revision: 2010 January 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Nutation. */
+ iauNut00a(date1, date2, dpsi, deps);
+
+/* Remaining results. */
+ iauPn00(date1, date2, *dpsi, *deps, epsa, rb, rp, rbp, rn, rbpn);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pn00b.c b/sofa/pn00b.c
new file mode 100644
index 0000000..a35cd51
--- /dev/null
+++ b/sofa/pn00b.c
@@ -0,0 +1,212 @@
+#include "sofam.h"
+
+void iauPn00b(double date1, double date2,
+ double *dpsi, double *deps, double *epsa,
+ double rb[3][3], double rp[3][3], double rbp[3][3],
+ double rn[3][3], double rbpn[3][3])
+/*
+** - - - - - - - - -
+** i a u P n 0 0 b
+** - - - - - - - - -
+**
+** Precession-nutation, IAU 2000B model: a multi-purpose function,
+** supporting classical (equinox-based) use directly and CIO-based
+** use indirectly.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** dpsi,deps double nutation (Note 2)
+** epsa double mean obliquity (Note 3)
+** rb double[3][3] frame bias matrix (Note 4)
+** rp double[3][3] precession matrix (Note 5)
+** rbp double[3][3] bias-precession matrix (Note 6)
+** rn double[3][3] nutation matrix (Note 7)
+** rbpn double[3][3] GCRS-to-true matrix (Notes 8,9)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The nutation components (luni-solar + planetary, IAU 2000B) in
+** longitude and obliquity are in radians and with respect to the
+** equinox and ecliptic of date. For more accurate results, but
+** at the cost of increased computation, use the iauPn00a function.
+** For the utmost accuracy, use the iauPn00 function, where the
+** nutation components are caller-specified.
+**
+** 3) The mean obliquity is consistent with the IAU 2000 precession.
+**
+** 4) The matrix rb transforms vectors from GCRS to J2000.0 mean
+** equator and equinox by applying frame bias.
+**
+** 5) The matrix rp transforms vectors from J2000.0 mean equator and
+** equinox to mean equator and equinox of date by applying
+** precession.
+**
+** 6) The matrix rbp transforms vectors from GCRS to mean equator and
+** equinox of date by applying frame bias then precession. It is
+** the product rp x rb.
+**
+** 7) The matrix rn transforms vectors from mean equator and equinox
+** of date to true equator and equinox of date by applying the
+** nutation (luni-solar + planetary).
+**
+** 8) The matrix rbpn transforms vectors from GCRS to true equator and
+** equinox of date. It is the product rn x rbp, applying frame
+** bias, precession and nutation in that order.
+**
+** 9) The X,Y,Z coordinates of the IAU 2000B Celestial Intermediate
+** Pole are elements (3,1-3) of the matrix rbpn.
+**
+** 10) It is permissible to re-use the same array in the returned
+** arguments. The arrays are filled in the stated order.
+**
+** Called:
+** iauNut00b nutation, IAU 2000B
+** iauPn00 bias/precession/nutation results, IAU 2000
+**
+** Reference:
+**
+** Capitaine, N., Chapront, J., Lambert, S. and Wallace, P.,
+** "Expressions for the Celestial Intermediate Pole and Celestial
+** Ephemeris Origin consistent with the IAU 2000A precession-
+** nutation model", Astron.Astrophys. 400, 1145-1154 (2003).
+**
+** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
+** intermediate origin" (CIO) by IAU 2006 Resolution 2.
+**
+** This revision: 2010 January 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Nutation. */
+ iauNut00b(date1, date2, dpsi, deps);
+
+/* Remaining results. */
+ iauPn00(date1, date2, *dpsi, *deps, epsa, rb, rp, rbp, rn, rbpn);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pn06.c b/sofa/pn06.c
new file mode 100644
index 0000000..1eb92ef
--- /dev/null
+++ b/sofa/pn06.c
@@ -0,0 +1,237 @@
+#include "sofam.h"
+
+void iauPn06(double date1, double date2, double dpsi, double deps,
+ double *epsa,
+ double rb[3][3], double rp[3][3], double rbp[3][3],
+ double rn[3][3], double rbpn[3][3])
+/*
+** - - - - - - - -
+** i a u P n 0 6
+** - - - - - - - -
+**
+** Precession-nutation, IAU 2006 model: a multi-purpose function,
+** supporting classical (equinox-based) use directly and CIO-based use
+** indirectly.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+** dpsi,deps double nutation (Note 2)
+**
+** Returned:
+** epsa double mean obliquity (Note 3)
+** rb double[3][3] frame bias matrix (Note 4)
+** rp double[3][3] precession matrix (Note 5)
+** rbp double[3][3] bias-precession matrix (Note 6)
+** rn double[3][3] nutation matrix (Note 7)
+** rbpn double[3][3] GCRS-to-true matrix (Note 8)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The caller is responsible for providing the nutation components;
+** they are in longitude and obliquity, in radians and are with
+** respect to the equinox and ecliptic of date. For high-accuracy
+** applications, free core nutation should be included as well as
+** any other relevant corrections to the position of the CIP.
+**
+** 3) The returned mean obliquity is consistent with the IAU 2006
+** precession.
+**
+** 4) The matrix rb transforms vectors from GCRS to J2000.0 mean
+** equator and equinox by applying frame bias.
+**
+** 5) The matrix rp transforms vectors from J2000.0 mean equator and
+** equinox to mean equator and equinox of date by applying
+** precession.
+**
+** 6) The matrix rbp transforms vectors from GCRS to mean equator and
+** equinox of date by applying frame bias then precession. It is
+** the product rp x rb.
+**
+** 7) The matrix rn transforms vectors from mean equator and equinox
+** of date to true equator and equinox of date by applying the
+** nutation (luni-solar + planetary).
+**
+** 8) The matrix rbpn transforms vectors from GCRS to true equator and
+** equinox of date. It is the product rn x rbp, applying frame
+** bias, precession and nutation in that order.
+**
+** 9) The X,Y,Z coordinates of the IAU 2000B Celestial Intermediate
+** Pole are elements (3,1-3) of the matrix rbpn.
+**
+** 10) It is permissible to re-use the same array in the returned
+** arguments. The arrays are filled in the stated order.
+**
+** Called:
+** iauPfw06 bias-precession F-W angles, IAU 2006
+** iauFw2m F-W angles to r-matrix
+** iauCr copy r-matrix
+** iauTr transpose r-matrix
+** iauRxr product of two r-matrices
+**
+** References:
+**
+** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855
+**
+** Wallace, P.T. & Capitaine, N., 2006, Astron.Astrophys. 459, 981
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double gamb, phib, psib, eps, r1[3][3], r2[3][3], rt[3][3];
+
+
+/* Bias-precession Fukushima-Williams angles of J2000.0 = frame bias. */
+ iauPfw06(DJM0, DJM00, &gamb, &phib, &psib, &eps);
+
+/* B matrix. */
+ iauFw2m(gamb, phib, psib, eps, r1);
+ iauCr(r1, rb);
+
+/* Bias-precession Fukushima-Williams angles of date. */
+ iauPfw06(date1, date2, &gamb, &phib, &psib, &eps);
+
+/* Bias-precession matrix. */
+ iauFw2m(gamb, phib, psib, eps, r2);
+ iauCr(r2, rbp);
+
+/* Solve for precession matrix. */
+ iauTr(r1, rt);
+ iauRxr(r2, rt, rp);
+
+/* Equinox-based bias-precession-nutation matrix. */
+ iauFw2m(gamb, phib, psib + dpsi, eps + deps, r1);
+ iauCr(r1, rbpn);
+
+/* Solve for nutation matrix. */
+ iauTr(r2, rt);
+ iauRxr(r1, rt, rn);
+
+/* Obliquity, mean of date. */
+ *epsa = eps;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pn06a.c b/sofa/pn06a.c
new file mode 100644
index 0000000..e70cfdc
--- /dev/null
+++ b/sofa/pn06a.c
@@ -0,0 +1,202 @@
+#include "sofam.h"
+
+void iauPn06a(double date1, double date2,
+ double *dpsi, double *deps, double *epsa,
+ double rb[3][3], double rp[3][3], double rbp[3][3],
+ double rn[3][3], double rbpn[3][3])
+/*
+** - - - - - - - - -
+** i a u P n 0 6 a
+** - - - - - - - - -
+**
+** Precession-nutation, IAU 2006/2000A models: a multi-purpose function,
+** supporting classical (equinox-based) use directly and CIO-based use
+** indirectly.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** dpsi,deps double nutation (Note 2)
+** epsa double mean obliquity (Note 3)
+** rb double[3][3] frame bias matrix (Note 4)
+** rp double[3][3] precession matrix (Note 5)
+** rbp double[3][3] bias-precession matrix (Note 6)
+** rn double[3][3] nutation matrix (Note 7)
+** rbpn double[3][3] GCRS-to-true matrix (Notes 8,9)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The nutation components (luni-solar + planetary, IAU 2000A) in
+** longitude and obliquity are in radians and with respect to the
+** equinox and ecliptic of date. Free core nutation is omitted;
+** for the utmost accuracy, use the iauPn06 function, where the
+** nutation components are caller-specified.
+**
+** 3) The mean obliquity is consistent with the IAU 2006 precession.
+**
+** 4) The matrix rb transforms vectors from GCRS to mean J2000.0 by
+** applying frame bias.
+**
+** 5) The matrix rp transforms vectors from mean J2000.0 to mean of
+** date by applying precession.
+**
+** 6) The matrix rbp transforms vectors from GCRS to mean of date by
+** applying frame bias then precession. It is the product rp x rb.
+**
+** 7) The matrix rn transforms vectors from mean of date to true of
+** date by applying the nutation (luni-solar + planetary).
+**
+** 8) The matrix rbpn transforms vectors from GCRS to true of date
+** (CIP/equinox). It is the product rn x rbp, applying frame bias,
+** precession and nutation in that order.
+**
+** 9) The X,Y,Z coordinates of the IAU 2006/2000A Celestial
+** Intermediate Pole are elements (1,1-3) of the matrix rbpn.
+**
+** 10) It is permissible to re-use the same array in the returned
+** arguments. The arrays are filled in the stated order.
+**
+** Called:
+** iauNut06a nutation, IAU 2006/2000A
+** iauPn06 bias/precession/nutation results, IAU 2006
+**
+** Reference:
+**
+** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855
+**
+** This revision: 2009 December 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Nutation. */
+ iauNut06a(date1, date2, dpsi, deps);
+
+/* Remaining results. */
+ iauPn06(date1, date2, *dpsi, *deps, epsa, rb, rp, rbp, rn, rbpn);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pnm00a.c b/sofa/pnm00a.c
new file mode 100644
index 0000000..d899d65
--- /dev/null
+++ b/sofa/pnm00a.c
@@ -0,0 +1,171 @@
+#include "sofam.h"
+
+void iauPnm00a(double date1, double date2, double rbpn[3][3])
+/*
+** - - - - - - - - - -
+** i a u P n m 0 0 a
+** - - - - - - - - - -
+**
+** Form the matrix of precession-nutation for a given date (including
+** frame bias), equinox-based, IAU 2000A model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rbpn double[3][3] classical NPB matrix (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix operates in the sense V(date) = rbpn * V(GCRS), where
+** the p-vector V(date) is with respect to the true equatorial triad
+** of date date1+date2 and the p-vector V(GCRS) is with respect to
+** the Geocentric Celestial Reference System (IAU, 2000).
+**
+** 3) A faster, but slightly less accurate result (about 1 mas), can be
+** obtained by using instead the iauPnm00b function.
+**
+** Called:
+** iauPn00a bias/precession/nutation, IAU 2000A
+**
+** Reference:
+**
+** IAU: Trans. International Astronomical Union, Vol. XXIVB; Proc.
+** 24th General Assembly, Manchester, UK. Resolutions B1.3, B1.6.
+** (2000)
+**
+** This revision: 2009 December 21
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dpsi, deps, epsa, rb[3][3], rp[3][3], rbp[3][3], rn[3][3];
+
+
+/* Obtain the required matrix (discarding other results). */
+ iauPn00a(date1, date2, &dpsi, &deps, &epsa, rb, rp, rbp, rn, rbpn);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pnm00b.c b/sofa/pnm00b.c
new file mode 100644
index 0000000..c0136b0
--- /dev/null
+++ b/sofa/pnm00b.c
@@ -0,0 +1,171 @@
+#include "sofam.h"
+
+void iauPnm00b(double date1, double date2, double rbpn[3][3])
+/*
+** - - - - - - - - - -
+** i a u P n m 0 0 b
+** - - - - - - - - - -
+**
+** Form the matrix of precession-nutation for a given date (including
+** frame bias), equinox-based, IAU 2000B model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rbpn double[3][3] bias-precession-nutation matrix (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix operates in the sense V(date) = rbpn * V(GCRS), where
+** the p-vector V(date) is with respect to the true equatorial triad
+** of date date1+date2 and the p-vector V(GCRS) is with respect to
+** the Geocentric Celestial Reference System (IAU, 2000).
+**
+** 3) The present function is faster, but slightly less accurate (about
+** 1 mas), than the iauPnm00a function.
+**
+** Called:
+** iauPn00b bias/precession/nutation, IAU 2000B
+**
+** Reference:
+**
+** IAU: Trans. International Astronomical Union, Vol. XXIVB; Proc.
+** 24th General Assembly, Manchester, UK. Resolutions B1.3, B1.6.
+** (2000)
+**
+** This revision: 2009 December 21
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dpsi, deps, epsa, rb[3][3], rp[3][3], rbp[3][3], rn[3][3];
+
+
+/* Obtain the required matrix (discarding other results). */
+ iauPn00b(date1, date2, &dpsi, &deps, &epsa, rb, rp, rbp, rn, rbpn);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pnm06a.c b/sofa/pnm06a.c
new file mode 100644
index 0000000..8085742
--- /dev/null
+++ b/sofa/pnm06a.c
@@ -0,0 +1,174 @@
+#include "sofam.h"
+
+void iauPnm06a(double date1, double date2, double rnpb[3][3])
+/*
+** - - - - - - - - - -
+** i a u P n m 0 6 a
+** - - - - - - - - - -
+**
+** Form the matrix of precession-nutation for a given date (including
+** frame bias), IAU 2006 precession and IAU 2000A nutation models.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** rnpb double[3][3] bias-precession-nutation matrix (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix operates in the sense V(date) = rnpb * V(GCRS), where
+** the p-vector V(date) is with respect to the true equatorial triad
+** of date date1+date2 and the p-vector V(GCRS) is with respect to
+** the Geocentric Celestial Reference System (IAU, 2000).
+**
+** Called:
+** iauPfw06 bias-precession F-W angles, IAU 2006
+** iauNut06a nutation, IAU 2006/2000A
+** iauFw2m F-W angles to r-matrix
+**
+** Reference:
+**
+** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855.
+**
+** This revision: 2009 December 21
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double gamb, phib, psib, epsa, dp, de;
+
+
+/* Fukushima-Williams angles for frame bias and precession. */
+ iauPfw06(date1, date2, &gamb, &phib, &psib, &epsa);
+
+/* Nutation components. */
+ iauNut06a(date1, date2, &dp, &de);
+
+/* Equinox based nutation x precession x bias matrix. */
+ iauFw2m(gamb, phib, psib + dp, epsa + de, rnpb);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pnm80.c b/sofa/pnm80.c
new file mode 100644
index 0000000..ce1750e
--- /dev/null
+++ b/sofa/pnm80.c
@@ -0,0 +1,176 @@
+#include "sofam.h"
+
+void iauPnm80(double date1, double date2, double rmatpn[3][3])
+/*
+** - - - - - - - - -
+** i a u P n m 8 0
+** - - - - - - - - -
+**
+** Form the matrix of precession/nutation for a given date, IAU 1976
+** precession model, IAU 1980 nutation model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TDB date (Note 1)
+**
+** Returned:
+** rmatpn double[3][3] combined precession/nutation matrix
+**
+** Notes:
+**
+** 1) The TDB date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TDB)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The matrix operates in the sense V(date) = rmatpn * V(J2000),
+** where the p-vector V(date) is with respect to the true equatorial
+** triad of date date1+date2 and the p-vector V(J2000) is with
+** respect to the mean equatorial triad of epoch J2000.0.
+**
+** Called:
+** iauPmat76 precession matrix, IAU 1976
+** iauNutm80 nutation matrix, IAU 1980
+** iauRxr product of two r-matrices
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992),
+** Section 3.3 (p145).
+**
+** This revision: 2010 January 23
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rmatp[3][3], rmatn[3][3];
+
+
+/* Precession matrix, J2000.0 to date. */
+ iauPmat76(date1, date2, rmatp);
+
+/* Nutation matrix. */
+ iauNutm80(date1, date2, rmatn);
+
+/* Combine the matrices: PN = N x P. */
+ iauRxr(rmatn, rmatp, rmatpn);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pom00.c b/sofa/pom00.c
new file mode 100644
index 0000000..33f7dc4
--- /dev/null
+++ b/sofa/pom00.c
@@ -0,0 +1,165 @@
+#include "sofam.h"
+
+void iauPom00(double xp, double yp, double sp, double rpom[3][3])
+/*
+** - - - - - - - - - -
+** i a u P o m 0 0
+** - - - - - - - - - -
+**
+** Form the matrix of polar motion for a given date, IAU 2000.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** xp,yp double coordinates of the pole (radians, Note 1)
+** sp double the TIO locator s' (radians, Note 2)
+**
+** Returned:
+** rpom double[3][3] polar-motion matrix (Note 3)
+**
+** Notes:
+**
+** 1) The arguments xp and yp are the coordinates (in radians) of the
+** Celestial Intermediate Pole with respect to the International
+** Terrestrial Reference System (see IERS Conventions 2003),
+** measured along the meridians to 0 and 90 deg west respectively.
+**
+** 2) The argument sp is the TIO locator s', in radians, which
+** positions the Terrestrial Intermediate Origin on the equator. It
+** is obtained from polar motion observations by numerical
+** integration, and so is in essence unpredictable. However, it is
+** dominated by a secular drift of about 47 microarcseconds per
+** century, and so can be taken into account by using s' = -47*t,
+** where t is centuries since J2000.0. The function iauSp00
+** implements this approximation.
+**
+** 3) The matrix operates in the sense V(TRS) = rpom * V(CIP), meaning
+** that it is the final rotation when computing the pointing
+** direction to a celestial source.
+**
+** Called:
+** iauIr initialize r-matrix to identity
+** iauRz rotate around Z-axis
+** iauRy rotate around Y-axis
+** iauRx rotate around X-axis
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+
+/* Construct the matrix. */
+ iauIr(rpom);
+ iauRz(sp, rpom);
+ iauRy(-xp, rpom);
+ iauRx(-yp, rpom);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/ppp.c b/sofa/ppp.c
new file mode 100644
index 0000000..b065f90
--- /dev/null
+++ b/sofa/ppp.c
@@ -0,0 +1,135 @@
+#include "sofam.h"
+
+void iauPpp(double a[3], double b[3], double apb[3])
+/*
+** - - - - - - -
+** i a u P p p
+** - - - - - - -
+**
+** P-vector addition.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double[3] first p-vector
+** b double[3] second p-vector
+**
+** Returned:
+** apb double[3] a + b
+**
+** Note:
+** It is permissible to re-use the same array for any of the
+** arguments.
+**
+** This revision: 2008 November 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ apb[0] = a[0] + b[0];
+ apb[1] = a[1] + b[1];
+ apb[2] = a[2] + b[2];
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/ppsp.c b/sofa/ppsp.c
new file mode 100644
index 0000000..80aa9b4
--- /dev/null
+++ b/sofa/ppsp.c
@@ -0,0 +1,144 @@
+#include "sofam.h"
+
+void iauPpsp(double a[3], double s, double b[3], double apsb[3])
+/*
+** - - - - - - - -
+** i a u P p s p
+** - - - - - - - -
+**
+** P-vector plus scaled p-vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double[3] first p-vector
+** s double scalar (multiplier for b)
+** b double[3] second p-vector
+**
+** Returned:
+** apsb double[3] a + s*b
+**
+** Note:
+** It is permissible for any of a, b and apsb to be the same array.
+**
+** Called:
+** iauSxp multiply p-vector by scalar
+** iauPpp p-vector plus p-vector
+**
+** This revision: 2008 November 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double sb[3];
+
+
+/* s*b. */
+ iauSxp(s, b, sb);
+
+/* a + s*b. */
+ iauPpp(a, sb, apsb);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pr00.c b/sofa/pr00.c
new file mode 100644
index 0000000..4a32a61
--- /dev/null
+++ b/sofa/pr00.c
@@ -0,0 +1,192 @@
+#include "sofam.h"
+
+void iauPr00(double date1, double date2, double *dpsipr, double *depspr)
+/*
+** - - - - - - - -
+** i a u P r 0 0
+** - - - - - - - -
+**
+** Precession-rate part of the IAU 2000 precession-nutation models
+** (part of MHB2000).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** dpsipr,depspr double precession corrections (Notes 2,3)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The precession adjustments are expressed as "nutation
+** components", corrections in longitude and obliquity with respect
+** to the J2000.0 equinox and ecliptic.
+**
+** 3) Although the precession adjustments are stated to be with respect
+** to Lieske et al. (1977), the MHB2000 model does not specify which
+** set of Euler angles are to be used and how the adjustments are to
+** be applied. The most literal and straightforward procedure is to
+** adopt the 4-rotation epsilon_0, psi_A, omega_A, xi_A option, and
+** to add dpsipr to psi_A and depspr to both omega_A and eps_A.
+**
+** 4) This is an implementation of one aspect of the IAU 2000A nutation
+** model, formally adopted by the IAU General Assembly in 2000,
+** namely MHB2000 (Mathews et al. 2002).
+**
+** References:
+**
+** Lieske, J.H., Lederle, T., Fricke, W. & Morando, B., "Expressions
+** for the precession quantities based upon the IAU (1976) System of
+** Astronomical Constants", Astron.Astrophys., 58, 1-16 (1977)
+**
+** Mathews, P.M., Herring, T.A., Buffet, B.A., "Modeling of nutation
+** and precession New nutation series for nonrigid Earth and
+** insights into the Earth's interior", J.Geophys.Res., 107, B4,
+** 2002. The MHB2000 code itself was obtained on 9th September 2002
+** from ftp://maia.usno.navy.mil/conv2000/chapter5/IAU2000A.
+**
+** Wallace, P.T., "Software for Implementing the IAU 2000
+** Resolutions", in IERS Workshop 5.1 (2002).
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t;
+
+/* Precession and obliquity corrections (radians per century) */
+ static const double PRECOR = -0.29965 * DAS2R,
+ OBLCOR = -0.02524 * DAS2R;
+
+
+/* Interval between fundamental epoch J2000.0 and given date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* Precession rate contributions with respect to IAU 1976/80. */
+ *dpsipr = PRECOR * t;
+ *depspr = OBLCOR * t;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/prec76.c b/sofa/prec76.c
new file mode 100644
index 0000000..c08700a
--- /dev/null
+++ b/sofa/prec76.c
@@ -0,0 +1,198 @@
+#include "sofam.h"
+
+void iauPrec76(double ep01, double ep02, double ep11, double ep12,
+ double *zeta, double *z, double *theta)
+/*
+** - - - - - - - - - -
+** i a u P r e c 7 6
+** - - - - - - - - - -
+**
+** IAU 1976 precession model.
+**
+** This function forms the three Euler angles which implement general
+** precession between two epochs, using the IAU 1976 model (as for
+** the FK5 catalog).
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** ep01,ep02 double TDB starting epoch (Note 1)
+** ep11,ep12 double TDB ending epoch (Note 1)
+**
+** Returned:
+** zeta double 1st rotation: radians cw around z
+** z double 3rd rotation: radians cw around z
+** theta double 2nd rotation: radians ccw around y
+**
+** Notes:
+**
+** 1) The epochs ep01+ep02 and ep11+ep12 are Julian Dates, apportioned
+** in any convenient way between the arguments epn1 and epn2. For
+** example, JD(TDB)=2450123.7 could be expressed in any of these
+** ways, among others:
+**
+** epn1 epn2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in cases
+** where the loss of several decimal digits of resolution is
+** acceptable. The J2000 method is best matched to the way the
+** argument is handled internally and will deliver the optimum
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+** The two epochs may be expressed using different methods, but at
+** the risk of losing some resolution.
+**
+** 2) The accumulated precession angles zeta, z, theta are expressed
+** through canonical polynomials which are valid only for a limited
+** time span. In addition, the IAU 1976 precession rate is known to
+** be imperfect. The absolute accuracy of the present formulation
+** is better than 0.1 arcsec from 1960AD to 2040AD, better than
+** 1 arcsec from 1640AD to 2360AD, and remains below 3 arcsec for
+** the whole of the period 500BC to 3000AD. The errors exceed
+** 10 arcsec outside the range 1200BC to 3900AD, exceed 100 arcsec
+** outside 4200BC to 5600AD and exceed 1000 arcsec outside 6800BC to
+** 8200AD.
+**
+** 3) The three angles are returned in the conventional order, which
+** is not the same as the order of the corresponding Euler
+** rotations. The precession matrix is
+** R_3(-z) x R_2(+theta) x R_3(-zeta).
+**
+** Reference:
+**
+** Lieske, J.H., 1979, Astron.Astrophys. 73, 282, equations
+** (6) & (7), p283.
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t0, t, tas2r, w;
+
+
+/* Interval between fundamental epoch J2000.0 and start epoch (JC). */
+ t0 = ((ep01 - DJ00) + ep02) / DJC;
+
+/* Interval over which precession required (JC). */
+ t = ((ep11 - ep01) + (ep12 - ep02)) / DJC;
+
+/* Euler angles. */
+ tas2r = t * DAS2R;
+ w = 2306.2181 + (1.39656 - 0.000139 * t0) * t0;
+
+ *zeta = (w + ((0.30188 - 0.000344 * t0) + 0.017998 * t) * t) * tas2r;
+
+ *z = (w + ((1.09468 + 0.000066 * t0) + 0.018203 * t) * t) * tas2r;
+
+ *theta = ((2004.3109 + (-0.85330 - 0.000217 * t0) * t0)
+ + ((-0.42665 - 0.000217 * t0) - 0.041833 * t) * t) * tas2r;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pv2p.c b/sofa/pv2p.c
new file mode 100644
index 0000000..dff3afc
--- /dev/null
+++ b/sofa/pv2p.c
@@ -0,0 +1,131 @@
+#include "sofam.h"
+
+void iauPv2p(double pv[2][3], double p[3])
+/*
+** - - - - - - - -
+** i a u P v 2 p
+** - - - - - - - -
+**
+** Discard velocity component of a pv-vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** pv double[2][3] pv-vector
+**
+** Returned:
+** p double[3] p-vector
+**
+** Called:
+** iauCp copy p-vector
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauCp(pv[0], p);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pv2s.c b/sofa/pv2s.c
new file mode 100644
index 0000000..1c52c03
--- /dev/null
+++ b/sofa/pv2s.c
@@ -0,0 +1,194 @@
+#include "sofam.h"
+
+void iauPv2s(double pv[2][3],
+ double *theta, double *phi, double *r,
+ double *td, double *pd, double *rd)
+/*
+** - - - - - - - -
+** i a u P v 2 s
+** - - - - - - - -
+**
+** Convert position/velocity from Cartesian to spherical coordinates.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** pv double[2][3] pv-vector
+**
+** Returned:
+** theta double longitude angle (radians)
+** phi double latitude angle (radians)
+** r double radial distance
+** td double rate of change of theta
+** pd double rate of change of phi
+** rd double rate of change of r
+**
+** Notes:
+**
+** 1) If the position part of pv is null, theta, phi, td and pd
+** are indeterminate. This is handled by extrapolating the
+** position through unit time by using the velocity part of
+** pv. This moves the origin without changing the direction
+** of the velocity component. If the position and velocity
+** components of pv are both null, zeroes are returned for all
+** six results.
+**
+** 2) If the position is a pole, theta, td and pd are indeterminate.
+** In such cases zeroes are returned for all three.
+**
+** This revision: 2008 October 28
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double x, y, z, xd, yd, zd, rxy2, rxy, r2, rtrue, rw, xyp;
+
+
+/* Components of position/velocity vector. */
+ x = pv[0][0];
+ y = pv[0][1];
+ z = pv[0][2];
+ xd = pv[1][0];
+ yd = pv[1][1];
+ zd = pv[1][2];
+
+/* Component of r in XY plane squared. */
+ rxy2 = x*x + y*y;
+
+/* Modulus squared. */
+ r2 = rxy2 + z*z;
+
+/* Modulus. */
+ rtrue = sqrt(r2);
+
+/* If null vector, move the origin along the direction of movement. */
+ rw = rtrue;
+ if (rtrue == 0.0) {
+ x = xd;
+ y = yd;
+ z = zd;
+ rxy2 = x*x + y*y;
+ r2 = rxy2 + z*z;
+ rw = sqrt(r2);
+ }
+
+/* Position and velocity in spherical coordinates. */
+ rxy = sqrt(rxy2);
+ xyp = x*xd + y*yd;
+ if (rxy2 != 0.0) {
+ *theta = atan2(y, x);
+ *phi = atan2(z, rxy);
+ *td = (x*yd - y*xd) / rxy2;
+ *pd = (zd*rxy2 - z*xyp) / (r2*rxy);
+ } else {
+ *theta = 0.0;
+ *phi = (z != 0.0) ? atan2(z, rxy) : 0.0;
+ *td = 0.0;
+ *pd = 0.0;
+ }
+ *r = rtrue;
+ *rd = (rw != 0.0) ? (xyp + z*zd) / rw : 0.0;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pvdpv.c b/sofa/pvdpv.c
new file mode 100644
index 0000000..dbe0b2e
--- /dev/null
+++ b/sofa/pvdpv.c
@@ -0,0 +1,152 @@
+#include "sofam.h"
+
+void iauPvdpv(double a[2][3], double b[2][3], double adb[2])
+/*
+** - - - - - - - - -
+** i a u P v d p v
+** - - - - - - - - -
+**
+** Inner (=scalar=dot) product of two pv-vectors.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double[2][3] first pv-vector
+** b double[2][3] second pv-vector
+**
+** Returned:
+** adb double[2] a . b (see note)
+**
+** Note:
+**
+** If the position and velocity components of the two pv-vectors are
+** ( ap, av ) and ( bp, bv ), the result, a . b, is the pair of
+** numbers ( ap . bp , ap . bv + av . bp ). The two numbers are the
+** dot-product of the two p-vectors and its derivative.
+**
+** Called:
+** iauPdp scalar product of two p-vectors
+**
+** This revision: 2008 May 22
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double adbd, addb;
+
+
+/* a . b = constant part of result. */
+ adb[0] = iauPdp(a[0], b[0]);
+
+/* a . bdot */
+ adbd = iauPdp(a[0], b[1]);
+
+/* adot . b */
+ addb = iauPdp(a[1], b[0]);
+
+/* Velocity part of result. */
+ adb[1] = adbd + addb;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pvm.c b/sofa/pvm.c
new file mode 100644
index 0000000..3561c87
--- /dev/null
+++ b/sofa/pvm.c
@@ -0,0 +1,136 @@
+#include "sofam.h"
+
+void iauPvm(double pv[2][3], double *r, double *s)
+/*
+** - - - - - - -
+** i a u P v m
+** - - - - - - -
+**
+** Modulus of pv-vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** pv double[2][3] pv-vector
+**
+** Returned:
+** r double modulus of position component
+** s double modulus of velocity component
+**
+** Called:
+** iauPm modulus of p-vector
+**
+** This revision: 2008 May 22
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Distance. */
+ *r = iauPm(pv[0]);
+
+/* Speed. */
+ *s = iauPm(pv[1]);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pvmpv.c b/sofa/pvmpv.c
new file mode 100644
index 0000000..740d54a
--- /dev/null
+++ b/sofa/pvmpv.c
@@ -0,0 +1,137 @@
+#include "sofam.h"
+
+void iauPvmpv(double a[2][3], double b[2][3], double amb[2][3])
+/*
+** - - - - - - - - -
+** i a u P v m p v
+** - - - - - - - - -
+**
+** Subtract one pv-vector from another.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double[2][3] first pv-vector
+** b double[2][3] second pv-vector
+**
+** Returned:
+** amb double[2][3] a - b
+**
+** Note:
+** It is permissible to re-use the same array for any of the
+** arguments.
+**
+** Called:
+** iauPmp p-vector minus p-vector
+**
+** This revision: 2008 November 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauPmp(a[0], b[0], amb[0]);
+ iauPmp(a[1], b[1], amb[1]);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pvppv.c b/sofa/pvppv.c
new file mode 100644
index 0000000..60d9a98
--- /dev/null
+++ b/sofa/pvppv.c
@@ -0,0 +1,137 @@
+#include "sofam.h"
+
+void iauPvppv(double a[2][3], double b[2][3], double apb[2][3])
+/*
+** - - - - - - - - -
+** i a u P v p p v
+** - - - - - - - - -
+**
+** Add one pv-vector to another.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double[2][3] first pv-vector
+** b double[2][3] second pv-vector
+**
+** Returned:
+** apb double[2][3] a + b
+**
+** Note:
+** It is permissible to re-use the same array for any of the
+** arguments.
+**
+** Called:
+** iauPpp p-vector plus p-vector
+**
+** This revision: 2008 November 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauPpp(a[0], b[0], apb[0]);
+ iauPpp(a[1], b[1], apb[1]);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pvstar.c b/sofa/pvstar.c
new file mode 100644
index 0000000..e804602
--- /dev/null
+++ b/sofa/pvstar.c
@@ -0,0 +1,257 @@
+#include "sofam.h"
+
+int iauPvstar(double pv[2][3], double *ra, double *dec,
+ double *pmr, double *pmd, double *px, double *rv)
+/*
+** - - - - - - - - - -
+** i a u P v s t a r
+** - - - - - - - - - -
+**
+** Convert star position+velocity vector to catalog coordinates.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given (Note 1):
+** pv double[2][3] pv-vector (AU, AU/day)
+**
+** Returned (Note 2):
+** ra double right ascension (radians)
+** dec double declination (radians)
+** pmr double RA proper motion (radians/year)
+** pmd double Dec proper motion (radians/year)
+** px double parallax (arcsec)
+** rv double radial velocity (km/s, positive = receding)
+**
+** Returned (function value):
+** int status:
+** 0 = OK
+** -1 = superluminal speed (Note 5)
+** -2 = null position vector
+**
+** Notes:
+**
+** 1) The specified pv-vector is the coordinate direction (and its rate
+** of change) for the date at which the light leaving the star
+** reached the solar-system barycenter.
+**
+** 2) The star data returned by this function are "observables" for an
+** imaginary observer at the solar-system barycenter. Proper motion
+** and radial velocity are, strictly, in terms of barycentric
+** coordinate time, TCB. For most practical applications, it is
+** permissible to neglect the distinction between TCB and ordinary
+** "proper" time on Earth (TT/TAI). The result will, as a rule, be
+** limited by the intrinsic accuracy of the proper-motion and
+** radial-velocity data; moreover, the supplied pv-vector is likely
+** to be merely an intermediate result (for example generated by the
+** function iauStarpv), so that a change of time unit will cancel
+** out overall.
+**
+** In accordance with normal star-catalog conventions, the object's
+** right ascension and declination are freed from the effects of
+** secular aberration. The frame, which is aligned to the catalog
+** equator and equinox, is Lorentzian and centered on the SSB.
+**
+** Summarizing, the specified pv-vector is for most stars almost
+** identical to the result of applying the standard geometrical
+** "space motion" transformation to the catalog data. The
+** differences, which are the subject of the Stumpff paper cited
+** below, are:
+**
+** (i) In stars with significant radial velocity and proper motion,
+** the constantly changing light-time distorts the apparent proper
+** motion. Note that this is a classical, not a relativistic,
+** effect.
+**
+** (ii) The transformation complies with special relativity.
+**
+** 3) Care is needed with units. The star coordinates are in radians
+** and the proper motions in radians per Julian year, but the
+** parallax is in arcseconds; the radial velocity is in km/s, but
+** the pv-vector result is in AU and AU/day.
+**
+** 4) The proper motions are the rate of change of the right ascension
+** and declination at the catalog epoch and are in radians per Julian
+** year. The RA proper motion is in terms of coordinate angle, not
+** true angle, and will thus be numerically larger at high
+** declinations.
+**
+** 5) Straight-line motion at constant speed in the inertial frame is
+** assumed. If the speed is greater than or equal to the speed of
+** light, the function aborts with an error status.
+**
+** 6) The inverse transformation is performed by the function iauStarpv.
+**
+** Called:
+** iauPn decompose p-vector into modulus and direction
+** iauPdp scalar product of two p-vectors
+** iauSxp multiply p-vector by scalar
+** iauPmp p-vector minus p-vector
+** iauPm modulus of p-vector
+** iauPpp p-vector plus p-vector
+** iauPv2s pv-vector to spherical
+** iauAnp normalize angle into range 0 to 2pi
+**
+** Reference:
+**
+** Stumpff, P., 1985, Astron.Astrophys. 144, 232-240.
+**
+** This revision: 2008 May 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double r, x[3], vr, ur[3], vt, ut[3], bett, betr, d, w, del,
+ usr[3], ust[3], a, rad, decd, rd;
+
+
+/* Isolate the radial component of the velocity (AU/day, inertial). */
+ iauPn(pv[0], &r, x);
+ vr = iauPdp(x, pv[1]);
+ iauSxp(vr, x, ur);
+
+/* Isolate the transverse component of the velocity (AU/day, inertial). */
+ iauPmp(pv[1], ur, ut);
+ vt = iauPm(ut);
+
+/* Special-relativity dimensionless parameters. */
+ bett = vt / DC;
+ betr = vr / DC;
+
+/* The inertial-to-observed correction terms. */
+ d = 1.0 + betr;
+ w = 1.0 - betr*betr - bett*bett;
+ if (d == 0.0 || w < 0) return -1;
+ del = sqrt(w) - 1.0;
+
+/* Apply relativistic correction factor to radial velocity component. */
+ w = (betr != 0) ? (betr - del) / (betr * d) : 1.0;
+ iauSxp(w, ur, usr);
+
+/* Apply relativistic correction factor to tangential velocity */
+/* component. */
+ iauSxp(1.0/d, ut, ust);
+
+/* Combine the two to obtain the observed velocity vector (AU/day). */
+ iauPpp(usr, ust, pv[1]);
+
+/* Cartesian to spherical. */
+ iauPv2s(pv, &a, dec, &r, &rad, &decd, &rd);
+ if (r == 0.0) return -2;
+
+/* Return RA in range 0 to 2pi. */
+ *ra = iauAnp(a);
+
+/* Return proper motions in radians per year. */
+ *pmr = rad * DJY;
+ *pmd = decd * DJY;
+
+/* Return parallax in arcsec. */
+ *px = DR2AS / r;
+
+/* Return radial velocity in km/s. */
+ *rv = 1e-3 * rd * DAU / DAYSEC;
+
+/* OK status. */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pvu.c b/sofa/pvu.c
new file mode 100644
index 0000000..d6f5811
--- /dev/null
+++ b/sofa/pvu.c
@@ -0,0 +1,143 @@
+#include "sofam.h"
+
+void iauPvu(double dt, double pv[2][3], double upv[2][3])
+/*
+** - - - - - - -
+** i a u P v u
+** - - - - - - -
+**
+** Update a pv-vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** dt double time interval
+** pv double[2][3] pv-vector
+**
+** Returned:
+** upv double[2][3] p updated, v unchanged
+**
+** Notes:
+**
+** 1) "Update" means "refer the position component of the vector
+** to a new date dt time units from the existing date".
+**
+** 2) The time units of dt must match those of the velocity.
+**
+** 3) It is permissible for pv and upv to be the same array.
+**
+** Called:
+** iauPpsp p-vector plus scaled p-vector
+** iauCp copy p-vector
+**
+** This revision: 2008 November 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauPpsp(pv[0], dt, pv[1], upv[0]);
+ iauCp(pv[1], upv[1]);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pvup.c b/sofa/pvup.c
new file mode 100644
index 0000000..e9b3137
--- /dev/null
+++ b/sofa/pvup.c
@@ -0,0 +1,138 @@
+#include "sofam.h"
+
+void iauPvup(double dt, double pv[2][3], double p[3])
+/*
+** - - - - - - - -
+** i a u P v u p
+** - - - - - - - -
+**
+** Update a pv-vector, discarding the velocity component.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** dt double time interval
+** pv double[2][3] pv-vector
+**
+** Returned:
+** p double[3] p-vector
+**
+** Notes:
+**
+** 1) "Update" means "refer the position component of the vector to a
+** new date dt time units from the existing date".
+**
+** 2) The time units of dt must match those of the velocity.
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ p[0] = pv[0][0] + dt * pv[1][0];
+ p[1] = pv[0][1] + dt * pv[1][1];
+ p[2] = pv[0][2] + dt * pv[1][2];
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pvxpv.c b/sofa/pvxpv.c
new file mode 100644
index 0000000..7b17208
--- /dev/null
+++ b/sofa/pvxpv.c
@@ -0,0 +1,157 @@
+#include "sofam.h"
+
+void iauPvxpv(double a[2][3], double b[2][3], double axb[2][3])
+/*
+** - - - - - - - - -
+** i a u P v x p v
+** - - - - - - - - -
+**
+** Outer (=vector=cross) product of two pv-vectors.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double[2][3] first pv-vector
+** b double[2][3] second pv-vector
+**
+** Returned:
+** axb double[2][3] a x b
+**
+** Notes:
+**
+** 1) If the position and velocity components of the two pv-vectors are
+** ( ap, av ) and ( bp, bv ), the result, a x b, is the pair of
+** vectors ( ap x bp, ap x bv + av x bp ). The two vectors are the
+** cross-product of the two p-vectors and its derivative.
+**
+** 2) It is permissible to re-use the same array for any of the
+** arguments.
+**
+** Called:
+** iauCpv copy pv-vector
+** iauPxp vector product of two p-vectors
+** iauPpp p-vector plus p-vector
+**
+** This revision: 2008 November 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double wa[2][3], wb[2][3], axbd[3], adxb[3];
+
+
+/* Make copies of the inputs. */
+ iauCpv(a, wa);
+ iauCpv(b, wb);
+
+/* a x b = position part of result. */
+ iauPxp(wa[0], wb[0], axb[0]);
+
+/* a x bdot + adot x b = velocity part of result. */
+ iauPxp(wa[0], wb[1], axbd);
+ iauPxp(wa[1], wb[0], adxb);
+ iauPpp(axbd, adxb, axb[1]);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/pxp.c b/sofa/pxp.c
new file mode 100644
index 0000000..b0a70b9
--- /dev/null
+++ b/sofa/pxp.c
@@ -0,0 +1,144 @@
+#include "sofam.h"
+
+void iauPxp(double a[3], double b[3], double axb[3])
+/*
+** - - - - - - -
+** i a u P x p
+** - - - - - - -
+**
+** p-vector outer (=vector=cross) product.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double[3] first p-vector
+** b double[3] second p-vector
+**
+** Returned:
+** axb double[3] a x b
+**
+** Note:
+** It is permissible to re-use the same array for any of the
+** arguments.
+**
+** This revision: 2008 November 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double xa, ya, za, xb, yb, zb;
+
+
+ xa = a[0];
+ ya = a[1];
+ za = a[2];
+ xb = b[0];
+ yb = b[1];
+ zb = b[2];
+ axb[0] = ya*zb - za*yb;
+ axb[1] = za*xb - xa*zb;
+ axb[2] = xa*yb - ya*xb;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/rm2v.c b/sofa/rm2v.c
new file mode 100644
index 0000000..839c5a1
--- /dev/null
+++ b/sofa/rm2v.c
@@ -0,0 +1,161 @@
+#include "sofam.h"
+
+void iauRm2v(double r[3][3], double w[3])
+/*
+** - - - - - - - -
+** i a u R m 2 v
+** - - - - - - - -
+**
+** Express an r-matrix as an r-vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** r double[3][3] rotation matrix
+**
+** Returned:
+** w double[3] rotation vector (Note 1)
+**
+** Notes:
+**
+** 1) A rotation matrix describes a rotation through some angle about
+** some arbitrary axis called the Euler axis. The "rotation vector"
+** returned by this function has the same direction as the Euler axis,
+** and its magnitude is the angle in radians. (The magnitude and
+** direction can be separated by means of the function iauPn.)
+**
+** 2) If r is null, so is the result. If r is not a rotation matrix
+** the result is undefined; r must be proper (i.e. have a positive
+** determinant) and real orthogonal (inverse = transpose).
+**
+** 3) The reference frame rotates clockwise as seen looking along
+** the rotation vector from the origin.
+**
+** This revision: 2010 August 27
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double x, y, z, s2, c2, phi, f;
+
+
+ x = r[1][2] - r[2][1];
+ y = r[2][0] - r[0][2];
+ z = r[0][1] - r[1][0];
+ s2 = sqrt(x*x + y*y + z*z);
+ if (s2 != 0) {
+ c2 = r[0][0] + r[1][1] + r[2][2] - 1.0;
+ phi = atan2(s2, c2);
+ f = phi / s2;
+ w[0] = x * f;
+ w[1] = y * f;
+ w[2] = z * f;
+ } else {
+ w[0] = 0.0;
+ w[1] = 0.0;
+ w[2] = 0.0;
+ }
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/rv2m.c b/sofa/rv2m.c
new file mode 100644
index 0000000..ae39fb7
--- /dev/null
+++ b/sofa/rv2m.c
@@ -0,0 +1,168 @@
+#include "sofam.h"
+
+void iauRv2m(double w[3], double r[3][3])
+/*
+** - - - - - - - -
+** i a u R v 2 m
+** - - - - - - - -
+**
+** Form the r-matrix corresponding to a given r-vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** w double[3] rotation vector (Note 1)
+**
+** Returned:
+** r double[3][3] rotation matrix
+**
+** Notes:
+**
+** 1) A rotation matrix describes a rotation through some angle about
+** some arbitrary axis called the Euler axis. The "rotation vector"
+** supplied to This function has the same direction as the Euler
+** axis, and its magnitude is the angle in radians.
+**
+** 2) If w is null, the unit matrix is returned.
+**
+** 3) The reference frame rotates clockwise as seen looking along the
+** rotation vector from the origin.
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double x, y, z, phi, s, c, f;
+
+
+/* Euler angle (magnitude of rotation vector) and functions. */
+ x = w[0];
+ y = w[1];
+ z = w[2];
+ phi = sqrt(x*x + y*y + z*z);
+ s = sin(phi);
+ c = cos(phi);
+ f = 1.0 - c;
+
+/* Euler axis (direction of rotation vector), perhaps null. */
+ if (phi != 0.0) {
+ x /= phi;
+ y /= phi;
+ z /= phi;
+ }
+
+/* Form the rotation matrix. */
+ r[0][0] = x*x*f + c;
+ r[0][1] = x*y*f + z*s;
+ r[0][2] = x*z*f - y*s;
+ r[1][0] = y*x*f - z*s;
+ r[1][1] = y*y*f + c;
+ r[1][2] = y*z*f + x*s;
+ r[2][0] = z*x*f + y*s;
+ r[2][1] = z*y*f - x*s;
+ r[2][2] = z*z*f + c;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/rx.c b/sofa/rx.c
new file mode 100644
index 0000000..b1b5a8d
--- /dev/null
+++ b/sofa/rx.c
@@ -0,0 +1,154 @@
+#include "sofam.h"
+
+void iauRx(double phi, double r[3][3])
+/*
+** - - - - - -
+** i a u R x
+** - - - - - -
+**
+** Rotate an r-matrix about the x-axis.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** phi double angle (radians)
+**
+** Given and returned:
+** r double[3][3] r-matrix
+**
+** Sign convention: The matrix can be used to rotate the reference
+** frame of a vector. Calling this function with positive phi
+** incorporates in the matrix an additional rotation, about the x-axis,
+** anticlockwise as seen looking towards the origin from positive x.
+**
+** Called:
+** iauIr initialize r-matrix to identity
+** iauRxr product of two r-matrices
+** iauCr copy r-matrix
+**
+** This revision: 2008 May 22
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double s, c, a[3][3], w[3][3];
+
+
+/* Matrix representing new rotation. */
+ s = sin(phi);
+ c = cos(phi);
+ iauIr(a);
+ a[1][1] = c;
+ a[2][1] = -s;
+ a[1][2] = s;
+ a[2][2] = c;
+
+/* Rotate. */
+ iauRxr(a, r, w);
+
+/* Return result. */
+ iauCr(w, r);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/rxp.c b/sofa/rxp.c
new file mode 100644
index 0000000..bb43c3c
--- /dev/null
+++ b/sofa/rxp.c
@@ -0,0 +1,149 @@
+#include "sofam.h"
+
+void iauRxp(double r[3][3], double p[3], double rp[3])
+/*
+** - - - - - - -
+** i a u R x p
+** - - - - - - -
+**
+** Multiply a p-vector by an r-matrix.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** r double[3][3] r-matrix
+** p double[3] p-vector
+**
+** Returned:
+** rp double[3] r * p
+**
+** Note:
+** It is permissible for p and rp to be the same array.
+**
+** Called:
+** iauCp copy p-vector
+**
+** This revision: 2008 October 28
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double w, wrp[3];
+ int i, j;
+
+
+/* Matrix r * vector p. */
+ for (j = 0; j < 3; j++) {
+ w = 0.0;
+ for (i = 0; i < 3; i++) {
+ w += r[j][i] * p[i];
+ }
+ wrp[j] = w;
+ }
+
+/* Return the result. */
+ iauCp(wrp, rp);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/rxpv.c b/sofa/rxpv.c
new file mode 100644
index 0000000..cae5664
--- /dev/null
+++ b/sofa/rxpv.c
@@ -0,0 +1,136 @@
+#include "sofam.h"
+
+void iauRxpv(double r[3][3], double pv[2][3], double rpv[2][3])
+/*
+** - - - - - - - -
+** i a u R x p v
+** - - - - - - - -
+**
+** Multiply a pv-vector by an r-matrix.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** r double[3][3] r-matrix
+** pv double[2][3] pv-vector
+**
+** Returned:
+** rpv double[2][3] r * pv
+**
+** Note:
+** It is permissible for pv and rpv to be the same array.
+**
+** Called:
+** iauRxp product of r-matrix and p-vector
+**
+** This revision: 2008 October 28
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauRxp(r, pv[0], rpv[0]);
+ iauRxp(r, pv[1], rpv[1]);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/rxr.c b/sofa/rxr.c
new file mode 100644
index 0000000..ba93540
--- /dev/null
+++ b/sofa/rxr.c
@@ -0,0 +1,149 @@
+#include "sofam.h"
+
+void iauRxr(double a[3][3], double b[3][3], double atb[3][3])
+/*
+** - - - - - - -
+** i a u R x r
+** - - - - - - -
+**
+** Multiply two r-matrices.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double[3][3] first r-matrix
+** b double[3][3] second r-matrix
+**
+** Returned:
+** atb double[3][3] a * b
+**
+** Note:
+** It is permissible to re-use the same array for any of the
+** arguments.
+**
+** Called:
+** iauCr copy r-matrix
+**
+** This revision: 2008 November 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int i, j, k;
+ double w, wm[3][3];
+
+
+ for (i = 0; i < 3; i++) {
+ for (j = 0; j < 3; j++) {
+ w = 0.0;
+ for (k = 0; k < 3; k++) {
+ w += a[i][k] * b[k][j];
+ }
+ wm[i][j] = w;
+ }
+ }
+ iauCr(wm, atb);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/ry.c b/sofa/ry.c
new file mode 100644
index 0000000..4d86cec
--- /dev/null
+++ b/sofa/ry.c
@@ -0,0 +1,154 @@
+#include "sofam.h"
+
+void iauRy(double theta, double r[3][3])
+/*
+** - - - - - -
+** i a u R y
+** - - - - - -
+**
+** Rotate an r-matrix about the y-axis.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** theta double angle (radians)
+**
+** Given and returned:
+** r double[3][3] r-matrix
+**
+** Sign convention: The matrix can be used to rotate the reference
+** frame of a vector. Calling This function with positive theta
+** incorporates in the matrix an additional rotation, about the y-axis,
+** anticlockwise as seen looking towards the origin from positive y.
+**
+** Called:
+** iauIr initialize r-matrix to identity
+** iauRxr product of two r-matrices
+** iauCr copy r-matrix
+**
+** This revision: 2008 May 22
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double s, c, a[3][3], w[3][3];
+
+
+/* Matrix representing new rotation. */
+ s = sin(theta);
+ c = cos(theta);
+ iauIr(a);
+ a[0][0] = c;
+ a[2][0] = s;
+ a[0][2] = -s;
+ a[2][2] = c;
+
+/* Rotate. */
+ iauRxr(a, r, w);
+
+/* Return result. */
+ iauCr(w, r);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/rz.c b/sofa/rz.c
new file mode 100644
index 0000000..cebbf5b
--- /dev/null
+++ b/sofa/rz.c
@@ -0,0 +1,154 @@
+#include "sofam.h"
+
+void iauRz(double psi, double r[3][3])
+/*
+** - - - - - -
+** i a u R z
+** - - - - - -
+**
+** Rotate an r-matrix about the z-axis.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** psi double angle (radians)
+**
+** Given and returned:
+** r double[3][3] r-matrix, rotated
+**
+** Sign convention: The matrix can be used to rotate the reference
+** frame of a vector. Calling This function with positive psi
+** incorporates in the matrix an additional rotation, about the z-axis,
+** anticlockwise as seen looking towards the origin from positive z.
+**
+** Called:
+** iauIr initialize r-matrix to identity
+** iauRxr product of two r-matrices
+** iauCr copy r-matrix
+**
+** This revision: 2008 May 22
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double s, c, a[3][3], w[3][3];
+
+
+/* Matrix representing new rotation. */
+ s = sin(psi);
+ c = cos(psi);
+ iauIr(a);
+ a[0][0] = c;
+ a[1][0] = -s;
+ a[0][1] = s;
+ a[1][1] = c;
+
+/* Rotate. */
+ iauRxr(a, r, w);
+
+/* Return result. */
+ iauCr(w, r);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/s00.c b/sofa/s00.c
new file mode 100644
index 0000000..47b7ad9
--- /dev/null
+++ b/sofa/s00.c
@@ -0,0 +1,421 @@
+#include "sofam.h"
+
+double iauS00(double date1, double date2, double x, double y)
+/*
+** - - - - - - -
+** i a u S 0 0
+** - - - - - - -
+**
+** The CIO locator s, positioning the Celestial Intermediate Origin on
+** the equator of the Celestial Intermediate Pole, given the CIP's X,Y
+** coordinates. Compatible with IAU 2000A precession-nutation.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+** x,y double CIP coordinates (Note 3)
+**
+** Returned (function value):
+** double the CIO locator s in radians (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The CIO locator s is the difference between the right ascensions
+** of the same point in two systems: the two systems are the GCRS
+** and the CIP,CIO, and the point is the ascending node of the
+** CIP equator. The quantity s remains below 0.1 arcsecond
+** throughout 1900-2100.
+**
+** 3) The series used to compute s is in fact for s+XY/2, where X and Y
+** are the x and y components of the CIP unit vector; this series
+** is more compact than a direct series for s would be. This
+** function requires X,Y to be supplied by the caller, who is
+** responsible for providing values that are consistent with the
+** supplied date.
+**
+** 4) The model is consistent with the IAU 2000A precession-nutation.
+**
+** Called:
+** iauFal03 mean anomaly of the Moon
+** iauFalp03 mean anomaly of the Sun
+** iauFaf03 mean argument of the latitude of the Moon
+** iauFad03 mean elongation of the Moon from the Sun
+** iauFaom03 mean longitude of the Moon's ascending node
+** iauFave03 mean longitude of Venus
+** iauFae03 mean longitude of Earth
+** iauFapa03 general accumulated precession in longitude
+**
+** References:
+**
+** Capitaine, N., Chapront, J., Lambert, S. and Wallace, P.,
+** "Expressions for the Celestial Intermediate Pole and Celestial
+** Ephemeris Origin consistent with the IAU 2000A precession-
+** nutation model", Astron.Astrophys. 400, 1145-1154 (2003)
+**
+** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
+** intermediate origin" (CIO) by IAU 2006 Resolution 2.
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2010 January 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Time since J2000.0, in Julian centuries */
+ double t;
+
+/* Miscellaneous */
+ int i, j;
+ double a, w0, w1, w2, w3, w4, w5;
+
+/* Fundamental arguments */
+ double fa[8];
+
+/* Returned value */
+ double s;
+
+/* --------------------- */
+/* The series for s+XY/2 */
+/* --------------------- */
+
+ typedef struct {
+ int nfa[8]; /* coefficients of l,l',F,D,Om,LVe,LE,pA */
+ double s, c; /* sine and cosine coefficients */
+ } TERM;
+
+/* Polynomial coefficients */
+ static const double sp[] = {
+
+ /* 1-6 */
+ 94.00e-6,
+ 3808.35e-6,
+ -119.94e-6,
+ -72574.09e-6,
+ 27.70e-6,
+ 15.61e-6
+ };
+
+/* Terms of order t^0 */
+ static const TERM s0[] = {
+
+ /* 1-10 */
+ {{ 0, 0, 0, 0, 1, 0, 0, 0}, -2640.73e-6, 0.39e-6 },
+ {{ 0, 0, 0, 0, 2, 0, 0, 0}, -63.53e-6, 0.02e-6 },
+ {{ 0, 0, 2, -2, 3, 0, 0, 0}, -11.75e-6, -0.01e-6 },
+ {{ 0, 0, 2, -2, 1, 0, 0, 0}, -11.21e-6, -0.01e-6 },
+ {{ 0, 0, 2, -2, 2, 0, 0, 0}, 4.57e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 3, 0, 0, 0}, -2.02e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 1, 0, 0, 0}, -1.98e-6, 0.00e-6 },
+ {{ 0, 0, 0, 0, 3, 0, 0, 0}, 1.72e-6, 0.00e-6 },
+ {{ 0, 1, 0, 0, 1, 0, 0, 0}, 1.41e-6, 0.01e-6 },
+ {{ 0, 1, 0, 0, -1, 0, 0, 0}, 1.26e-6, 0.01e-6 },
+
+ /* 11-20 */
+ {{ 1, 0, 0, 0, -1, 0, 0, 0}, 0.63e-6, 0.00e-6 },
+ {{ 1, 0, 0, 0, 1, 0, 0, 0}, 0.63e-6, 0.00e-6 },
+ {{ 0, 1, 2, -2, 3, 0, 0, 0}, -0.46e-6, 0.00e-6 },
+ {{ 0, 1, 2, -2, 1, 0, 0, 0}, -0.45e-6, 0.00e-6 },
+ {{ 0, 0, 4, -4, 4, 0, 0, 0}, -0.36e-6, 0.00e-6 },
+ {{ 0, 0, 1, -1, 1, -8, 12, 0}, 0.24e-6, 0.12e-6 },
+ {{ 0, 0, 2, 0, 0, 0, 0, 0}, -0.32e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 2, 0, 0, 0}, -0.28e-6, 0.00e-6 },
+ {{ 1, 0, 2, 0, 3, 0, 0, 0}, -0.27e-6, 0.00e-6 },
+ {{ 1, 0, 2, 0, 1, 0, 0, 0}, -0.26e-6, 0.00e-6 },
+
+ /* 21-30 */
+ {{ 0, 0, 2, -2, 0, 0, 0, 0}, 0.21e-6, 0.00e-6 },
+ {{ 0, 1, -2, 2, -3, 0, 0, 0}, -0.19e-6, 0.00e-6 },
+ {{ 0, 1, -2, 2, -1, 0, 0, 0}, -0.18e-6, 0.00e-6 },
+ {{ 0, 0, 0, 0, 0, 8,-13, -1}, 0.10e-6, -0.05e-6 },
+ {{ 0, 0, 0, 2, 0, 0, 0, 0}, -0.15e-6, 0.00e-6 },
+ {{ 2, 0, -2, 0, -1, 0, 0, 0}, 0.14e-6, 0.00e-6 },
+ {{ 0, 1, 2, -2, 2, 0, 0, 0}, 0.14e-6, 0.00e-6 },
+ {{ 1, 0, 0, -2, 1, 0, 0, 0}, -0.14e-6, 0.00e-6 },
+ {{ 1, 0, 0, -2, -1, 0, 0, 0}, -0.14e-6, 0.00e-6 },
+ {{ 0, 0, 4, -2, 4, 0, 0, 0}, -0.13e-6, 0.00e-6 },
+
+ /* 31-33 */
+ {{ 0, 0, 2, -2, 4, 0, 0, 0}, 0.11e-6, 0.00e-6 },
+ {{ 1, 0, -2, 0, -3, 0, 0, 0}, -0.11e-6, 0.00e-6 },
+ {{ 1, 0, -2, 0, -1, 0, 0, 0}, -0.11e-6, 0.00e-6 }
+ };
+
+/* Terms of order t^1 */
+ static const TERM s1[] ={
+
+ /* 1-3 */
+ {{ 0, 0, 0, 0, 2, 0, 0, 0}, -0.07e-6, 3.57e-6 },
+ {{ 0, 0, 0, 0, 1, 0, 0, 0}, 1.71e-6, -0.03e-6 },
+ {{ 0, 0, 2, -2, 3, 0, 0, 0}, 0.00e-6, 0.48e-6 }
+ };
+
+/* Terms of order t^2 */
+ static const TERM s2[] ={
+
+ /* 1-10 */
+ {{ 0, 0, 0, 0, 1, 0, 0, 0}, 743.53e-6, -0.17e-6 },
+ {{ 0, 0, 2, -2, 2, 0, 0, 0}, 56.91e-6, 0.06e-6 },
+ {{ 0, 0, 2, 0, 2, 0, 0, 0}, 9.84e-6, -0.01e-6 },
+ {{ 0, 0, 0, 0, 2, 0, 0, 0}, -8.85e-6, 0.01e-6 },
+ {{ 0, 1, 0, 0, 0, 0, 0, 0}, -6.38e-6, -0.05e-6 },
+ {{ 1, 0, 0, 0, 0, 0, 0, 0}, -3.07e-6, 0.00e-6 },
+ {{ 0, 1, 2, -2, 2, 0, 0, 0}, 2.23e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 1, 0, 0, 0}, 1.67e-6, 0.00e-6 },
+ {{ 1, 0, 2, 0, 2, 0, 0, 0}, 1.30e-6, 0.00e-6 },
+ {{ 0, 1, -2, 2, -2, 0, 0, 0}, 0.93e-6, 0.00e-6 },
+
+ /* 11-20 */
+ {{ 1, 0, 0, -2, 0, 0, 0, 0}, 0.68e-6, 0.00e-6 },
+ {{ 0, 0, 2, -2, 1, 0, 0, 0}, -0.55e-6, 0.00e-6 },
+ {{ 1, 0, -2, 0, -2, 0, 0, 0}, 0.53e-6, 0.00e-6 },
+ {{ 0, 0, 0, 2, 0, 0, 0, 0}, -0.27e-6, 0.00e-6 },
+ {{ 1, 0, 0, 0, 1, 0, 0, 0}, -0.27e-6, 0.00e-6 },
+ {{ 1, 0, -2, -2, -2, 0, 0, 0}, -0.26e-6, 0.00e-6 },
+ {{ 1, 0, 0, 0, -1, 0, 0, 0}, -0.25e-6, 0.00e-6 },
+ {{ 1, 0, 2, 0, 1, 0, 0, 0}, 0.22e-6, 0.00e-6 },
+ {{ 2, 0, 0, -2, 0, 0, 0, 0}, -0.21e-6, 0.00e-6 },
+ {{ 2, 0, -2, 0, -1, 0, 0, 0}, 0.20e-6, 0.00e-6 },
+
+ /* 21-25 */
+ {{ 0, 0, 2, 2, 2, 0, 0, 0}, 0.17e-6, 0.00e-6 },
+ {{ 2, 0, 2, 0, 2, 0, 0, 0}, 0.13e-6, 0.00e-6 },
+ {{ 2, 0, 0, 0, 0, 0, 0, 0}, -0.13e-6, 0.00e-6 },
+ {{ 1, 0, 2, -2, 2, 0, 0, 0}, -0.12e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 0, 0, 0, 0}, -0.11e-6, 0.00e-6 }
+ };
+
+/* Terms of order t^3 */
+ static const TERM s3[] ={
+
+ /* 1-4 */
+ {{ 0, 0, 0, 0, 1, 0, 0, 0}, 0.30e-6, -23.51e-6 },
+ {{ 0, 0, 2, -2, 2, 0, 0, 0}, -0.03e-6, -1.39e-6 },
+ {{ 0, 0, 2, 0, 2, 0, 0, 0}, -0.01e-6, -0.24e-6 },
+ {{ 0, 0, 0, 0, 2, 0, 0, 0}, 0.00e-6, 0.22e-6 }
+ };
+
+/* Terms of order t^4 */
+ static const TERM s4[] ={
+
+ /* 1-1 */
+ {{ 0, 0, 0, 0, 1, 0, 0, 0}, -0.26e-6, -0.01e-6 }
+ };
+
+/* Number of terms in the series */
+ const int NS0 = (int) (sizeof s0 / sizeof (TERM));
+ const int NS1 = (int) (sizeof s1 / sizeof (TERM));
+ const int NS2 = (int) (sizeof s2 / sizeof (TERM));
+ const int NS3 = (int) (sizeof s3 / sizeof (TERM));
+ const int NS4 = (int) (sizeof s4 / sizeof (TERM));
+
+/*--------------------------------------------------------------------*/
+
+/* Interval between fundamental epoch J2000.0 and current date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* Fundamental Arguments (from IERS Conventions 2003) */
+
+/* Mean anomaly of the Moon. */
+ fa[0] = iauFal03(t);
+
+/* Mean anomaly of the Sun. */
+ fa[1] = iauFalp03(t);
+
+/* Mean longitude of the Moon minus that of the ascending node. */
+ fa[2] = iauFaf03(t);
+
+/* Mean elongation of the Moon from the Sun. */
+ fa[3] = iauFad03(t);
+
+/* Mean longitude of the ascending node of the Moon. */
+ fa[4] = iauFaom03(t);
+
+/* Mean longitude of Venus. */
+ fa[5] = iauFave03(t);
+
+/* Mean longitude of Earth. */
+ fa[6] = iauFae03(t);
+
+/* General precession in longitude. */
+ fa[7] = iauFapa03(t);
+
+/* Evaluate s. */
+ w0 = sp[0];
+ w1 = sp[1];
+ w2 = sp[2];
+ w3 = sp[3];
+ w4 = sp[4];
+ w5 = sp[5];
+
+ for (i = NS0-1; i >= 0; i--) {
+ a = 0.0;
+ for (j = 0; j < 8; j++) {
+ a += (double)s0[i].nfa[j] * fa[j];
+ }
+ w0 += s0[i].s * sin(a) + s0[i].c * cos(a);
+ }
+
+ for (i = NS1-1; i >= 0; i--) {
+ a = 0.0;
+ for (j = 0; j < 8; j++) {
+ a += (double)s1[i].nfa[j] * fa[j];
+ }
+ w1 += s1[i].s * sin(a) + s1[i].c * cos(a);
+ }
+
+ for (i = NS2-1; i >= 0; i--) {
+ a = 0.0;
+ for (j = 0; j < 8; j++) {
+ a += (double)s2[i].nfa[j] * fa[j];
+ }
+ w2 += s2[i].s * sin(a) + s2[i].c * cos(a);
+ }
+
+ for (i = NS3-1; i >= 0; i--) {
+ a = 0.0;
+ for (j = 0; j < 8; j++) {
+ a += (double)s3[i].nfa[j] * fa[j];
+ }
+ w3 += s3[i].s * sin(a) + s3[i].c * cos(a);
+ }
+
+ for (i = NS4-1; i >= 0; i--) {
+ a = 0.0;
+ for (j = 0; j < 8; j++) {
+ a += (double)s4[i].nfa[j] * fa[j];
+ }
+ w4 += s4[i].s * sin(a) + s4[i].c * cos(a);
+ }
+
+ s = (w0 +
+ (w1 +
+ (w2 +
+ (w3 +
+ (w4 +
+ w5 * t) * t) * t) * t) * t) * DAS2R - x*y/2.0;
+
+ return s;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/s00a.c b/sofa/s00a.c
new file mode 100644
index 0000000..c4162c4
--- /dev/null
+++ b/sofa/s00a.c
@@ -0,0 +1,193 @@
+#include "sofam.h"
+
+double iauS00a(double date1, double date2)
+/*
+** - - - - - - - -
+** i a u S 0 0 a
+** - - - - - - - -
+**
+** The CIO locator s, positioning the Celestial Intermediate Origin on
+** the equator of the Celestial Intermediate Pole, using the IAU 2000A
+** precession-nutation model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned (function value):
+** double the CIO locator s in radians (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The CIO locator s is the difference between the right ascensions
+** of the same point in two systems. The two systems are the GCRS
+** and the CIP,CIO, and the point is the ascending node of the
+** CIP equator. The CIO locator s remains a small fraction of
+** 1 arcsecond throughout 1900-2100.
+**
+** 3) The series used to compute s is in fact for s+XY/2, where X and Y
+** are the x and y components of the CIP unit vector; this series
+** is more compact than a direct series for s would be. The present
+** function uses the full IAU 2000A nutation model when predicting
+** the CIP position. Faster results, with no significant loss of
+** accuracy, can be obtained via the function iauS00b, which uses
+** instead the IAU 2000B truncated model.
+**
+** Called:
+** iauPnm00a classical NPB matrix, IAU 2000A
+** iauBnp2xy extract CIP X,Y from the BPN matrix
+** iauS00 the CIO locator s, given X,Y, IAU 2000A
+**
+** References:
+**
+** Capitaine, N., Chapront, J., Lambert, S. and Wallace, P.,
+** "Expressions for the Celestial Intermediate Pole and Celestial
+** Ephemeris Origin consistent with the IAU 2000A precession-
+** nutation model", Astron.Astrophys. 400, 1145-1154 (2003)
+**
+** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
+** intermediate origin" (CIO) by IAU 2006 Resolution 2.
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2010 January 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rbpn[3][3], x, y, s;
+
+
+/* Bias-precession-nutation-matrix, IAU 2000A. */
+ iauPnm00a(date1, date2, rbpn);
+
+/* Extract the CIP coordinates. */
+ iauBpn2xy(rbpn, &x, &y);
+
+/* Compute the CIO locator s, given the CIP coordinates. */
+ s = iauS00(date1, date2, x, y);
+
+ return s;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/s00b.c b/sofa/s00b.c
new file mode 100644
index 0000000..8293b8f
--- /dev/null
+++ b/sofa/s00b.c
@@ -0,0 +1,193 @@
+#include "sofam.h"
+
+double iauS00b(double date1, double date2)
+/*
+** - - - - - - - -
+** i a u S 0 0 b
+** - - - - - - - -
+**
+** The CIO locator s, positioning the Celestial Intermediate Origin on
+** the equator of the Celestial Intermediate Pole, using the IAU 2000B
+** precession-nutation model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned (function value):
+** double the CIO locator s in radians (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The CIO locator s is the difference between the right ascensions
+** of the same point in two systems. The two systems are the GCRS
+** and the CIP,CIO, and the point is the ascending node of the
+** CIP equator. The CIO locator s remains a small fraction of
+** 1 arcsecond throughout 1900-2100.
+**
+** 3) The series used to compute s is in fact for s+XY/2, where X and Y
+** are the x and y components of the CIP unit vector; this series
+** is more compact than a direct series for s would be. The present
+** function uses the IAU 2000B truncated nutation model when
+** predicting the CIP position. The function iauS00a uses instead
+** the full IAU 2000A model, but with no significant increase in
+** accuracy and at some cost in speed.
+**
+** Called:
+** iauPnm00b classical NPB matrix, IAU 2000B
+** iauBnp2xy extract CIP X,Y from the BPN matrix
+** iauS00 the CIO locator s, given X,Y, IAU 2000A
+**
+** References:
+**
+** Capitaine, N., Chapront, J., Lambert, S. and Wallace, P.,
+** "Expressions for the Celestial Intermediate Pole and Celestial
+** Ephemeris Origin consistent with the IAU 2000A precession-
+** nutation model", Astron.Astrophys. 400, 1145-1154 (2003)
+**
+** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
+** intermediate origin" (CIO) by IAU 2006 Resolution 2.
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2010 January 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rbpn[3][3], x, y, s;
+
+
+/* Bias-precession-nutation-matrix, IAU 2000B. */
+ iauPnm00b(date1, date2, rbpn);
+
+/* Extract the CIP coordinates. */
+ iauBpn2xy(rbpn, &x, &y);
+
+/* Compute the CIO locator s, given the CIP coordinates. */
+ s = iauS00(date1, date2, x, y);
+
+ return s;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/s06.c b/sofa/s06.c
new file mode 100644
index 0000000..68d43d2
--- /dev/null
+++ b/sofa/s06.c
@@ -0,0 +1,418 @@
+#include "sofam.h"
+
+double iauS06(double date1, double date2, double x, double y)
+/*
+** - - - - - - -
+** i a u S 0 6
+** - - - - - - -
+**
+** The CIO locator s, positioning the Celestial Intermediate Origin on
+** the equator of the Celestial Intermediate Pole, given the CIP's X,Y
+** coordinates. Compatible with IAU 2006/2000A precession-nutation.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+** x,y double CIP coordinates (Note 3)
+**
+** Returned (function value):
+** double the CIO locator s in radians (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The CIO locator s is the difference between the right ascensions
+** of the same point in two systems: the two systems are the GCRS
+** and the CIP,CIO, and the point is the ascending node of the
+** CIP equator. The quantity s remains below 0.1 arcsecond
+** throughout 1900-2100.
+**
+** 3) The series used to compute s is in fact for s+XY/2, where X and Y
+** are the x and y components of the CIP unit vector; this series
+** is more compact than a direct series for s would be. This
+** function requires X,Y to be supplied by the caller, who is
+** responsible for providing values that are consistent with the
+** supplied date.
+**
+** 4) The model is consistent with the "P03" precession (Capitaine et
+** al. 2003), adopted by IAU 2006 Resolution 1, 2006, and the
+** IAU 2000A nutation (with P03 adjustments).
+**
+** Called:
+** iauFal03 mean anomaly of the Moon
+** iauFalp03 mean anomaly of the Sun
+** iauFaf03 mean argument of the latitude of the Moon
+** iauFad03 mean elongation of the Moon from the Sun
+** iauFaom03 mean longitude of the Moon's ascending node
+** iauFave03 mean longitude of Venus
+** iauFae03 mean longitude of Earth
+** iauFapa03 general accumulated precession in longitude
+**
+** References:
+**
+** Capitaine, N., Wallace, P.T. & Chapront, J., 2003, Astron.
+** Astrophys. 432, 355
+**
+** McCarthy, D.D., Petit, G. (eds.) 2004, IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG
+**
+** This revision: 2009 December 17
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Time since J2000.0, in Julian centuries */
+ double t;
+
+/* Miscellaneous */
+ int i, j;
+ double a, w0, w1, w2, w3, w4, w5;
+
+/* Fundamental arguments */
+ double fa[8];
+
+/* Returned value */
+ double s;
+
+/* --------------------- */
+/* The series for s+XY/2 */
+/* --------------------- */
+
+ typedef struct {
+ int nfa[8]; /* coefficients of l,l',F,D,Om,LVe,LE,pA */
+ double s, c; /* sine and cosine coefficients */
+ } TERM;
+
+/* Polynomial coefficients */
+ static const double sp[] = {
+
+ /* 1-6 */
+ 94.00e-6,
+ 3808.65e-6,
+ -122.68e-6,
+ -72574.11e-6,
+ 27.98e-6,
+ 15.62e-6
+ };
+
+/* Terms of order t^0 */
+ static const TERM s0[] = {
+
+ /* 1-10 */
+ {{ 0, 0, 0, 0, 1, 0, 0, 0}, -2640.73e-6, 0.39e-6 },
+ {{ 0, 0, 0, 0, 2, 0, 0, 0}, -63.53e-6, 0.02e-6 },
+ {{ 0, 0, 2, -2, 3, 0, 0, 0}, -11.75e-6, -0.01e-6 },
+ {{ 0, 0, 2, -2, 1, 0, 0, 0}, -11.21e-6, -0.01e-6 },
+ {{ 0, 0, 2, -2, 2, 0, 0, 0}, 4.57e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 3, 0, 0, 0}, -2.02e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 1, 0, 0, 0}, -1.98e-6, 0.00e-6 },
+ {{ 0, 0, 0, 0, 3, 0, 0, 0}, 1.72e-6, 0.00e-6 },
+ {{ 0, 1, 0, 0, 1, 0, 0, 0}, 1.41e-6, 0.01e-6 },
+ {{ 0, 1, 0, 0, -1, 0, 0, 0}, 1.26e-6, 0.01e-6 },
+
+ /* 11-20 */
+ {{ 1, 0, 0, 0, -1, 0, 0, 0}, 0.63e-6, 0.00e-6 },
+ {{ 1, 0, 0, 0, 1, 0, 0, 0}, 0.63e-6, 0.00e-6 },
+ {{ 0, 1, 2, -2, 3, 0, 0, 0}, -0.46e-6, 0.00e-6 },
+ {{ 0, 1, 2, -2, 1, 0, 0, 0}, -0.45e-6, 0.00e-6 },
+ {{ 0, 0, 4, -4, 4, 0, 0, 0}, -0.36e-6, 0.00e-6 },
+ {{ 0, 0, 1, -1, 1, -8, 12, 0}, 0.24e-6, 0.12e-6 },
+ {{ 0, 0, 2, 0, 0, 0, 0, 0}, -0.32e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 2, 0, 0, 0}, -0.28e-6, 0.00e-6 },
+ {{ 1, 0, 2, 0, 3, 0, 0, 0}, -0.27e-6, 0.00e-6 },
+ {{ 1, 0, 2, 0, 1, 0, 0, 0}, -0.26e-6, 0.00e-6 },
+
+ /* 21-30 */
+ {{ 0, 0, 2, -2, 0, 0, 0, 0}, 0.21e-6, 0.00e-6 },
+ {{ 0, 1, -2, 2, -3, 0, 0, 0}, -0.19e-6, 0.00e-6 },
+ {{ 0, 1, -2, 2, -1, 0, 0, 0}, -0.18e-6, 0.00e-6 },
+ {{ 0, 0, 0, 0, 0, 8,-13, -1}, 0.10e-6, -0.05e-6 },
+ {{ 0, 0, 0, 2, 0, 0, 0, 0}, -0.15e-6, 0.00e-6 },
+ {{ 2, 0, -2, 0, -1, 0, 0, 0}, 0.14e-6, 0.00e-6 },
+ {{ 0, 1, 2, -2, 2, 0, 0, 0}, 0.14e-6, 0.00e-6 },
+ {{ 1, 0, 0, -2, 1, 0, 0, 0}, -0.14e-6, 0.00e-6 },
+ {{ 1, 0, 0, -2, -1, 0, 0, 0}, -0.14e-6, 0.00e-6 },
+ {{ 0, 0, 4, -2, 4, 0, 0, 0}, -0.13e-6, 0.00e-6 },
+
+ /* 31-33 */
+ {{ 0, 0, 2, -2, 4, 0, 0, 0}, 0.11e-6, 0.00e-6 },
+ {{ 1, 0, -2, 0, -3, 0, 0, 0}, -0.11e-6, 0.00e-6 },
+ {{ 1, 0, -2, 0, -1, 0, 0, 0}, -0.11e-6, 0.00e-6 }
+ };
+
+/* Terms of order t^1 */
+ static const TERM s1[] = {
+
+ /* 1 - 3 */
+ {{ 0, 0, 0, 0, 2, 0, 0, 0}, -0.07e-6, 3.57e-6 },
+ {{ 0, 0, 0, 0, 1, 0, 0, 0}, 1.73e-6, -0.03e-6 },
+ {{ 0, 0, 2, -2, 3, 0, 0, 0}, 0.00e-6, 0.48e-6 }
+ };
+
+/* Terms of order t^2 */
+ static const TERM s2[] = {
+
+ /* 1-10 */
+ {{ 0, 0, 0, 0, 1, 0, 0, 0}, 743.52e-6, -0.17e-6 },
+ {{ 0, 0, 2, -2, 2, 0, 0, 0}, 56.91e-6, 0.06e-6 },
+ {{ 0, 0, 2, 0, 2, 0, 0, 0}, 9.84e-6, -0.01e-6 },
+ {{ 0, 0, 0, 0, 2, 0, 0, 0}, -8.85e-6, 0.01e-6 },
+ {{ 0, 1, 0, 0, 0, 0, 0, 0}, -6.38e-6, -0.05e-6 },
+ {{ 1, 0, 0, 0, 0, 0, 0, 0}, -3.07e-6, 0.00e-6 },
+ {{ 0, 1, 2, -2, 2, 0, 0, 0}, 2.23e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 1, 0, 0, 0}, 1.67e-6, 0.00e-6 },
+ {{ 1, 0, 2, 0, 2, 0, 0, 0}, 1.30e-6, 0.00e-6 },
+ {{ 0, 1, -2, 2, -2, 0, 0, 0}, 0.93e-6, 0.00e-6 },
+
+ /* 11-20 */
+ {{ 1, 0, 0, -2, 0, 0, 0, 0}, 0.68e-6, 0.00e-6 },
+ {{ 0, 0, 2, -2, 1, 0, 0, 0}, -0.55e-6, 0.00e-6 },
+ {{ 1, 0, -2, 0, -2, 0, 0, 0}, 0.53e-6, 0.00e-6 },
+ {{ 0, 0, 0, 2, 0, 0, 0, 0}, -0.27e-6, 0.00e-6 },
+ {{ 1, 0, 0, 0, 1, 0, 0, 0}, -0.27e-6, 0.00e-6 },
+ {{ 1, 0, -2, -2, -2, 0, 0, 0}, -0.26e-6, 0.00e-6 },
+ {{ 1, 0, 0, 0, -1, 0, 0, 0}, -0.25e-6, 0.00e-6 },
+ {{ 1, 0, 2, 0, 1, 0, 0, 0}, 0.22e-6, 0.00e-6 },
+ {{ 2, 0, 0, -2, 0, 0, 0, 0}, -0.21e-6, 0.00e-6 },
+ {{ 2, 0, -2, 0, -1, 0, 0, 0}, 0.20e-6, 0.00e-6 },
+
+ /* 21-25 */
+ {{ 0, 0, 2, 2, 2, 0, 0, 0}, 0.17e-6, 0.00e-6 },
+ {{ 2, 0, 2, 0, 2, 0, 0, 0}, 0.13e-6, 0.00e-6 },
+ {{ 2, 0, 0, 0, 0, 0, 0, 0}, -0.13e-6, 0.00e-6 },
+ {{ 1, 0, 2, -2, 2, 0, 0, 0}, -0.12e-6, 0.00e-6 },
+ {{ 0, 0, 2, 0, 0, 0, 0, 0}, -0.11e-6, 0.00e-6 }
+ };
+
+/* Terms of order t^3 */
+ static const TERM s3[] = {
+
+ /* 1-4 */
+ {{ 0, 0, 0, 0, 1, 0, 0, 0}, 0.30e-6, -23.42e-6 },
+ {{ 0, 0, 2, -2, 2, 0, 0, 0}, -0.03e-6, -1.46e-6 },
+ {{ 0, 0, 2, 0, 2, 0, 0, 0}, -0.01e-6, -0.25e-6 },
+ {{ 0, 0, 0, 0, 2, 0, 0, 0}, 0.00e-6, 0.23e-6 }
+ };
+
+/* Terms of order t^4 */
+ static const TERM s4[] = {
+
+ /* 1-1 */
+ {{ 0, 0, 0, 0, 1, 0, 0, 0}, -0.26e-6, -0.01e-6 }
+ };
+
+/* Number of terms in the series */
+ static const int NS0 = (int) (sizeof s0 / sizeof (TERM));
+ static const int NS1 = (int) (sizeof s1 / sizeof (TERM));
+ static const int NS2 = (int) (sizeof s2 / sizeof (TERM));
+ static const int NS3 = (int) (sizeof s3 / sizeof (TERM));
+ static const int NS4 = (int) (sizeof s4 / sizeof (TERM));
+
+/*--------------------------------------------------------------------*/
+
+/* Interval between fundamental epoch J2000.0 and current date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* Fundamental Arguments (from IERS Conventions 2003) */
+
+/* Mean anomaly of the Moon. */
+ fa[0] = iauFal03(t);
+
+/* Mean anomaly of the Sun. */
+ fa[1] = iauFalp03(t);
+
+/* Mean longitude of the Moon minus that of the ascending node. */
+ fa[2] = iauFaf03(t);
+
+/* Mean elongation of the Moon from the Sun. */
+ fa[3] = iauFad03(t);
+
+/* Mean longitude of the ascending node of the Moon. */
+ fa[4] = iauFaom03(t);
+
+/* Mean longitude of Venus. */
+ fa[5] = iauFave03(t);
+
+/* Mean longitude of Earth. */
+ fa[6] = iauFae03(t);
+
+/* General precession in longitude. */
+ fa[7] = iauFapa03(t);
+
+/* Evaluate s. */
+ w0 = sp[0];
+ w1 = sp[1];
+ w2 = sp[2];
+ w3 = sp[3];
+ w4 = sp[4];
+ w5 = sp[5];
+
+ for (i = NS0-1; i >= 0; i--) {
+ a = 0.0;
+ for (j = 0; j < 8; j++) {
+ a += (double)s0[i].nfa[j] * fa[j];
+ }
+ w0 += s0[i].s * sin(a) + s0[i].c * cos(a);
+ }
+
+ for (i = NS1-1; i >= 0; i--) {
+ a = 0.0;
+ for (j = 0; j < 8; j++) {
+ a += (double)s1[i].nfa[j] * fa[j];
+ }
+ w1 += s1[i].s * sin(a) + s1[i].c * cos(a);
+ }
+
+ for (i = NS2-1; i >= 0; i--) {
+ a = 0.0;
+ for (j = 0; j < 8; j++) {
+ a += (double)s2[i].nfa[j] * fa[j];
+ }
+ w2 += s2[i].s * sin(a) + s2[i].c * cos(a);
+ }
+
+ for (i = NS3-1; i >= 0; i--) {
+ a = 0.0;
+ for (j = 0; j < 8; j++) {
+ a += (double)s3[i].nfa[j] * fa[j];
+ }
+ w3 += s3[i].s * sin(a) + s3[i].c * cos(a);
+ }
+
+ for (i = NS4-1; i >= 0; i--) {
+ a = 0.0;
+ for (j = 0; j < 8; j++) {
+ a += (double)s4[i].nfa[j] * fa[j];
+ }
+ w4 += s4[i].s * sin(a) + s4[i].c * cos(a);
+ }
+
+ s = (w0 +
+ (w1 +
+ (w2 +
+ (w3 +
+ (w4 +
+ w5 * t) * t) * t) * t) * t) * DAS2R - x*y/2.0;
+
+ return s;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/s06a.c b/sofa/s06a.c
new file mode 100644
index 0000000..3b209bf
--- /dev/null
+++ b/sofa/s06a.c
@@ -0,0 +1,195 @@
+#include "sofam.h"
+
+double iauS06a(double date1, double date2)
+/*
+** - - - - - - - -
+** i a u S 0 6 a
+** - - - - - - - -
+**
+** The CIO locator s, positioning the Celestial Intermediate Origin on
+** the equator of the Celestial Intermediate Pole, using the IAU 2006
+** precession and IAU 2000A nutation models.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned (function value):
+** double the CIO locator s in radians (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The CIO locator s is the difference between the right ascensions
+** of the same point in two systems. The two systems are the GCRS
+** and the CIP,CIO, and the point is the ascending node of the
+** CIP equator. The CIO locator s remains a small fraction of
+** 1 arcsecond throughout 1900-2100.
+**
+** 3) The series used to compute s is in fact for s+XY/2, where X and Y
+** are the x and y components of the CIP unit vector; this series is
+** more compact than a direct series for s would be. The present
+** function uses the full IAU 2000A nutation model when predicting
+** the CIP position.
+**
+** Called:
+** iauPnm06a classical NPB matrix, IAU 2006/2000A
+** iauBpn2xy extract CIP X,Y coordinates from NPB matrix
+** iauS06 the CIO locator s, given X,Y, IAU 2006
+**
+** References:
+**
+** Capitaine, N., Chapront, J., Lambert, S. and Wallace, P.,
+** "Expressions for the Celestial Intermediate Pole and Celestial
+** Ephemeris Origin consistent with the IAU 2000A precession-
+** nutation model", Astron.Astrophys. 400, 1145-1154 (2003)
+**
+** n.b. The celestial ephemeris origin (CEO) was renamed "celestial
+** intermediate origin" (CIO) by IAU 2006 Resolution 2.
+**
+** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855
+**
+** McCarthy, D. D., Petit, G. (eds.), 2004, IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG
+**
+** Wallace, P.T. & Capitaine, N., 2006, Astron.Astrophys. 459, 981
+**
+** This revision: 2010 January 18
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rnpb[3][3], x, y, s;
+
+
+/* Bias-precession-nutation-matrix, IAU 20006/2000A. */
+ iauPnm06a(date1, date2, rnpb);
+
+/* Extract the CIP coordinates. */
+ iauBpn2xy(rnpb, &x, &y);
+
+/* Compute the CIO locator s, given the CIP coordinates. */
+ s = iauS06(date1, date2, x, y);
+
+ return s;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/s2c.c b/sofa/s2c.c
new file mode 100644
index 0000000..535756f
--- /dev/null
+++ b/sofa/s2c.c
@@ -0,0 +1,135 @@
+#include "sofam.h"
+
+void iauS2c(double theta, double phi, double c[3])
+/*
+** - - - - - - -
+** i a u S 2 c
+** - - - - - - -
+**
+** Convert spherical coordinates to Cartesian.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** theta double longitude angle (radians)
+** phi double latitude angle (radians)
+**
+** Returned:
+** c double[3] direction cosines
+**
+** This revision: 2008 October 28
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double cp;
+
+
+ cp = cos(phi);
+ c[0] = cos(theta) * cp;
+ c[1] = sin(theta) * cp;
+ c[2] = sin(phi);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/s2p.c b/sofa/s2p.c
new file mode 100644
index 0000000..0abb56c
--- /dev/null
+++ b/sofa/s2p.c
@@ -0,0 +1,138 @@
+#include "sofam.h"
+
+void iauS2p(double theta, double phi, double r, double p[3])
+/*
+** - - - - - - -
+** i a u S 2 p
+** - - - - - - -
+**
+** Convert spherical polar coordinates to p-vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** theta double longitude angle (radians)
+** phi double latitude angle (radians)
+** r double radial distance
+**
+** Returned:
+** p double[3] Cartesian coordinates
+**
+** Called:
+** iauS2c spherical coordinates to unit vector
+** iauSxp multiply p-vector by scalar
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double u[3];
+
+
+ iauS2c(theta, phi, u);
+ iauSxp(r, u, p);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/s2pv.c b/sofa/s2pv.c
new file mode 100644
index 0000000..2f20a04
--- /dev/null
+++ b/sofa/s2pv.c
@@ -0,0 +1,153 @@
+#include "sofam.h"
+
+void iauS2pv(double theta, double phi, double r,
+ double td, double pd, double rd,
+ double pv[2][3])
+/*
+** - - - - - - - -
+** i a u S 2 p v
+** - - - - - - - -
+**
+** Convert position/velocity from spherical to Cartesian coordinates.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** theta double longitude angle (radians)
+** phi double latitude angle (radians)
+** r double radial distance
+** td double rate of change of theta
+** pd double rate of change of phi
+** rd double rate of change of r
+**
+** Returned:
+** pv double[2][3] pv-vector
+**
+** This revision: 2008 May 25
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double st, ct, sp, cp, rcp, x, y, rpd, w;
+
+
+ st = sin(theta);
+ ct = cos(theta);
+ sp = sin(phi);
+ cp = cos(phi);
+ rcp = r * cp;
+ x = rcp * ct;
+ y = rcp * st;
+ rpd = r * pd;
+ w = rpd*sp - cp*rd;
+
+ pv[0][0] = x;
+ pv[0][1] = y;
+ pv[0][2] = r * sp;
+ pv[1][0] = -y*td - w*ct;
+ pv[1][1] = x*td - w*st;
+ pv[1][2] = rpd*cp + sp*rd;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/s2xpv.c b/sofa/s2xpv.c
new file mode 100644
index 0000000..a2577e5
--- /dev/null
+++ b/sofa/s2xpv.c
@@ -0,0 +1,137 @@
+#include "sofam.h"
+
+void iauS2xpv(double s1, double s2, double pv[2][3], double spv[2][3])
+/*
+** - - - - - - - - -
+** i a u S 2 x p v
+** - - - - - - - - -
+**
+** Multiply a pv-vector by two scalars.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** s1 double scalar to multiply position component by
+** s2 double scalar to multiply velocity component by
+** pv double[2][3] pv-vector
+**
+** Returned:
+** spv double[2][3] pv-vector: p scaled by s1, v scaled by s2
+**
+** Note:
+** It is permissible for pv and spv to be the same array.
+**
+** Called:
+** iauSxp multiply p-vector by scalar
+**
+** This revision: 2008 October 28
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauSxp(s1, pv[0], spv[0]);
+ iauSxp(s2, pv[1], spv[1]);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/sepp.c b/sofa/sepp.c
new file mode 100644
index 0000000..4bee435
--- /dev/null
+++ b/sofa/sepp.c
@@ -0,0 +1,155 @@
+#include "sofam.h"
+
+double iauSepp(double a[3], double b[3])
+/*
+** - - - - - - - -
+** i a u S e p p
+** - - - - - - - -
+**
+** Angular separation between two p-vectors.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** a double[3] first p-vector (not necessarily unit length)
+** b double[3] second p-vector (not necessarily unit length)
+**
+** Returned (function value):
+** double angular separation (radians, always positive)
+**
+** Notes:
+**
+** 1) If either vector is null, a zero result is returned.
+**
+** 2) The angular separation is most simply formulated in terms of
+** scalar product. However, this gives poor accuracy for angles
+** near zero and pi. The present algorithm uses both cross product
+** and dot product, to deliver full accuracy whatever the size of
+** the angle.
+**
+** Called:
+** iauPxp vector product of two p-vectors
+** iauPm modulus of p-vector
+** iauPdp scalar product of two p-vectors
+**
+** This revision: 2008 May 22
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double axb[3], ss, cs, s;
+
+
+/* Sine of angle between the vectors, multiplied by the two moduli. */
+ iauPxp(a, b, axb);
+ ss = iauPm(axb);
+
+/* Cosine of the angle, multiplied by the two moduli. */
+ cs = iauPdp(a, b);
+
+/* The angle. */
+ s = ((ss != 0.0) || (cs != 0.0)) ? atan2(ss, cs) : 0.0;
+
+ return s;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/seps.c b/sofa/seps.c
new file mode 100644
index 0000000..839e9f9
--- /dev/null
+++ b/sofa/seps.c
@@ -0,0 +1,143 @@
+#include "sofam.h"
+
+double iauSeps(double al, double ap, double bl, double bp)
+/*
+** - - - - - - - -
+** i a u S e p s
+** - - - - - - - -
+**
+** Angular separation between two sets of spherical coordinates.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** al double first longitude (radians)
+** ap double first latitude (radians)
+** bl double second longitude (radians)
+** bp double second latitude (radians)
+**
+** Returned (function value):
+** double angular separation (radians)
+**
+** Called:
+** iauS2c spherical coordinates to unit vector
+** iauSepp angular separation between two p-vectors
+**
+** This revision: 2008 May 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double ac[3], bc[3], s;
+
+
+/* Spherical to Cartesian. */
+ iauS2c(al, ap, ac);
+ iauS2c(bl, bp, bc);
+
+/* Angle between the vectors. */
+ s = iauSepp(ac, bc);
+
+ return s;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/sofa.h b/sofa/sofa.h
new file mode 100644
index 0000000..43e08dc
--- /dev/null
+++ b/sofa/sofa.h
@@ -0,0 +1,429 @@
+#ifndef SOFAHDEF
+#define SOFAHDEF
+
+/*
+** - - - - - - -
+** s o f a . h
+** - - - - - - -
+**
+** Prototype function declarations for SOFA library.
+**
+** This file is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** This revision: 2012 February 23
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+
+#include "math.h"
+
+#ifdef __cplusplus
+extern "C" {
+#endif
+
+/* Astronomy/Calendars */
+int iauCal2jd(int iy, int im, int id, double *djm0, double *djm);
+double iauEpb(double dj1, double dj2);
+void iauEpb2jd(double epb, double *djm0, double *djm);
+double iauEpj(double dj1, double dj2);
+void iauEpj2jd(double epj, double *djm0, double *djm);
+int iauJd2cal(double dj1, double dj2,
+ int *iy, int *im, int *id, double *fd);
+int iauJdcalf(int ndp, double dj1, double dj2, int iymdf[4]);
+
+/* Astronomy/Ephemerides */
+int iauEpv00(double date1, double date2,
+ double pvh[2][3], double pvb[2][3]);
+int iauPlan94(double date1, double date2, int np, double pv[2][3]);
+
+/* Astronomy/FundamentalArgs */
+double iauFad03(double t);
+double iauFae03(double t);
+double iauFaf03(double t);
+double iauFaju03(double t);
+double iauFal03(double t);
+double iauFalp03(double t);
+double iauFama03(double t);
+double iauFame03(double t);
+double iauFane03(double t);
+double iauFaom03(double t);
+double iauFapa03(double t);
+double iauFasa03(double t);
+double iauFaur03(double t);
+double iauFave03(double t);
+
+/* Astronomy/PrecNutPolar */
+void iauBi00(double *dpsibi, double *depsbi, double *dra);
+void iauBp00(double date1, double date2,
+ double rb[3][3], double rp[3][3], double rbp[3][3]);
+void iauBp06(double date1, double date2,
+ double rb[3][3], double rp[3][3], double rbp[3][3]);
+void iauBpn2xy(double rbpn[3][3], double *x, double *y);
+void iauC2i00a(double date1, double date2, double rc2i[3][3]);
+void iauC2i00b(double date1, double date2, double rc2i[3][3]);
+void iauC2i06a(double date1, double date2, double rc2i[3][3]);
+void iauC2ibpn(double date1, double date2, double rbpn[3][3],
+ double rc2i[3][3]);
+void iauC2ixy(double date1, double date2, double x, double y,
+ double rc2i[3][3]);
+void iauC2ixys(double x, double y, double s, double rc2i[3][3]);
+void iauC2t00a(double tta, double ttb, double uta, double utb,
+ double xp, double yp, double rc2t[3][3]);
+void iauC2t00b(double tta, double ttb, double uta, double utb,
+ double xp, double yp, double rc2t[3][3]);
+void iauC2t06a(double tta, double ttb, double uta, double utb,
+ double xp, double yp, double rc2t[3][3]);
+void iauC2tcio(double rc2i[3][3], double era, double rpom[3][3],
+ double rc2t[3][3]);
+void iauC2teqx(double rbpn[3][3], double gst, double rpom[3][3],
+ double rc2t[3][3]);
+void iauC2tpe(double tta, double ttb, double uta, double utb,
+ double dpsi, double deps, double xp, double yp,
+ double rc2t[3][3]);
+void iauC2txy(double tta, double ttb, double uta, double utb,
+ double x, double y, double xp, double yp,
+ double rc2t[3][3]);
+double iauEo06a(double date1, double date2);
+double iauEors(double rnpb[3][3], double s);
+void iauFw2m(double gamb, double phib, double psi, double eps,
+ double r[3][3]);
+void iauFw2xy(double gamb, double phib, double psi, double eps,
+ double *x, double *y);
+void iauNum00a(double date1, double date2, double rmatn[3][3]);
+void iauNum00b(double date1, double date2, double rmatn[3][3]);
+void iauNum06a(double date1, double date2, double rmatn[3][3]);
+void iauNumat(double epsa, double dpsi, double deps, double rmatn[3][3]);
+void iauNut00a(double date1, double date2, double *dpsi, double *deps);
+void iauNut00b(double date1, double date2, double *dpsi, double *deps);
+void iauNut06a(double date1, double date2, double *dpsi, double *deps);
+void iauNut80(double date1, double date2, double *dpsi, double *deps);
+void iauNutm80(double date1, double date2, double rmatn[3][3]);
+double iauObl06(double date1, double date2);
+double iauObl80(double date1, double date2);
+void iauP06e(double date1, double date2,
+ double *eps0, double *psia, double *oma, double *bpa,
+ double *bqa, double *pia, double *bpia,
+ double *epsa, double *chia, double *za, double *zetaa,
+ double *thetaa, double *pa,
+ double *gam, double *phi, double *psi);
+void iauPb06(double date1, double date2,
+ double *bzeta, double *bz, double *btheta);
+void iauPfw06(double date1, double date2,
+ double *gamb, double *phib, double *psib, double *epsa);
+void iauPmat00(double date1, double date2, double rbp[3][3]);
+void iauPmat06(double date1, double date2, double rbp[3][3]);
+void iauPmat76(double date1, double date2, double rmatp[3][3]);
+void iauPn00(double date1, double date2, double dpsi, double deps,
+ double *epsa,
+ double rb[3][3], double rp[3][3], double rbp[3][3],
+ double rn[3][3], double rbpn[3][3]);
+void iauPn00a(double date1, double date2,
+ double *dpsi, double *deps, double *epsa,
+ double rb[3][3], double rp[3][3], double rbp[3][3],
+ double rn[3][3], double rbpn[3][3]);
+void iauPn00b(double date1, double date2,
+ double *dpsi, double *deps, double *epsa,
+ double rb[3][3], double rp[3][3], double rbp[3][3],
+ double rn[3][3], double rbpn[3][3]);
+void iauPn06(double date1, double date2, double dpsi, double deps,
+ double *epsa,
+ double rb[3][3], double rp[3][3], double rbp[3][3],
+ double rn[3][3], double rbpn[3][3]);
+void iauPn06a(double date1, double date2,
+ double *dpsi, double *deps, double *epsa,
+ double rb[3][3], double rp[3][3], double rbp[3][3],
+ double rn[3][3], double rbpn[3][3]);
+void iauPnm00a(double date1, double date2, double rbpn[3][3]);
+void iauPnm00b(double date1, double date2, double rbpn[3][3]);
+void iauPnm06a(double date1, double date2, double rnpb[3][3]);
+void iauPnm80(double date1, double date2, double rmatpn[3][3]);
+void iauPom00(double xp, double yp, double sp, double rpom[3][3]);
+void iauPr00(double date1, double date2, double *dpsipr, double *depspr);
+void iauPrec76(double ep01, double ep02, double ep11, double ep12,
+ double *zeta, double *z, double *theta);
+double iauS00(double date1, double date2, double x, double y);
+double iauS00a(double date1, double date2);
+double iauS00b(double date1, double date2);
+double iauS06(double date1, double date2, double x, double y);
+double iauS06a(double date1, double date2);
+double iauSp00(double date1, double date2);
+void iauXy06(double date1, double date2, double *x, double *y);
+void iauXys00a(double date1, double date2,
+ double *x, double *y, double *s);
+void iauXys00b(double date1, double date2,
+ double *x, double *y, double *s);
+void iauXys06a(double date1, double date2,
+ double *x, double *y, double *s);
+
+/* Astronomy/RotationAndTime */
+double iauEe00(double date1, double date2, double epsa, double dpsi);
+double iauEe00a(double date1, double date2);
+double iauEe00b(double date1, double date2);
+double iauEe06a(double date1, double date2);
+double iauEect00(double date1, double date2);
+double iauEqeq94(double date1, double date2);
+double iauEra00(double dj1, double dj2);
+double iauGmst00(double uta, double utb, double tta, double ttb);
+double iauGmst06(double uta, double utb, double tta, double ttb);
+double iauGmst82(double dj1, double dj2);
+double iauGst00a(double uta, double utb, double tta, double ttb);
+double iauGst00b(double uta, double utb);
+double iauGst06(double uta, double utb, double tta, double ttb,
+ double rnpb[3][3]);
+double iauGst06a(double uta, double utb, double tta, double ttb);
+double iauGst94(double uta, double utb);
+
+/* Astronomy/SpaceMotion */
+int iauPvstar(double pv[2][3], double *ra, double *dec,
+ double *pmr, double *pmd, double *px, double *rv);
+int iauStarpv(double ra, double dec,
+ double pmr, double pmd, double px, double rv,
+ double pv[2][3]);
+
+/* Astronomy/StarCatalogs */
+void iauFk52h(double r5, double d5,
+ double dr5, double dd5, double px5, double rv5,
+ double *rh, double *dh,
+ double *drh, double *ddh, double *pxh, double *rvh);
+void iauFk5hip(double r5h[3][3], double s5h[3]);
+void iauFk5hz(double r5, double d5, double date1, double date2,
+ double *rh, double *dh);
+void iauH2fk5(double rh, double dh,
+ double drh, double ddh, double pxh, double rvh,
+ double *r5, double *d5,
+ double *dr5, double *dd5, double *px5, double *rv5);
+void iauHfk5z(double rh, double dh, double date1, double date2,
+ double *r5, double *d5, double *dr5, double *dd5);
+int iauStarpm(double ra1, double dec1,
+ double pmr1, double pmd1, double px1, double rv1,
+ double ep1a, double ep1b, double ep2a, double ep2b,
+ double *ra2, double *dec2,
+ double *pmr2, double *pmd2, double *px2, double *rv2);
+
+/* Astronomy/Geodetic/Geocentric */
+int iauEform(int n, double *a, double *f);
+int iauGc2gd(int n, double xyz[3],
+ double *elong, double *phi, double *height);
+int iauGc2gde(double a, double f, double xyz[3],
+ double *elong, double *phi, double *height);
+int iauGd2gc(int n, double elong, double phi, double height,
+ double xyz[3]);
+int iauGd2gce(double a, double f,
+ double elong, double phi, double height, double xyz[3]);
+
+/* Astronomy/Timescales */
+int iauD2dtf(const char *scale, int ndp, double d1, double d2,
+ int *iy, int *im, int *id, int ihmsf[4]);
+int iauDat(int iy, int im, int id, double fd, double *deltat);
+double iauDtdb(double date1, double date2,
+ double ut, double elong, double u, double v);
+int iauDtf2d(const char *scale, int iy, int im, int id,
+ int ihr, int imn, double sec, double *d1, double *d2);
+int iauTaitt(double tai1, double tai2, double *tt1, double *tt2);
+int iauTaiut1(double tai1, double tai2, double dta,
+ double *ut11, double *ut12);
+int iauTaiutc(double tai1, double tai2, double *utc1, double *utc2);
+int iauTcbtdb(double tcb1, double tcb2, double *tdb1, double *tdb2);
+int iauTcgtt(double tcg1, double tcg2, double *tt1, double *tt2);
+int iauTdbtcb(double tdb1, double tdb2, double *tcb1, double *tcb2);
+int iauTdbtt(double tdb1, double tdb2, double dtr,
+ double *tt1, double *tt2);
+int iauTttai(double tt1, double tt2, double *tai1, double *tai2);
+int iauTttcg(double tt1, double tt2, double *tcg1, double *tcg2);
+int iauTttdb(double tt1, double tt2, double dtr,
+ double *tdb1, double *tdb2);
+int iauTtut1(double tt1, double tt2, double dt,
+ double *ut11, double *ut12);
+int iauUt1tai(double ut11, double ut12, double dta,
+ double *tai1, double *tai2);
+int iauUt1tt(double ut11, double ut12, double dt,
+ double *tt1, double *tt2);
+int iauUt1utc(double ut11, double ut12, double dut1,
+ double *utc1, double *utc2);
+int iauUtctai(double utc1, double utc2, double *tai1, double *tai2);
+int iauUtcut1(double utc1, double utc2, double dut1,
+ double *ut11, double *ut12);
+
+/* VectorMatrix/AngleOps */
+void iauA2af(int ndp, double angle, char *sign, int idmsf[4]);
+void iauA2tf(int ndp, double angle, char *sign, int ihmsf[4]);
+int iauAf2a(char s, int ideg, int iamin, double asec, double *rad);
+double iauAnp(double a);
+double iauAnpm(double a);
+void iauD2tf(int ndp, double days, char *sign, int ihmsf[4]);
+int iauTf2a(char s, int ihour, int imin, double sec, double *rad);
+int iauTf2d(char s, int ihour, int imin, double sec, double *days);
+
+/* VectorMatrix/BuildRotations */
+void iauRx(double phi, double r[3][3]);
+void iauRy(double theta, double r[3][3]);
+void iauRz(double psi, double r[3][3]);
+
+/* VectorMatrix/CopyExtendExtract */
+void iauCp(double p[3], double c[3]);
+void iauCpv(double pv[2][3], double c[2][3]);
+void iauCr(double r[3][3], double c[3][3]);
+void iauP2pv(double p[3], double pv[2][3]);
+void iauPv2p(double pv[2][3], double p[3]);
+
+/* VectorMatrix/Initialization */
+void iauIr(double r[3][3]);
+void iauZp(double p[3]);
+void iauZpv(double pv[2][3]);
+void iauZr(double r[3][3]);
+
+/* VectorMatrix/MatrixOps */
+void iauRxr(double a[3][3], double b[3][3], double atb[3][3]);
+void iauTr(double r[3][3], double rt[3][3]);
+
+/* VectorMatrix/MatrixVectorProducts */
+void iauRxp(double r[3][3], double p[3], double rp[3]);
+void iauRxpv(double r[3][3], double pv[2][3], double rpv[2][3]);
+void iauTrxp(double r[3][3], double p[3], double trp[3]);
+void iauTrxpv(double r[3][3], double pv[2][3], double trpv[2][3]);
+
+/* VectorMatrix/RotationVectors */
+void iauRm2v(double r[3][3], double w[3]);
+void iauRv2m(double w[3], double r[3][3]);
+
+/* VectorMatrix/SeparationAndAngle */
+double iauPap(double a[3], double b[3]);
+double iauPas(double al, double ap, double bl, double bp);
+double iauSepp(double a[3], double b[3]);
+double iauSeps(double al, double ap, double bl, double bp);
+
+/* VectorMatrix/SphericalCartesian */
+void iauC2s(double p[3], double *theta, double *phi);
+void iauP2s(double p[3], double *theta, double *phi, double *r);
+void iauPv2s(double pv[2][3],
+ double *theta, double *phi, double *r,
+ double *td, double *pd, double *rd);
+void iauS2c(double theta, double phi, double c[3]);
+void iauS2p(double theta, double phi, double r, double p[3]);
+void iauS2pv(double theta, double phi, double r,
+ double td, double pd, double rd,
+ double pv[2][3]);
+
+/* VectorMatrix/VectorOps */
+double iauPdp(double a[3], double b[3]);
+double iauPm(double p[3]);
+void iauPmp(double a[3], double b[3], double amb[3]);
+void iauPn(double p[3], double *r, double u[3]);
+void iauPpp(double a[3], double b[3], double apb[3]);
+void iauPpsp(double a[3], double s, double b[3], double apsb[3]);
+void iauPvdpv(double a[2][3], double b[2][3], double adb[2]);
+void iauPvm(double pv[2][3], double *r, double *s);
+void iauPvmpv(double a[2][3], double b[2][3], double amb[2][3]);
+void iauPvppv(double a[2][3], double b[2][3], double apb[2][3]);
+void iauPvu(double dt, double pv[2][3], double upv[2][3]);
+void iauPvup(double dt, double pv[2][3], double p[3]);
+void iauPvxpv(double a[2][3], double b[2][3], double axb[2][3]);
+void iauPxp(double a[3], double b[3], double axb[3]);
+void iauS2xpv(double s1, double s2, double pv[2][3], double spv[2][3]);
+void iauSxp(double s, double p[3], double sp[3]);
+void iauSxpv(double s, double pv[2][3], double spv[2][3]);
+
+#ifdef __cplusplus
+}
+#endif
+
+#endif
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
diff --git a/sofa/sofam.h b/sofa/sofam.h
new file mode 100644
index 0000000..a6fce72
--- /dev/null
+++ b/sofa/sofam.h
@@ -0,0 +1,205 @@
+#ifndef SOFAMHDEF
+#define SOFAMHDEF
+
+/*
+** - - - - - - - -
+** s o f a m . h
+** - - - - - - - -
+**
+** Macros used by SOFA library.
+**
+** This file is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Please note that the constants defined below are to be used only in
+** the context of the SOFA software, and have no other official IAU
+** status.
+**
+** This revision: 2012 February 23
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+
+#include "sofa.h"
+
+
+/* Pi */
+#define DPI (3.141592653589793238462643)
+
+/* 2Pi */
+#define D2PI (6.283185307179586476925287)
+
+/* Degrees to radians */
+#define DD2R (1.745329251994329576923691e-2)
+
+/* Radians to arcseconds */
+#define DR2AS (206264.8062470963551564734)
+
+/* Arcseconds to radians */
+#define DAS2R (4.848136811095359935899141e-6)
+
+/* Seconds of time to radians */
+#define DS2R (7.272205216643039903848712e-5)
+
+/* Arcseconds in a full circle */
+#define TURNAS (1296000.0)
+
+/* Milliarcseconds to radians */
+#define DMAS2R (DAS2R / 1e3)
+
+/* Length of tropical year B1900 (days) */
+#define DTY (365.242198781)
+
+/* Seconds per day. */
+#define DAYSEC (86400.0)
+
+/* Days per Julian year */
+#define DJY (365.25)
+
+/* Days per Julian century */
+#define DJC (36525.0)
+
+/* Days per Julian millennium */
+#define DJM (365250.0)
+
+/* Reference epoch (J2000.0), Julian Date */
+#define DJ00 (2451545.0)
+
+/* Julian Date of Modified Julian Date zero */
+#define DJM0 (2400000.5)
+
+/* Reference epoch (J2000.0), Modified Julian Date */
+#define DJM00 (51544.5)
+
+/* 1977 Jan 1.0 as MJD */
+#define DJM77 (43144.0)
+
+/* TT minus TAI (s) */
+#define TTMTAI (32.184)
+
+/* AU (m) */
+#define DAU (149597870e3)
+
+/* Speed of light (AU per day) */
+#define DC (DAYSEC / 499.004782)
+
+/* L_G = 1 - d(TT)/d(TCG) */
+#define ELG (6.969290134e-10)
+
+/* L_B = 1 - d(TDB)/d(TCB), and TDB (s) at TAI 1977/1/1.0 */
+#define ELB (1.550519768e-8)
+#define TDB0 (-6.55e-5)
+
+/* dint(A) - truncate to nearest whole number towards zero (double) */
+#define dint(A) ((A)<0.0?ceil(A):floor(A))
+
+/* dnint(A) - round to nearest whole number (double) */
+#define dnint(A) ((A)<0.0?ceil((A)-0.5):floor((A)+0.5))
+
+/* dsign(A,B) - magnitude of A with sign of B (double) */
+#define dsign(A,B) ((B)<0.0?-fabs(A):fabs(A))
+
+/* Reference ellipsoids */
+#define WGS84 1
+#define GRS80 2
+#define WGS72 3
+
+#endif
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
diff --git a/sofa/sp00.c b/sofa/sp00.c
new file mode 100644
index 0000000..1c9e318
--- /dev/null
+++ b/sofa/sp00.c
@@ -0,0 +1,168 @@
+#include "sofam.h"
+
+double iauSp00(double date1, double date2)
+/*
+** - - - - - - - -
+** i a u S p 0 0
+** - - - - - - - -
+**
+** The TIO locator s', positioning the Terrestrial Intermediate Origin
+** on the equator of the Celestial Intermediate Pole.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned (function value):
+** double the TIO locator s' in radians (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The TIO locator s' is obtained from polar motion observations by
+** numerical integration, and so is in essence unpredictable.
+** However, it is dominated by a secular drift of about
+** 47 microarcseconds per century, which is the approximation
+** evaluated by the present function.
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2008 May 24
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double t, sp;
+
+
+/* Interval between fundamental epoch J2000.0 and current date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* Approximate s'. */
+ sp = -47e-6 * t * DAS2R;
+
+ return sp;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/starpm.c b/sofa/starpm.c
new file mode 100644
index 0000000..ba9e4c3
--- /dev/null
+++ b/sofa/starpm.c
@@ -0,0 +1,255 @@
+#include "sofam.h"
+
+int iauStarpm(double ra1, double dec1,
+ double pmr1, double pmd1, double px1, double rv1,
+ double ep1a, double ep1b, double ep2a, double ep2b,
+ double *ra2, double *dec2,
+ double *pmr2, double *pmd2, double *px2, double *rv2)
+/*
+** - - - - - - - - - -
+** i a u S t a r p m
+** - - - - - - - - - -
+**
+** Star proper motion: update star catalog data for space motion.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** ra1 double right ascension (radians), before
+** dec1 double declination (radians), before
+** pmr1 double RA proper motion (radians/year), before
+** pmd1 double Dec proper motion (radians/year), before
+** px1 double parallax (arcseconds), before
+** rv1 double radial velocity (km/s, +ve = receding), before
+** ep1a double "before" epoch, part A (Note 1)
+** ep1b double "before" epoch, part B (Note 1)
+** ep2a double "after" epoch, part A (Note 1)
+** ep2b double "after" epoch, part B (Note 1)
+**
+** Returned:
+** ra2 double right ascension (radians), after
+** dec2 double declination (radians), after
+** pmr2 double RA proper motion (radians/year), after
+** pmd2 double Dec proper motion (radians/year), after
+** px2 double parallax (arcseconds), after
+** rv2 double radial velocity (km/s, +ve = receding), after
+**
+** Returned (function value):
+** int status:
+** -1 = system error (should not occur)
+** 0 = no warnings or errors
+** 1 = distance overridden (Note 6)
+** 2 = excessive velocity (Note 7)
+** 4 = solution didn't converge (Note 8)
+** else = binary logical OR of the above warnings
+**
+** Notes:
+**
+** 1) The starting and ending TDB dates ep1a+ep1b and ep2a+ep2b are
+** Julian Dates, apportioned in any convenient way between the two
+** parts (A and B). For example, JD(TDB)=2450123.7 could be
+** expressed in any of these ways, among others:
+**
+** epna epnb
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) In accordance with normal star-catalog conventions, the object's
+** right ascension and declination are freed from the effects of
+** secular aberration. The frame, which is aligned to the catalog
+** equator and equinox, is Lorentzian and centered on the SSB.
+**
+** The proper motions are the rate of change of the right ascension
+** and declination at the catalog epoch and are in radians per TDB
+** Julian year.
+**
+** The parallax and radial velocity are in the same frame.
+**
+** 3) Care is needed with units. The star coordinates are in radians
+** and the proper motions in radians per Julian year, but the
+** parallax is in arcseconds.
+**
+** 4) The RA proper motion is in terms of coordinate angle, not true
+** angle. If the catalog uses arcseconds for both RA and Dec proper
+** motions, the RA proper motion will need to be divided by cos(Dec)
+** before use.
+**
+** 5) Straight-line motion at constant speed, in the inertial frame,
+** is assumed.
+**
+** 6) An extremely small (or zero or negative) parallax is interpreted
+** to mean that the object is on the "celestial sphere", the radius
+** of which is an arbitrary (large) value (see the iauStarpv
+** function for the value used). When the distance is overridden in
+** this way, the status, initially zero, has 1 added to it.
+**
+** 7) If the space velocity is a significant fraction of c (see the
+** constant VMAX in the function iauStarpv), it is arbitrarily set
+** to zero. When this action occurs, 2 is added to the status.
+**
+** 8) The relativistic adjustment carried out in the iauStarpv function
+** involves an iterative calculation. If the process fails to
+** converge within a set number of iterations, 4 is added to the
+** status.
+**
+** Called:
+** iauStarpv star catalog data to space motion pv-vector
+** iauPvu update a pv-vector
+** iauPdp scalar product of two p-vectors
+** iauPvstar space motion pv-vector to star catalog data
+**
+** This revision: 2008 May 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double pv1[2][3], tl1, dt, pv[2][3], r2, rdv, v2, c2mv2, tl2,
+ pv2[2][3];
+ int j1, j2, j;
+
+
+/* RA,Dec etc. at the "before" epoch to space motion pv-vector. */
+ j1 = iauStarpv(ra1, dec1, pmr1, pmd1, px1, rv1, pv1);
+
+/* Light time when observed (days). */
+ tl1 = iauPm(pv1[0]) / DC;
+
+/* Time interval, "before" to "after" (days). */
+ dt = (ep2a - ep1a) + (ep2b - ep1b);
+
+/* Move star along track from the "before" observed position to the */
+/* "after" geometric position. */
+ iauPvu(dt + tl1, pv1, pv);
+
+/* From this geometric position, deduce the observed light time (days) */
+/* at the "after" epoch (with theoretically unneccessary error check). */
+ r2 = iauPdp(pv[0], pv[0]);
+ rdv = iauPdp(pv[0], pv[1]);
+ v2 = iauPdp(pv[1], pv[1]);
+ c2mv2 = DC*DC - v2;
+ if (c2mv2 <= 0) return -1;
+ tl2 = (-rdv + sqrt(rdv*rdv + c2mv2*r2)) / c2mv2;
+
+/* Move the position along track from the observed place at the */
+/* "before" epoch to the observed place at the "after" epoch. */
+ iauPvu(dt + (tl1 - tl2), pv1, pv2);
+
+/* Space motion pv-vector to RA,Dec etc. at the "after" epoch. */
+ j2 = iauPvstar(pv2, ra2, dec2, pmr2, pmd2, px2, rv2);
+
+/* Final status. */
+ j = (j2 == 0) ? j1 : -1;
+
+ return j;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/starpv.c b/sofa/starpv.c
new file mode 100644
index 0000000..696c01a
--- /dev/null
+++ b/sofa/starpv.c
@@ -0,0 +1,314 @@
+#include "sofam.h"
+
+int iauStarpv(double ra, double dec,
+ double pmr, double pmd, double px, double rv,
+ double pv[2][3])
+/*
+** - - - - - - - - - -
+** i a u S t a r p v
+** - - - - - - - - - -
+**
+** Convert star catalog coordinates to position+velocity vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given (Note 1):
+** ra double right ascension (radians)
+** dec double declination (radians)
+** pmr double RA proper motion (radians/year)
+** pmd double Dec proper motion (radians/year)
+** px double parallax (arcseconds)
+** rv double radial velocity (km/s, positive = receding)
+**
+** Returned (Note 2):
+** pv double[2][3] pv-vector (AU, AU/day)
+**
+** Returned (function value):
+** int status:
+** 0 = no warnings
+** 1 = distance overridden (Note 6)
+** 2 = excessive speed (Note 7)
+** 4 = solution didn't converge (Note 8)
+** else = binary logical OR of the above
+**
+** Notes:
+**
+** 1) The star data accepted by this function are "observables" for an
+** imaginary observer at the solar-system barycenter. Proper motion
+** and radial velocity are, strictly, in terms of barycentric
+** coordinate time, TCB. For most practical applications, it is
+** permissible to neglect the distinction between TCB and ordinary
+** "proper" time on Earth (TT/TAI). The result will, as a rule, be
+** limited by the intrinsic accuracy of the proper-motion and
+** radial-velocity data; moreover, the pv-vector is likely to be
+** merely an intermediate result, so that a change of time unit
+** would cancel out overall.
+**
+** In accordance with normal star-catalog conventions, the object's
+** right ascension and declination are freed from the effects of
+** secular aberration. The frame, which is aligned to the catalog
+** equator and equinox, is Lorentzian and centered on the SSB.
+**
+** 2) The resulting position and velocity pv-vector is with respect to
+** the same frame and, like the catalog coordinates, is freed from
+** the effects of secular aberration. Should the "coordinate
+** direction", where the object was located at the catalog epoch, be
+** required, it may be obtained by calculating the magnitude of the
+** position vector pv[0][0-2] dividing by the speed of light in
+** AU/day to give the light-time, and then multiplying the space
+** velocity pv[1][0-2] by this light-time and adding the result to
+** pv[0][0-2].
+**
+** Summarizing, the pv-vector returned is for most stars almost
+** identical to the result of applying the standard geometrical
+** "space motion" transformation. The differences, which are the
+** subject of the Stumpff paper referenced below, are:
+**
+** (i) In stars with significant radial velocity and proper motion,
+** the constantly changing light-time distorts the apparent proper
+** motion. Note that this is a classical, not a relativistic,
+** effect.
+**
+** (ii) The transformation complies with special relativity.
+**
+** 3) Care is needed with units. The star coordinates are in radians
+** and the proper motions in radians per Julian year, but the
+** parallax is in arcseconds; the radial velocity is in km/s, but
+** the pv-vector result is in AU and AU/day.
+**
+** 4) The RA proper motion is in terms of coordinate angle, not true
+** angle. If the catalog uses arcseconds for both RA and Dec proper
+** motions, the RA proper motion will need to be divided by cos(Dec)
+** before use.
+**
+** 5) Straight-line motion at constant speed, in the inertial frame,
+** is assumed.
+**
+** 6) An extremely small (or zero or negative) parallax is interpreted
+** to mean that the object is on the "celestial sphere", the radius
+** of which is an arbitrary (large) value (see the constant PXMIN).
+** When the distance is overridden in this way, the status,
+** initially zero, has 1 added to it.
+**
+** 7) If the space velocity is a significant fraction of c (see the
+** constant VMAX), it is arbitrarily set to zero. When this action
+** occurs, 2 is added to the status.
+**
+** 8) The relativistic adjustment involves an iterative calculation.
+** If the process fails to converge within a set number (IMAX) of
+** iterations, 4 is added to the status.
+**
+** 9) The inverse transformation is performed by the function
+** iauPvstar.
+**
+** Called:
+** iauS2pv spherical coordinates to pv-vector
+** iauPm modulus of p-vector
+** iauZp zero p-vector
+** iauPn decompose p-vector into modulus and direction
+** iauPdp scalar product of two p-vectors
+** iauSxp multiply p-vector by scalar
+** iauPmp p-vector minus p-vector
+** iauPpp p-vector plus p-vector
+**
+** Reference:
+**
+** Stumpff, P., 1985, Astron.Astrophys. 144, 232-240.
+**
+** This revision: 2009 July 6
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+/* Smallest allowed parallax */
+ static const double PXMIN = 1e-7;
+
+/* Largest allowed speed (fraction of c) */
+ static const double VMAX = 0.5;
+
+/* Maximum number of iterations for relativistic solution */
+ static const int IMAX = 100;
+
+ int i, iwarn;
+ double w, r, rd, rad, decd, v, x[3], usr[3], ust[3],
+ vsr, vst, betst, betsr, bett, betr,
+ dd, ddel, ur[3], ut[3],
+ d = 0.0, del = 0.0, /* to prevent */
+ odd = 0.0, oddel = 0.0, /* compiler */
+ od = 0.0, odel = 0.0; /* warnings */
+
+
+/* Distance (AU). */
+ if (px >= PXMIN) {
+ w = px;
+ iwarn = 0;
+ } else {
+ w = PXMIN;
+ iwarn = 1;
+ }
+ r = DR2AS / w;
+
+/* Radial velocity (AU/day). */
+ rd = DAYSEC * rv * 1e3 / DAU;
+
+/* Proper motion (radian/day). */
+ rad = pmr / DJY;
+ decd = pmd / DJY;
+
+/* To pv-vector (AU,AU/day). */
+ iauS2pv(ra, dec, r, rad, decd, rd, pv);
+
+/* If excessive velocity, arbitrarily set it to zero. */
+ v = iauPm(pv[1]);
+ if (v / DC > VMAX) {
+ iauZp(pv[1]);
+ iwarn += 2;
+ }
+
+/* Isolate the radial component of the velocity (AU/day). */
+ iauPn(pv[0], &w, x);
+ vsr = iauPdp(x, pv[1]);
+ iauSxp(vsr, x, usr);
+
+/* Isolate the transverse component of the velocity (AU/day). */
+ iauPmp(pv[1], usr, ust);
+ vst = iauPm(ust);
+
+/* Special-relativity dimensionless parameters. */
+ betsr = vsr / DC;
+ betst = vst / DC;
+
+/* Determine the inertial-to-observed relativistic correction terms. */
+ bett = betst;
+ betr = betsr;
+ for (i = 0; i < IMAX; i++) {
+ d = 1.0 + betr;
+ del = sqrt(1.0 - betr*betr - bett*bett) - 1.0;
+ betr = d * betsr + del;
+ bett = d * betst;
+ if (i > 0) {
+ dd = fabs(d - od);
+ ddel = fabs(del - odel);
+ if ((i > 1) && (dd >= odd) && (ddel >= oddel)) break;
+ odd = dd;
+ oddel = ddel;
+ }
+ od = d;
+ odel = del;
+ }
+ if (i >= IMAX) iwarn += 4;
+
+/* Replace observed radial velocity with inertial value. */
+ w = (betsr != 0.0) ? d + del / betsr : 1.0;
+ iauSxp(w, usr, ur);
+
+/* Replace observed tangential velocity with inertial value. */
+ iauSxp(d, ust, ut);
+
+/* Combine the two to obtain the inertial space velocity. */
+ iauPpp(ur, ut, pv[1]);
+
+/* Return the status. */
+ return iwarn;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/sxp.c b/sofa/sxp.c
new file mode 100644
index 0000000..f0f2862
--- /dev/null
+++ b/sofa/sxp.c
@@ -0,0 +1,134 @@
+#include "sofam.h"
+
+void iauSxp(double s, double p[3], double sp[3])
+/*
+** - - - - - - -
+** i a u S x p
+** - - - - - - -
+**
+** Multiply a p-vector by a scalar.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** s double scalar
+** p double[3] p-vector
+**
+** Returned:
+** sp double[3] s * p
+**
+** Note:
+** It is permissible for p and sp to be the same array.
+**
+** This revision: 2008 October 28
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ sp[0] = s * p[0];
+ sp[1] = s * p[1];
+ sp[2] = s * p[2];
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/sxpv.c b/sofa/sxpv.c
new file mode 100644
index 0000000..ae2b2bc
--- /dev/null
+++ b/sofa/sxpv.c
@@ -0,0 +1,135 @@
+#include "sofam.h"
+
+void iauSxpv(double s, double pv[2][3], double spv[2][3])
+/*
+** - - - - - - - -
+** i a u S x p v
+** - - - - - - - -
+**
+** Multiply a pv-vector by a scalar.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** s double scalar
+** pv double[2][3] pv-vector
+**
+** Returned:
+** spv double[2][3] s * pv
+**
+** Note:
+** It is permissible for pv and psv to be the same array
+**
+** Called:
+** iauS2xpv multiply pv-vector by two scalars
+**
+** This revision: 2008 October 28
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauS2xpv(s, s, pv, spv);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/taitt.c b/sofa/taitt.c
new file mode 100644
index 0000000..16c314a
--- /dev/null
+++ b/sofa/taitt.c
@@ -0,0 +1,160 @@
+#include "sofam.h"
+
+int iauTaitt(double tai1, double tai2, double *tt1, double *tt2)
+/*
+** - - - - - - - - -
+** i a u T a i t t
+** - - - - - - - - -
+**
+** Time scale transformation: International Atomic Time, TAI, to
+** Terrestrial Time, TT.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** tai1,tai2 double TAI as a 2-part Julian Date
+**
+** Returned:
+** tt1,tt2 double TT as a 2-part Julian Date
+**
+** Returned (function value):
+** int status: 0 = OK
+**
+** Note:
+**
+** tai1+tai2 is Julian Date, apportioned in any convenient way
+** between the two arguments, for example where tai1 is the Julian
+** Day Number and tai2 is the fraction of a day. The returned
+** tt1,tt2 follow suit.
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992)
+**
+** This revision: 2011 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+
+/* TT minus TAI (days). */
+ static const double dtat = TTMTAI/DAYSEC;
+
+
+/* Result, safeguarding precision. */
+ if ( tai1 > tai2 ) {
+ *tt1 = tai1;
+ *tt2 = tai2 + dtat;
+ } else {
+ *tt1 = tai1 + dtat;
+ *tt2 = tai2;
+ }
+
+/* Status (always OK). */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/taiut1.c b/sofa/taiut1.c
new file mode 100644
index 0000000..f6a59c3
--- /dev/null
+++ b/sofa/taiut1.c
@@ -0,0 +1,162 @@
+#include "sofam.h"
+
+int iauTaiut1(double tai1, double tai2, double dta,
+ double *ut11, double *ut12)
+/*
+** - - - - - - - - - -
+** i a u T a i u t 1
+** - - - - - - - - - -
+**
+** Time scale transformation: International Atomic Time, TAI, to
+** Universal Time, UT1.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** tai1,tai2 double TAI as a 2-part Julian Date
+** dta double UT1-TAI in seconds
+**
+** Returned:
+** ut11,ut12 double UT1 as a 2-part Julian Date
+**
+** Returned (function value):
+** int status: 0 = OK
+**
+** Notes:
+**
+** 1) tai1+tai2 is Julian Date, apportioned in any convenient way
+** between the two arguments, for example where tai1 is the Julian
+** Day Number and tai2 is the fraction of a day. The returned
+** UT11,UT12 follow suit.
+**
+** 2) The argument dta, i.e. UT1-TAI, is an observed quantity, and is
+** available from IERS tabulations.
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992)
+**
+** This revision: 2011 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+**
+*/
+{
+ double dtad;
+
+
+/* Result, safeguarding precision. */
+ dtad = dta / DAYSEC;
+ if ( tai1 > tai2 ) {
+ *ut11 = tai1;
+ *ut12 = tai2 + dtad;
+ } else {
+ *ut11 = tai1 + dtad;
+ *ut12 = tai2;
+ }
+
+/* Status (always OK). */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/taiutc.c b/sofa/taiutc.c
new file mode 100644
index 0000000..13910d0
--- /dev/null
+++ b/sofa/taiutc.c
@@ -0,0 +1,232 @@
+#include "sofam.h"
+
+int iauTaiutc(double tai1, double tai2, double *utc1, double *utc2)
+/*
+** - - - - - - - - - -
+** i a u T a i u t c
+** - - - - - - - - - -
+**
+** Time scale transformation: International Atomic Time, TAI, to
+** Coordinated Universal Time, UTC.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** tai1,tai2 double TAI as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** utc1,utc2 double UTC as a 2-part quasi Julian Date (Notes 1-3)
+**
+** Returned (function value):
+** int status: +1 = dubious year (Note 4)
+** 0 = OK
+** -1 = unacceptable date
+**
+** Notes:
+**
+** 1) tai1+tai2 is Julian Date, apportioned in any convenient way
+** between the two arguments, for example where tai1 is the Julian
+** Day Number and tai2 is the fraction of a day. The returned utc1
+** and utc2 form an analogous pair, except that a special convention
+** is used, to deal with the problem of leap seconds - see the next
+** note.
+**
+** 2) JD cannot unambiguously represent UTC during a leap second unless
+** special measures are taken. The convention in the present
+** function is that the JD day represents UTC days whether the
+** length is 86399, 86400 or 86401 SI seconds.
+**
+** 3) The function iauD2dtf can be used to transform the UTC quasi-JD
+** into calendar date and clock time, including UTC leap second
+** handling.
+**
+** 4) The warning status "dubious year" flags UTCs that predate the
+** introduction of the time scale and that are too far in the future
+** to be trusted. See iauDat for further details.
+**
+** Called:
+** iauJd2cal JD to Gregorian calendar
+** iauDat delta(AT) = TAI-UTC
+** iauCal2jd Gregorian calendar to JD
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992)
+**
+** This revision: 2011 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int big1;
+ int i, iy, im, id, js;
+ double a1, a2, d1, dats1, d2, fd, ddats, dats2, datd, as1, as2, da;
+
+
+/* Put the two parts of the TAI into big-first order. */
+ big1 = ( tai1 >= tai2 );
+ if ( big1 ) {
+ a1 = tai1;
+ a2 = tai2;
+ } else {
+ a1 = tai2;
+ a2 = tai1;
+ }
+
+/* See if the TAI can possibly be in a leap-second day. */
+ d1 = a1;
+ dats1 = 0.0;
+ for ( i = -1; i <= 3; i++ ) {
+ d2 = a2 + (double) i;
+ if ( iauJd2cal(d1, d2, &iy, &im, &id, &fd) ) return -1;
+ js = iauDat(iy, im, id, 0.0, &dats2);
+ if ( js < 0 ) return -1;
+ if ( i == -1 ) dats1 = dats2;
+ ddats = dats2 - dats1;
+ datd = dats1 / DAYSEC;
+ if ( fabs(ddats) >= 0.5 ) {
+
+ /* Yes. Get TAI for the start of the UTC day that */
+ /* ends in a leap. */
+ if ( iauCal2jd(iy, im, id, &d1, &d2) ) return -1;
+ as1 = d1;
+ as2 = d2 - 1.0 + datd;
+
+ /* Is the TAI after this point? */
+ da = a1 - as1;
+ da = da + ( a2 - as2 );
+ if ( da > 0 ) {
+
+ /* Yes: fraction of the current UTC day that has elapsed. */
+ fd = da * DAYSEC / ( DAYSEC + ddats );
+
+ /* Ramp TAI-UTC to bring about SOFA's JD(UTC) convention. */
+ datd += ddats * ( fd <= 1.0 ? fd : 1.0 ) / DAYSEC;
+ }
+
+ /* Done. */
+ break;
+ }
+ dats1 = dats2;
+ }
+
+/* Subtract the (possibly adjusted) TAI-UTC from TAI to give UTC. */
+ a2 -= datd;
+
+/* Return the UTC result, preserving the TAI order. */
+ if ( big1 ) {
+ *utc1 = a1;
+ *utc2 = a2;
+ } else {
+ *utc1 = a2;
+ *utc2 = a1;
+ }
+
+/* Status. */
+ return js;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/tcbtdb.c b/sofa/tcbtdb.c
new file mode 100644
index 0000000..1a80592
--- /dev/null
+++ b/sofa/tcbtdb.c
@@ -0,0 +1,182 @@
+#include "sofam.h"
+
+int iauTcbtdb(double tcb1, double tcb2, double *tdb1, double *tdb2)
+/*
+** - - - - - - - - - -
+** i a u T c b t d b
+** - - - - - - - - - -
+**
+** Time scale transformation: Barycentric Coordinate Time, TCB, to
+** Barycentric Dynamical Time, TDB.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** tcb1,tcb2 double TCB as a 2-part Julian Date
+**
+** Returned:
+** tdb1,tdb2 double TDB as a 2-part Julian Date
+**
+** Returned (function value):
+** int status: 0 = OK
+**
+** Notes:
+**
+** 1) tcb1+tcb2 is Julian Date, apportioned in any convenient way
+** between the two arguments, for example where tcb1 is the Julian
+** Day Number and tcb2 is the fraction of a day. The returned
+** tdb1,tdb2 follow suit.
+**
+** 2) The 2006 IAU General Assembly introduced a conventional linear
+** transformation between TDB and TCB. This transformation
+** compensates for the drift between TCB and terrestrial time TT,
+** and keeps TDB approximately centered on TT. Because the
+** relationship between TT and TCB depends on the adopted solar
+** system ephemeris, the degree of alignment between TDB and TT over
+** long intervals will vary according to which ephemeris is used.
+** Former definitions of TDB attempted to avoid this problem by
+** stipulating that TDB and TT should differ only by periodic
+** effects. This is a good description of the nature of the
+** relationship but eluded precise mathematical formulation. The
+** conventional linear relationship adopted in 2006 sidestepped
+** these difficulties whilst delivering a TDB that in practice was
+** consistent with values before that date.
+**
+** 3) TDB is essentially the same as Teph, the time argument for the
+** JPL solar system ephemerides.
+**
+** Reference:
+**
+** IAU 2006 Resolution B3
+**
+** This revision: 2011 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+
+/* 1977 Jan 1 00:00:32.184 TT, as two-part JD */
+ static const double t77td = DJM0 + DJM77;
+ static const double t77tf = TTMTAI/DAYSEC;
+
+/* TDB (days) at TAI 1977 Jan 1.0 */
+ static const double tdb0 = TDB0/DAYSEC;
+
+ double d;
+
+
+/* Result, safeguarding precision. */
+ if ( tcb1 > tcb2 ) {
+ d = tcb1 - t77td;
+ *tdb1 = tcb1;
+ *tdb2 = tcb2 + tdb0 - ( d + ( tcb2 - t77tf ) ) * ELB;
+ } else {
+ d = tcb2 - t77td;
+ *tdb1 = tcb1 + tdb0 - ( d + ( tcb1 - t77tf ) ) * ELB;
+ *tdb2 = tcb2;
+ }
+
+/* Status (always OK). */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/tcgtt.c b/sofa/tcgtt.c
new file mode 100644
index 0000000..85b86d9
--- /dev/null
+++ b/sofa/tcgtt.c
@@ -0,0 +1,159 @@
+#include "sofam.h"
+
+int iauTcgtt(double tcg1, double tcg2, double *tt1, double *tt2)
+/*
+** - - - - - - - - -
+** i a u T c g t t
+** - - - - - - - - -
+**
+** Time scale transformation: Geocentric Coordinate Time, TCG, to
+** Terrestrial Time, TT.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** tcg1,tcg2 double TCG as a 2-part Julian Date
+**
+** Returned:
+** tt1,tt2 double TT as a 2-part Julian Date
+**
+** Returned (function value):
+** int status: 0 = OK
+**
+** Note:
+**
+** tcg1+tcg2 is Julian Date, apportioned in any convenient way
+** between the two arguments, for example where tcg1 is the Julian
+** Day Number and tcg22 is the fraction of a day. The returned
+** tt1,tt2 follow suit.
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),.
+** IERS Technical Note No. 32, BKG (2004)
+**
+** IAU 2000 Resolution B1.9
+**
+** This revision: 2010 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+
+/* 1977 Jan 1 00:00:32.184 TT, as MJD */
+ static const double t77t = DJM77 + TTMTAI/DAYSEC;
+
+
+/* Result, safeguarding precision. */
+ if ( tcg1 > tcg2 ) {
+ *tt1 = tcg1;
+ *tt2 = tcg2 - ( ( tcg1 - DJM0 ) + ( tcg2 - t77t ) ) * ELG;
+ } else {
+ *tt1 = tcg1 - ( ( tcg2 - DJM0 ) + ( tcg1 - t77t ) ) * ELG;
+ *tt2 = tcg2;
+ }
+
+/* OK status. */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/tdbtcb.c b/sofa/tdbtcb.c
new file mode 100644
index 0000000..35d5ded
--- /dev/null
+++ b/sofa/tdbtcb.c
@@ -0,0 +1,187 @@
+#include "sofam.h"
+
+int iauTdbtcb(double tdb1, double tdb2, double *tcb1, double *tcb2)
+/*
+** - - - - - - - - - -
+** i a u T d b t c b
+** - - - - - - - - - -
+**
+** Time scale transformation: Barycentric Dynamical Time, TDB, to
+** Barycentric Coordinate Time, TCB.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** tdb1,tdb2 double TDB as a 2-part Julian Date
+**
+** Returned:
+** tcb1,tcb2 double TCB as a 2-part Julian Date
+**
+** Returned (function value):
+** int status: 0 = OK
+**
+** Notes:
+**
+** 1) tdb1+tdb2 is Julian Date, apportioned in any convenient way
+** between the two arguments, for example where tdb1 is the Julian
+** Day Number and tdb2 is the fraction of a day. The returned
+** tcb1,tcb2 follow suit.
+**
+** 2) The 2006 IAU General Assembly introduced a conventional linear
+** transformation between TDB and TCB. This transformation
+** compensates for the drift between TCB and terrestrial time TT,
+** and keeps TDB approximately centered on TT. Because the
+** relationship between TT and TCB depends on the adopted solar
+** system ephemeris, the degree of alignment between TDB and TT over
+** long intervals will vary according to which ephemeris is used.
+** Former definitions of TDB attempted to avoid this problem by
+** stipulating that TDB and TT should differ only by periodic
+** effects. This is a good description of the nature of the
+** relationship but eluded precise mathematical formulation. The
+** conventional linear relationship adopted in 2006 sidestepped
+** these difficulties whilst delivering a TDB that in practice was
+** consistent with values before that date.
+**
+** 3) TDB is essentially the same as Teph, the time argument for the
+** JPL solar system ephemerides.
+**
+** Reference:
+**
+** IAU 2006 Resolution B3
+**
+** This revision: 2011 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+
+/* 1977 Jan 1 00:00:32.184 TT, as two-part JD */
+ static const double t77td = DJM0 + DJM77;
+ static const double t77tf = TTMTAI/DAYSEC;
+
+/* TDB (days) at TAI 1977 Jan 1.0 */
+ static const double tdb0 = TDB0/DAYSEC;
+
+/* TDB to TCB rate */
+ static const double elbb = ELB/(1.0-ELB);
+
+ double d, f;
+
+
+/* Result, preserving date format but safeguarding precision. */
+ if ( tdb1 > tdb2 ) {
+ d = t77td - tdb1;
+ f = tdb2 - tdb0;
+ *tcb1 = tdb1;
+ *tcb2 = f - ( d - ( f - t77tf ) ) * elbb;
+ } else {
+ d = t77td - tdb2;
+ f = tdb1 - tdb0;
+ *tcb1 = f + ( d - ( f - t77tf ) ) * elbb;
+ *tcb2 = tdb2;
+ }
+
+/* Status (always OK). */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/tdbtt.c b/sofa/tdbtt.c
new file mode 100644
index 0000000..b5d81fe
--- /dev/null
+++ b/sofa/tdbtt.c
@@ -0,0 +1,172 @@
+#include "sofam.h"
+
+int iauTdbtt(double tdb1, double tdb2, double dtr,
+ double *tt1, double *tt2 )
+/*
+** - - - - - - - - -
+** i a u T d b t t
+** - - - - - - - - -
+**
+** Time scale transformation: Barycentric Dynamical Time, TDB, to
+** Terrestrial Time, TT.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** tdb1,tdb2 double TDB as a 2-part Julian Date
+** dtr double TDB-TT in seconds
+**
+** Returned:
+** tt1,tt2 double TT as a 2-part Julian Date
+**
+** Returned (function value):
+** int status: 0 = OK
+**
+** Notes:
+**
+** 1) tdb1+tdb2 is Julian Date, apportioned in any convenient way
+** between the two arguments, for example where tdb1 is the Julian
+** Day Number and tdb2 is the fraction of a day. The returned
+** tt1,tt2 follow suit.
+**
+** 2) The argument dtr represents the quasi-periodic component of the
+** GR transformation between TT and TCB. It is dependent upon the
+** adopted solar-system ephemeris, and can be obtained by numerical
+** integration, by interrogating a precomputed time ephemeris or by
+** evaluating a model such as that implemented in the SOFA function
+** iauDtdb. The quantity is dominated by an annual term of 1.7 ms
+** amplitude.
+**
+** 3) TDB is essentially the same as Teph, the time argument for the
+** JPL solar system ephemerides.
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** IAU 2006 Resolution 3
+**
+** This revision: 2011 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+**
+*/
+{
+ double dtrd;
+
+
+/* Result, safeguarding precision. */
+ dtrd = dtr / DAYSEC;
+ if ( tdb1 > tdb2 ) {
+ *tt1 = tdb1;
+ *tt2 = tdb2 - dtrd;
+ } else {
+ *tt1 = tdb1 - dtrd;
+ *tt2 = tdb2;
+ }
+
+/* Status (always OK). */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/tf2a.c b/sofa/tf2a.c
new file mode 100644
index 0000000..4059f90
--- /dev/null
+++ b/sofa/tf2a.c
@@ -0,0 +1,157 @@
+#include "sofam.h"
+#include <stdlib.h>
+
+int iauTf2a(char s, int ihour, int imin, double sec, double *rad)
+/*
+** - - - - - - - -
+** i a u T f 2 a
+** - - - - - - - -
+**
+** Convert hours, minutes, seconds to radians.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** s char sign: '-' = negative, otherwise positive
+** ihour int hours
+** imin int minutes
+** sec double seconds
+**
+** Returned:
+** rad double angle in radians
+**
+** Returned (function value):
+** int status: 0 = OK
+** 1 = ihour outside range 0-23
+** 2 = imin outside range 0-59
+** 3 = sec outside range 0-59.999...
+**
+** Notes:
+**
+** 1) The result is computed even if any of the range checks fail.
+**
+** 2) Negative ihour, imin and/or sec produce a warning status, but
+** the absolute value is used in the conversion.
+**
+** 3) If there are multiple errors, the status value reflects only the
+** first, the smallest taking precedence.
+**
+** This revision: 2012 February 13
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+
+/* Compute the interval. */
+ *rad = ( s == '-' ? -1.0 : 1.0 ) *
+ ( 60.0 * ( 60.0 * ( (double) abs(ihour) ) +
+ ( (double) abs(imin) ) ) +
+ fabs(sec) ) * DS2R;
+
+/* Validate arguments and return status. */
+ if ( ihour < 0 || ihour > 23 ) return 1;
+ if ( imin < 0 || imin > 59 ) return 2;
+ if ( sec < 0.0 || sec >= 60.0 ) return 3;
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/tf2d.c b/sofa/tf2d.c
new file mode 100644
index 0000000..e3bbe54
--- /dev/null
+++ b/sofa/tf2d.c
@@ -0,0 +1,157 @@
+#include "sofam.h"
+#include <stdlib.h>
+
+int iauTf2d(char s, int ihour, int imin, double sec, double *days)
+/*
+** - - - - - - - -
+** i a u T f 2 d
+** - - - - - - - -
+**
+** Convert hours, minutes, seconds to days.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** s char sign: '-' = negative, otherwise positive
+** ihour int hours
+** imin int minutes
+** sec double seconds
+**
+** Returned:
+** days double interval in days
+**
+** Returned (function value):
+** int status: 0 = OK
+** 1 = ihour outside range 0-23
+** 2 = imin outside range 0-59
+** 3 = sec outside range 0-59.999...
+**
+** Notes:
+**
+** 1) The result is computed even if any of the range checks fail.
+**
+** 2) Negative ihour, imin and/or sec produce a warning status, but
+** the absolute value is used in the conversion.
+**
+** 3) If there are multiple errors, the status value reflects only the
+** first, the smallest taking precedence.
+**
+** This revision: 2012 February 13
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+
+/* Compute the interval. */
+ *days = ( s == '-' ? -1.0 : 1.0 ) *
+ ( 60.0 * ( 60.0 * ( (double) abs(ihour) ) +
+ ( (double) abs(imin) ) ) +
+ fabs(sec) ) / DAYSEC;
+
+/* Validate arguments and return status. */
+ if ( ihour < 0 || ihour > 23 ) return 1;
+ if ( imin < 0 || imin > 59 ) return 2;
+ if ( sec < 0.0 || sec >= 60.0 ) return 3;
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/tr.c b/sofa/tr.c
new file mode 100644
index 0000000..56c93eb
--- /dev/null
+++ b/sofa/tr.c
@@ -0,0 +1,143 @@
+#include "sofam.h"
+
+void iauTr(double r[3][3], double rt[3][3])
+/*
+** - - - - - -
+** i a u T r
+** - - - - - -
+**
+** Transpose an r-matrix.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** r double[3][3] r-matrix
+**
+** Returned:
+** rt double[3][3] transpose
+**
+** Note:
+** It is permissible for r and rt to be the same array.
+**
+** Called:
+** iauCr copy r-matrix
+**
+** This revision: 2008 May 22
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double wm[3][3];
+ int i, j;
+
+
+ for (i = 0; i < 3; i++) {
+ for (j = 0; j < 3; j++) {
+ wm[i][j] = r[j][i];
+ }
+ }
+ iauCr(wm, rt);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/trxp.c b/sofa/trxp.c
new file mode 100644
index 0000000..948ca39
--- /dev/null
+++ b/sofa/trxp.c
@@ -0,0 +1,143 @@
+#include "sofam.h"
+
+void iauTrxp(double r[3][3], double p[3], double trp[3])
+/*
+** - - - - - - - -
+** i a u T r x p
+** - - - - - - - -
+**
+** Multiply a p-vector by the transpose of an r-matrix.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** r double[3][3] r-matrix
+** p double[3] p-vector
+**
+** Returned:
+** trp double[3] r * p
+**
+** Note:
+** It is permissible for p and trp to be the same array.
+**
+** Called:
+** iauTr transpose r-matrix
+** iauRxp product of r-matrix and p-vector
+**
+** This revision: 2008 October 28
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double tr[3][3];
+
+
+/* Transpose of matrix r. */
+ iauTr(r, tr);
+
+/* Matrix tr * vector p -> vector trp. */
+ iauRxp(tr, p, trp);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/trxpv.c b/sofa/trxpv.c
new file mode 100644
index 0000000..9f4156a
--- /dev/null
+++ b/sofa/trxpv.c
@@ -0,0 +1,143 @@
+#include "sofam.h"
+
+void iauTrxpv(double r[3][3], double pv[2][3], double trpv[2][3])
+/*
+** - - - - - - - - -
+** i a u T r x p v
+** - - - - - - - - -
+**
+** Multiply a pv-vector by the transpose of an r-matrix.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Given:
+** r double[3][3] r-matrix
+** pv double[2][3] pv-vector
+**
+** Returned:
+** trpv double[2][3] r * pv
+**
+** Note:
+** It is permissible for pv and trpv to be the same array.
+**
+** Called:
+** iauTr transpose r-matrix
+** iauRxpv product of r-matrix and pv-vector
+**
+** This revision: 2008 October 28
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double tr[3][3];
+
+
+/* Transpose of matrix r. */
+ iauTr(r, tr);
+
+/* Matrix tr * vector pv -> vector trpv. */
+ iauRxpv(tr, pv, trpv);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/tttai.c b/sofa/tttai.c
new file mode 100644
index 0000000..0139442
--- /dev/null
+++ b/sofa/tttai.c
@@ -0,0 +1,160 @@
+#include "sofam.h"
+
+int iauTttai(double tt1, double tt2, double *tai1, double *tai2)
+/*
+** - - - - - - - - -
+** i a u T t t a i
+** - - - - - - - - -
+**
+** Time scale transformation: Terrestrial Time, TT, to International
+** Atomic Time, TAI.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** tt1,tt2 double TT as a 2-part Julian Date
+**
+** Returned:
+** tai1,tai2 double TAI as a 2-part Julian Date
+**
+** Returned (function value):
+** int status: 0 = OK
+**
+** Note:
+**
+** tt1+tt2 is Julian Date, apportioned in any convenient way between
+** the two arguments, for example where tt1 is the Julian Day Number
+** and tt2 is the fraction of a day. The returned tai1,tai2 follow
+** suit.
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992)
+**
+** This revision: 2011 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+
+/* TT minus TAI (days). */
+ static const double dtat = TTMTAI/DAYSEC;
+
+
+/* Result, safeguarding precision. */
+ if ( tt1 > tt2 ) {
+ *tai1 = tt1;
+ *tai2 = tt2 - dtat;
+ } else {
+ *tai1 = tt1 - dtat;
+ *tai2 = tt2;
+ }
+
+/* Status (always OK). */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/tttcg.c b/sofa/tttcg.c
new file mode 100644
index 0000000..124ff22
--- /dev/null
+++ b/sofa/tttcg.c
@@ -0,0 +1,162 @@
+#include "sofam.h"
+
+int iauTttcg(double tt1, double tt2, double *tcg1, double *tcg2)
+/*
+** - - - - - - - - -
+** i a u T t t c g
+** - - - - - - - - -
+**
+** Time scale transformation: Terrestrial Time, TT, to Geocentric
+** Coordinate Time, TCG.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** tt1,tt2 double TT as a 2-part Julian Date
+**
+** Returned:
+** tcg1,tcg2 double TCG as a 2-part Julian Date
+**
+** Returned (function value):
+** int status: 0 = OK
+**
+** Note:
+**
+** tt1+tt2 is Julian Date, apportioned in any convenient way between
+** the two arguments, for example where tt1 is the Julian Day Number
+** and tt2 is the fraction of a day. The returned tcg1,tcg2 follow
+** suit.
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** IAU 2000 Resolution B1.9
+**
+** This revision: 2010 May 13
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+
+/* 1977 Jan 1 00:00:32.184 TT, as MJD */
+ static const double t77t = DJM77 + TTMTAI/DAYSEC;
+
+/* TT to TCG rate */
+ static const double elgg = ELG/(1.0-ELG);
+
+
+/* Result, safeguarding precision. */
+ if ( tt1 > tt2 ) {
+ *tcg1 = tt1;
+ *tcg2 = tt2 + ( ( tt1 - DJM0 ) + ( tt2 - t77t ) ) * elgg;
+ } else {
+ *tcg1 = tt1 + ( ( tt2 - DJM0 ) + ( tt1 - t77t ) ) * elgg;
+ *tcg2 = tt2;
+ }
+
+/* Status (always OK). */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/tttdb.c b/sofa/tttdb.c
new file mode 100644
index 0000000..a8e611e
--- /dev/null
+++ b/sofa/tttdb.c
@@ -0,0 +1,171 @@
+#include "sofam.h"
+
+int iauTttdb(double tt1, double tt2, double dtr,
+ double *tdb1, double *tdb2)
+/*
+** - - - - - - - - -
+** i a u T t t d b
+** - - - - - - - - -
+**
+** Time scale transformation: Terrestrial Time, TT, to Barycentric
+** Dynamical Time, TDB.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** tt1,tt2 double TT as a 2-part Julian Date
+** dtr double TDB-TT in seconds
+**
+** Returned:
+** tdb1,tdb2 double TDB as a 2-part Julian Date
+**
+** Returned (function value):
+** int status: 0 = OK
+**
+** Notes:
+**
+** 1) tt1+tt2 is Julian Date, apportioned in any convenient way between
+** the two arguments, for example where tt1 is the Julian Day Number
+** and tt2 is the fraction of a day. The returned tdb1,tdb2 follow
+** suit.
+**
+** 2) The argument dtr represents the quasi-periodic component of the
+** GR transformation between TT and TCB. It is dependent upon the
+** adopted solar-system ephemeris, and can be obtained by numerical
+** integration, by interrogating a precomputed time ephemeris or by
+** evaluating a model such as that implemented in the SOFA function
+** iauDtdb. The quantity is dominated by an annual term of 1.7 ms
+** amplitude.
+**
+** 3) TDB is essentially the same as Teph, the time argument for the JPL
+** solar system ephemerides.
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** IAU 2006 Resolution 3
+**
+** This revision: 2011 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dtrd;
+
+
+/* Result, safeguarding precision. */
+ dtrd = dtr / DAYSEC;
+ if ( tt1 > tt2 ) {
+ *tdb1 = tt1;
+ *tdb2 = tt2 + dtrd;
+ } else {
+ *tdb1 = tt1 + dtrd;
+ *tdb2 = tt2;
+ }
+
+/* Status (always OK). */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/ttut1.c b/sofa/ttut1.c
new file mode 100644
index 0000000..3b1a3d8
--- /dev/null
+++ b/sofa/ttut1.c
@@ -0,0 +1,160 @@
+#include "sofam.h"
+
+int iauTtut1(double tt1, double tt2, double dt,
+ double *ut11, double *ut12)
+/*
+** - - - - - - - - -
+** i a u T t u t 1
+** - - - - - - - - -
+**
+** Time scale transformation: Terrestrial Time, TT, to Universal Time,
+** UT1.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** tt1,tt2 double TT as a 2-part Julian Date
+** dt double TT-UT1 in seconds
+**
+** Returned:
+** ut11,ut12 double UT1 as a 2-part Julian Date
+**
+** Returned (function value):
+** int status: 0 = OK
+**
+** Notes:
+**
+** 1) tt1+tt2 is Julian Date, apportioned in any convenient way between
+** the two arguments, for example where tt1 is the Julian Day Number
+** and tt2 is the fraction of a day. The returned ut11,ut12 follow
+** suit.
+**
+** 2) The argument dt is classical Delta T.
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992)
+**
+** This revision: 2011 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dtd;
+
+
+/* Result, safeguarding precision. */
+ dtd = dt / DAYSEC;
+ if ( tt1 > tt2 ) {
+ *ut11 = tt1;
+ *ut12 = tt2 - dtd;
+ } else {
+ *ut11 = tt1 - dtd;
+ *ut12 = tt2;
+ }
+
+/* Status (always OK). */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/ut1tai.c b/sofa/ut1tai.c
new file mode 100644
index 0000000..3779ccc
--- /dev/null
+++ b/sofa/ut1tai.c
@@ -0,0 +1,161 @@
+#include "sofam.h"
+
+int iauUt1tai(double ut11, double ut12, double dta,
+ double *tai1, double *tai2)
+/*
+** - - - - - - - - - -
+** i a u U t 1 t a i
+** - - - - - - - - - -
+**
+** Time scale transformation: Universal Time, UT1, to International
+** Atomic Time, TAI.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** ut11,ut12 double UT1 as a 2-part Julian Date
+** dta double UT1-TAI in seconds
+**
+** Returned:
+** tai1,tai2 double TAI as a 2-part Julian Date
+**
+** Returned (function value):
+** int status: 0 = OK
+**
+** Notes:
+**
+** 1) ut11+ut12 is Julian Date, apportioned in any convenient way
+** between the two arguments, for example where ut11 is the Julian
+** Day Number and ut12 is the fraction of a day. The returned
+** tai1,tai2 follow suit.
+**
+** 2) The argument dta, i.e. UT1-TAI, is an observed quantity, and is
+** available from IERS tabulations.
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992)
+**
+** This revision: 2011 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dtad;
+
+
+/* Result, safeguarding precision. */
+ dtad = dta / DAYSEC;
+ if ( ut11 > ut12 ) {
+ *tai1 = ut11;
+ *tai2 = ut12 - dtad;
+ } else {
+ *tai1 = ut11 - dtad;
+ *tai2 = ut12;
+ }
+
+/* Status (always OK). */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/ut1tt.c b/sofa/ut1tt.c
new file mode 100644
index 0000000..3b53f51
--- /dev/null
+++ b/sofa/ut1tt.c
@@ -0,0 +1,160 @@
+#include "sofam.h"
+
+int iauUt1tt(double ut11, double ut12, double dt,
+ double *tt1, double *tt2)
+/*
+** - - - - - - - - -
+** i a u U t 1 t t
+** - - - - - - - - -
+**
+** Time scale transformation: Universal Time, UT1, to Terrestrial
+** Time, TT.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** ut11,ut12 double UT1 as a 2-part Julian Date
+** dt double TT-UT1 in seconds
+**
+** Returned:
+** tt1,tt2 double TT as a 2-part Julian Date
+**
+** Returned (function value):
+** int status: 0 = OK
+**
+** Notes:
+**
+** 1) ut11+ut12 is Julian Date, apportioned in any convenient way
+** between the two arguments, for example where ut11 is the Julian
+** Day Number and ut12 is the fraction of a day. The returned
+** tt1,tt2 follow suit.
+**
+** 2) The argument dt is classical Delta T.
+**
+** Reference:
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992)
+**
+** This revision: 2011 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double dtd;
+
+
+/* Result, safeguarding precision. */
+ dtd = dt / DAYSEC;
+ if ( ut11 > ut12 ) {
+ *tt1 = ut11;
+ *tt2 = ut12 + dtd;
+ } else {
+ *tt1 = ut11 + dtd;
+ *tt2 = ut12;
+ }
+
+/* Status (always OK). */
+ return 0;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/ut1utc.c b/sofa/ut1utc.c
new file mode 100644
index 0000000..e8789df
--- /dev/null
+++ b/sofa/ut1utc.c
@@ -0,0 +1,243 @@
+#include "sofam.h"
+
+int iauUt1utc(double ut11, double ut12, double dut1,
+ double *utc1, double *utc2)
+/*
+** - - - - - - - - - -
+** i a u U t 1 u t c
+** - - - - - - - - - -
+**
+** Time scale transformation: Universal Time, UT1, to Coordinated
+** Universal Time, UTC.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** ut11,ut12 double UT1 as a 2-part Julian Date (Note 1)
+** dut1 double Delta UT1: UT1-UTC in seconds (Note 2)
+**
+** Returned:
+** utc1,utc2 double UTC as a 2-part quasi Julian Date (Notes 3,4)
+**
+** Returned (function value):
+** int status: +1 = dubious year (Note 5)
+** 0 = OK
+** -1 = unacceptable date
+**
+** Notes:
+**
+** 1) ut11+ut12 is Julian Date, apportioned in any convenient way
+** between the two arguments, for example where ut11 is the Julian
+** Day Number and ut12 is the fraction of a day. The returned utc1
+** and utc2 form an analogous pair, except that a special convention
+** is used, to deal with the problem of leap seconds - see Note 3.
+**
+** 2) Delta UT1 can be obtained from tabulations provided by the
+** International Earth Rotation and Reference Systems Service. The
+** value changes abruptly by 1s at a leap second; however, close to
+** a leap second the algorithm used here is tolerant of the "wrong"
+** choice of value being made.
+**
+** 3) JD cannot unambiguously represent UTC during a leap second unless
+** special measures are taken. The convention in the present
+** function is that the returned quasi JD day UTC1+UTC2 represents
+** UTC days whether the length is 86399, 86400 or 86401 SI seconds.
+**
+** 4) The function iauD2dtf can be used to transform the UTC quasi-JD
+** into calendar date and clock time, including UTC leap second
+** handling.
+**
+** 5) The warning status "dubious year" flags UTCs that predate the
+** introduction of the time scale and that are too far in the future
+** to be trusted. See iauDat for further details.
+**
+** Called:
+** iauJd2cal JD to Gregorian calendar
+** iauDat delta(AT) = TAI-UTC
+** iauCal2jd Gregorian calendar to JD
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992)
+**
+** This revision: 2011 May 14
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int big1;
+ int i, iy, im, id, js;
+ double duts, u1, u2, d1, dats1, d2, fd, dats2, ddats, us1, us2, du;
+
+
+/* UT1-UTC in seconds. */
+ duts = dut1;
+
+/* Put the two parts of the UT1 into big-first order. */
+ big1 = ( ut11 >= ut12 );
+ if ( big1 ) {
+ u1 = ut11;
+ u2 = ut12;
+ } else {
+ u1 = ut12;
+ u2 = ut11;
+ }
+
+/* See if the UT1 can possibly be in a leap-second day. */
+ d1 = u1;
+ dats1 = 0;
+ for ( i = -1; i <= 3; i++ ) {
+ d2 = u2 + (double) i;
+ if ( iauJd2cal(d1, d2, &iy, &im, &id, &fd) ) return -1;
+ js = iauDat(iy, im, id, 0.0, &dats2);
+ if ( js < 0 ) return -1;
+ if ( i == - 1 ) dats1 = dats2;
+ ddats = dats2 - dats1;
+ if ( fabs(ddats) >= 0.5 ) {
+
+ /* Yes, leap second nearby: ensure UT1-UTC is "before" value. */
+ if ( ddats * duts >= 0 ) duts -= ddats;
+
+ /* UT1 for the start of the UTC day that ends in a leap. */
+ if ( iauCal2jd(iy, im, id, &d1, &d2) ) return -1;
+ us1 = d1;
+ us2 = d2 - 1.0 + duts/DAYSEC;
+
+ /* Is the UT1 after this point? */
+ du = u1 - us1;
+ du += u2 - us2;
+ if ( du > 0 ) {
+
+ /* Yes: fraction of the current UTC day that has elapsed. */
+ fd = du * DAYSEC / ( DAYSEC + ddats );
+
+ /* Ramp UT1-UTC to bring about SOFA's JD(UTC) convention. */
+ duts += ddats * ( fd <= 1.0 ? fd : 1.0 );
+ }
+
+ /* Done. */
+ break;
+ }
+ dats1 = dats2;
+ }
+
+/* Subtract the (possibly adjusted) UT1-UTC from UT1 to give UTC. */
+ u2 -= duts / DAYSEC;
+
+/* Result, safeguarding precision. */
+ if ( big1 ) {
+ *utc1 = u1;
+ *utc2 = u2;
+ } else {
+ *utc1 = u2;
+ *utc2 = u1;
+ }
+
+/* Status. */
+ return js;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/utctai.c b/sofa/utctai.c
new file mode 100644
index 0000000..2215b0c
--- /dev/null
+++ b/sofa/utctai.c
@@ -0,0 +1,213 @@
+#include "sofam.h"
+
+int iauUtctai(double utc1, double utc2, double *tai1, double *tai2)
+/*
+** - - - - - - - - - -
+** i a u U t c t a i
+** - - - - - - - - - -
+**
+** Time scale transformation: Coordinated Universal Time, UTC, to
+** International Atomic Time, TAI.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** utc1,utc2 double UTC as a 2-part quasi Julian Date (Notes 1-4)
+**
+** Returned:
+** tai1,tai2 double TAI as a 2-part Julian Date (Note 5)
+**
+** Returned (function value):
+** int status: +1 = dubious year (Note 3)
+** 0 = OK
+** -1 = unacceptable date
+**
+** Notes:
+**
+** 1) utc1+utc2 is quasi Julian Date (see Note 2), apportioned in any
+** convenient way between the two arguments, for example where utc1
+** is the Julian Day Number and utc2 is the fraction of a day.
+**
+** 2) JD cannot unambiguously represent UTC during a leap second unless
+** special measures are taken. The convention in the present
+** function is that the JD day represents UTC days whether the
+** length is 86399, 86400 or 86401 SI seconds.
+**
+** 3) The warning status "dubious year" flags UTCs that predate the
+** introduction of the time scale and that are too far in the future
+** to be trusted. See iauDat for further details.
+**
+** 4) The function iauDtf2d converts from calendar date and time of day
+** into 2-part Julian Date, and in the case of UTC implements the
+** leap-second-ambiguity convention described above.
+**
+** 5) The returned TAI1,TAI2 are such that their sum is the TAI Julian
+** Date.
+**
+** Called:
+** iauJd2cal JD to Gregorian calendar
+** iauDat delta(AT) = TAI-UTC
+** iauCal2jd Gregorian calendar to JD
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992)
+**
+** This revision: 2010 September 10
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+**
+*/
+{
+ int big1;
+ int iy, im, id, js, iyt, imt, idt;
+ double u1, u2, fd, dats, fdt, datst, ddat, z1, z2, a2;
+
+
+/* Put the two parts of the UTC into big-first order. */
+ big1 = ( utc1 >= utc2 );
+ if ( big1 ) {
+ u1 = utc1;
+ u2 = utc2;
+ } else {
+ u1 = utc2;
+ u2 = utc1;
+ }
+
+/* Get TAI-UTC now. */
+ if ( iauJd2cal(u1, u2, &iy, &im, &id, &fd) ) return -1;
+ js = iauDat(iy, im, id, fd, &dats);
+ if ( js < 0 ) return -1;
+
+/* Get TAI-UTC tomorrow. */
+ if ( iauJd2cal(u1+1.5, u2-fd, &iyt, &imt, &idt, &fdt) ) return -1;
+ js = iauDat(iyt, imt, idt, fdt, &datst);
+ if ( js < 0 ) return -1;
+
+/* If today ends in a leap second, scale the fraction into SI days. */
+ ddat = datst - dats;
+ if ( fabs(ddat) > 0.5 ) fd += fd * ddat / DAYSEC;
+
+/* Today's calendar date to 2-part JD. */
+ if ( iauCal2jd(iy, im, id, &z1, &z2) ) return -1;
+
+/* Assemble the TAI result, preserving the UTC split and order. */
+ a2 = z1 - u1;
+ a2 += z2;
+ a2 += fd + dats / DAYSEC;
+ if ( big1 ) {
+ *tai1 = u1;
+ *tai2 = a2;
+ } else {
+ *tai1 = a2;
+ *tai2 = u1;
+ }
+
+/* Status. */
+ return js;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/utcut1.c b/sofa/utcut1.c
new file mode 100644
index 0000000..42eba17
--- /dev/null
+++ b/sofa/utcut1.c
@@ -0,0 +1,201 @@
+#include "sofam.h"
+
+int iauUtcut1(double utc1, double utc2, double dut1,
+ double *ut11, double *ut12)
+/*
+** - - - - - - - - - -
+** i a u U t c u t 1
+** - - - - - - - - - -
+**
+** Time scale transformation: Coordinated Universal Time, UTC, to
+** Universal Time, UT1.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards of Fundamental Astronomy) software collection.
+**
+** Status: canonical.
+**
+** Given:
+** utc1,utc2 double UTC as a 2-part quasi Julian Date (Notes 1-4)
+** dut1 double Delta UT1 = UT1-UTC in seconds (Note 5)
+**
+** Returned:
+** ut11,ut12 double UT1 as a 2-part Julian Date (Note 6)
+**
+** Returned (function value):
+** int status: +1 = dubious year (Note 7)
+** 0 = OK
+** -1 = unacceptable date
+**
+** Notes:
+**
+** 1) utc1+utc2 is quasi Julian Date (see Note 2), apportioned in any
+** convenient way between the two arguments, for example where utc1
+** is the Julian Day Number and utc2 is the fraction of a day.
+**
+** 2) JD cannot unambiguously represent UTC during a leap second unless
+** special measures are taken. The convention in the present
+** function is that the JD day represents UTC days whether the
+** length is 86399, 86400 or 86401 SI seconds.
+**
+** 3) The warning status "dubious year" flags UTCs that predate the
+** introduction of the time scale and that are too far in the future
+** to be trusted. See iauDat for further details.
+**
+** 4) The function iauDtf2d converts from calendar date and time of
+** day into 2-part Julian Date, and in the case of UTC implements
+** the leap-second-ambiguity convention described above.
+**
+** 5) Delta UT1 can be obtained from tabulations provided by the
+** International Earth Rotation and Reference Systems Service. It
+** It is the caller's responsibility to supply a DUT argument
+** containing the UT1-UTC value that matches the given UTC.
+**
+** 6) The returned ut11,ut12 are such that their sum is the UT1 Julian
+** Date.
+**
+** 7) The warning status "dubious year" flags UTCs that predate the
+** introduction of the time scale and that are too far in the future
+** to be trusted. See iauDat for further details.
+**
+** References:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** Explanatory Supplement to the Astronomical Almanac,
+** P. Kenneth Seidelmann (ed), University Science Books (1992)
+**
+** Called:
+** iauJd2cal JD to Gregorian calendar
+** iauDat delta(AT) = TAI-UTC
+** iauUtctai UTC to TAI
+** iauTaiut1 TAI to UT1
+**
+** This revision: 2010 May 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int iy, im, id, js, jw;
+ double w, dat, dta, tai1, tai2;
+
+
+/* Look up TAI-UTC. */
+ if ( iauJd2cal(utc1, utc2, &iy, &im, &id, &w) ) return -1;
+ js = iauDat ( iy, im, id, 0.0, &dat);
+ if ( js < 0 ) return -1;
+
+/* Form UT1-TAI. */
+ dta = dut1 - dat;
+
+/* UTC to TAI to UT1. */
+ jw = iauUtctai(utc1, utc2, &tai1, &tai2);
+ if ( jw < 0 ) {
+ return -1;
+ } else if ( jw > 0 ) {
+ js = jw;
+ }
+ if ( iauTaiut1(tai1, tai2, dta, ut11, ut12) ) return -1;
+
+/* Status. */
+ return js;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/xy06.c b/sofa/xy06.c
new file mode 100644
index 0000000..09084d1
--- /dev/null
+++ b/sofa/xy06.c
@@ -0,0 +1,2808 @@
+#include "sofam.h"
+
+void iauXy06(double date1, double date2, double *x, double *y)
+/*
+** - - - - - - - -
+** i a u X y 0 6
+** - - - - - - - -
+**
+** X,Y coordinates of celestial intermediate pole from series based
+** on IAU 2006 precession and IAU 2000A nutation.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: canonical model.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** x,y double CIP X,Y coordinates (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The X,Y coordinates are those of the unit vector towards the
+** celestial intermediate pole. They represent the combined effects
+** of frame bias, precession and nutation.
+**
+** 3) The fundamental arguments used are as adopted in IERS Conventions
+** (2003) and are from Simon et al. (1994) and Souchay et al.
+** (1999).
+**
+** 4) This is an alternative to the angles-based method, via the SOFA
+** function iauFw2xy and as used in iauXys06a for example. The two
+** methods agree at the 1 microarcsecond level (at present), a
+** negligible amount compared with the intrinsic accuracy of the
+** models. However, it would be unwise to mix the two methods
+** (angles-based and series-based) in a single application.
+**
+** Called:
+** iauFal03 mean anomaly of the Moon
+** iauFalp03 mean anomaly of the Sun
+** iauFaf03 mean argument of the latitude of the Moon
+** iauFad03 mean elongation of the Moon from the Sun
+** iauFaom03 mean longitude of the Moon's ascending node
+** iauFame03 mean longitude of Mercury
+** iauFave03 mean longitude of Venus
+** iauFae03 mean longitude of Earth
+** iauFama03 mean longitude of Mars
+** iauFaju03 mean longitude of Jupiter
+** iauFasa03 mean longitude of Saturn
+** iauFaur03 mean longitude of Uranus
+** iauFane03 mean longitude of Neptune
+** iauFapa03 general accumulated precession in longitude
+**
+** References:
+**
+** Capitaine, N., Wallace, P.T. & Chapront, J., 2003,
+** Astron.Astrophys., 412, 567
+**
+** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855
+**
+** McCarthy, D. D., Petit, G. (eds.), 2004, IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG
+**
+** Simon, J.L., Bretagnon, P., Chapront, J., Chapront-Touze, M.,
+** Francou, G. & Laskar, J., Astron.Astrophys., 1994, 282, 663
+**
+** Souchay, J., Loysel, B., Kinoshita, H., Folgueira, M., 1999,
+** Astron.Astrophys.Supp.Ser. 135, 111
+**
+** Wallace, P.T. & Capitaine, N., 2006, Astron.Astrophys. 459, 981
+**
+** This revision: 2009 October 16
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+
+/* Maximum power of T in the polynomials for X and Y */
+#define MAXPT (5)
+
+/* Polynomial coefficients (arcsec, X then Y). */
+ static const double xyp[2][MAXPT+1] = {
+
+ { -0.016617,
+ 2004.191898,
+ -0.4297829,
+ -0.19861834,
+ 0.000007578,
+ 0.0000059285
+ },
+ { -0.006951,
+ -0.025896,
+ -22.4072747,
+ 0.00190059,
+ 0.001112526,
+ 0.0000001358
+ }
+ };
+
+/* Fundamental-argument multipliers: luni-solar terms */
+ static const int mfals[][5] = {
+
+ /* 1-10 */
+ { 0, 0, 0, 0, 1 },
+ { 0, 0, 2, -2, 2 },
+ { 0, 0, 2, 0, 2 },
+ { 0, 0, 0, 0, 2 },
+ { 0, 1, 0, 0, 0 },
+ { 0, 1, 2, -2, 2 },
+ { 1, 0, 0, 0, 0 },
+ { 0, 0, 2, 0, 1 },
+ { 1, 0, 2, 0, 2 },
+ { 0, 1, -2, 2, -2 },
+
+ /* 11-20 */
+ { 0, 0, 2, -2, 1 },
+ { 1, 0, -2, 0, -2 },
+ { 1, 0, 0, -2, 0 },
+ { 1, 0, 0, 0, 1 },
+ { 1, 0, 0, 0, -1 },
+ { 1, 0, -2, -2, -2 },
+ { 1, 0, 2, 0, 1 },
+ { 2, 0, -2, 0, -1 },
+ { 0, 0, 0, 2, 0 },
+ { 0, 0, 2, 2, 2 },
+
+ /* 21-30 */
+ { 2, 0, 0, -2, 0 },
+ { 0, 2, -2, 2, -2 },
+ { 2, 0, 2, 0, 2 },
+ { 1, 0, 2, -2, 2 },
+ { 1, 0, -2, 0, -1 },
+ { 2, 0, 0, 0, 0 },
+ { 0, 0, 2, 0, 0 },
+ { 0, 1, 0, 0, 1 },
+ { 1, 0, 0, -2, -1 },
+ { 0, 2, 2, -2, 2 },
+
+ /* 31-40 */
+ { 0, 0, 2, -2, 0 },
+ { 1, 0, 0, -2, 1 },
+ { 0, 1, 0, 0, -1 },
+ { 0, 2, 0, 0, 0 },
+ { 1, 0, -2, -2, -1 },
+ { 1, 0, 2, 2, 2 },
+ { 0, 1, 2, 0, 2 },
+ { 2, 0, -2, 0, 0 },
+ { 0, 0, 2, 2, 1 },
+ { 0, 1, -2, 0, -2 },
+
+ /* 41-50 */
+ { 0, 0, 0, 2, 1 },
+ { 1, 0, 2, -2, 1 },
+ { 2, 0, 0, -2, -1 },
+ { 2, 0, 2, -2, 2 },
+ { 2, 0, 2, 0, 1 },
+ { 0, 0, 0, 2, -1 },
+ { 0, 1, -2, 2, -1 },
+ { 1, 1, 0, -2, 0 },
+ { 2, 0, 0, -2, 1 },
+ { 1, 0, 0, 2, 0 },
+
+ /* 51-60 */
+ { 0, 1, 2, -2, 1 },
+ { 1, -1, 0, 0, 0 },
+ { 0, 1, -1, 1, -1 },
+ { 2, 0, -2, 0, -2 },
+ { 0, 1, 0, -2, 0 },
+ { 1, 0, 0, -1, 0 },
+ { 3, 0, 2, 0, 2 },
+ { 0, 0, 0, 1, 0 },
+ { 1, -1, 2, 0, 2 },
+ { 1, 1, -2, -2, -2 },
+
+ /* 61-70 */
+ { 1, 0, -2, 0, 0 },
+ { 2, 0, 0, 0, -1 },
+ { 0, 1, -2, -2, -2 },
+ { 1, 1, 2, 0, 2 },
+ { 2, 0, 0, 0, 1 },
+ { 1, 1, 0, 0, 0 },
+ { 1, 0, -2, 2, -1 },
+ { 1, 0, 2, 0, 0 },
+ { 1, -1, 0, -1, 0 },
+ { 1, 0, 0, 0, 2 },
+
+ /* 71-80 */
+ { 1, 0, -1, 0, -1 },
+ { 0, 0, 2, 1, 2 },
+ { 1, 0, -2, -4, -2 },
+ { 1, -1, 0, -1, -1 },
+ { 1, 0, 2, 2, 1 },
+ { 0, 2, -2, 2, -1 },
+ { 1, 0, 0, 0, -2 },
+ { 2, 0, -2, -2, -2 },
+ { 1, 1, 2, -2, 2 },
+ { 2, 0, -2, -4, -2 },
+
+ /* 81-90 */
+ { 1, 0, -4, 0, -2 },
+ { 2, 0, 2, -2, 1 },
+ { 1, 0, 0, -1, -1 },
+ { 2, 0, 2, 2, 2 },
+ { 3, 0, 0, 0, 0 },
+ { 1, 0, 0, 2, 1 },
+ { 0, 0, 2, -2, -1 },
+ { 3, 0, 2, -2, 2 },
+ { 0, 0, 4, -2, 2 },
+ { 1, 0, 0, -4, 0 },
+
+ /* 91-100 */
+ { 0, 1, 2, 0, 1 },
+ { 2, 0, 0, -4, 0 },
+ { 1, 1, 0, -2, -1 },
+ { 2, 0, -2, 0, 1 },
+ { 0, 0, 2, 0, -1 },
+ { 0, 1, -2, 0, -1 },
+ { 0, 1, 0, 0, 2 },
+ { 0, 0, 2, -1, 2 },
+ { 0, 0, 2, 4, 2 },
+ { 2, 1, 0, -2, 0 },
+
+ /* 101-110 */
+ { 1, 1, 0, -2, 1 },
+ { 1, -1, 0, -2, 0 },
+ { 1, -1, 0, -1, -2 },
+ { 1, -1, 0, 0, 1 },
+ { 0, 1, -2, 2, 0 },
+ { 0, 1, 0, 0, -2 },
+ { 1, -1, 2, 2, 2 },
+ { 1, 0, 0, 2, -1 },
+ { 1, -1, -2, -2, -2 },
+ { 3, 0, 2, 0, 1 },
+
+ /* 111-120 */
+ { 0, 1, 2, 2, 2 },
+ { 1, 0, 2, -2, 0 },
+ { 1, 1, -2, -2, -1 },
+ { 1, 0, 2, -4, 1 },
+ { 0, 1, -2, -2, -1 },
+ { 2, -1, 2, 0, 2 },
+ { 0, 0, 0, 2, 2 },
+ { 1, -1, 2, 0, 1 },
+ { 1, -1, -2, 0, -2 },
+ { 0, 1, 0, 2, 0 },
+
+ /* 121-130 */
+ { 0, 1, 2, -2, 0 },
+ { 0, 0, 0, 1, 1 },
+ { 1, 0, -2, -2, 0 },
+ { 0, 3, 2, -2, 2 },
+ { 2, 1, 2, 0, 2 },
+ { 1, 1, 0, 0, 1 },
+ { 2, 0, 0, 2, 0 },
+ { 1, 1, 2, 0, 1 },
+ { 1, 0, 0, -2, -2 },
+ { 1, 0, -2, 2, 0 },
+
+ /* 131-140 */
+ { 1, 0, -1, 0, -2 },
+ { 0, 1, 0, -2, 1 },
+ { 0, 1, 0, 1, 0 },
+ { 0, 0, 0, 1, -1 },
+ { 1, 0, -2, 2, -2 },
+ { 1, -1, 0, 0, -1 },
+ { 0, 0, 0, 4, 0 },
+ { 1, -1, 0, 2, 0 },
+ { 1, 0, 2, 1, 2 },
+ { 1, 0, 2, -1, 2 },
+
+ /* 141-150 */
+ { 0, 0, 2, 1, 1 },
+ { 1, 0, 0, -2, 2 },
+ { 1, 0, -2, 0, 1 },
+ { 1, 0, -2, -4, -1 },
+ { 0, 0, 2, 2, 0 },
+ { 1, 1, 2, -2, 1 },
+ { 1, 0, -2, 1, -1 },
+ { 0, 0, 1, 0, 1 },
+ { 2, 0, -2, -2, -1 },
+ { 4, 0, 2, 0, 2 },
+
+ /* 151-160 */
+ { 2, -1, 0, 0, 0 },
+ { 2, 1, 2, -2, 2 },
+ { 0, 1, 2, 1, 2 },
+ { 1, 0, 4, -2, 2 },
+ { 1, 1, 0, 0, -1 },
+ { 2, 0, 2, 0, 0 },
+ { 2, 0, -2, -4, -1 },
+ { 1, 0, -1, 0, 0 },
+ { 1, 0, 0, 1, 0 },
+ { 0, 1, 0, 2, 1 },
+
+ /* 161-170 */
+ { 1, 0, -4, 0, -1 },
+ { 1, 0, 0, -4, -1 },
+ { 2, 0, 2, 2, 1 },
+ { 2, 1, 0, 0, 0 },
+ { 0, 0, 2, -3, 2 },
+ { 1, 2, 0, -2, 0 },
+ { 0, 3, 0, 0, 0 },
+ { 0, 0, 4, 0, 2 },
+ { 0, 0, 2, -4, 1 },
+ { 2, 0, 0, -2, -2 },
+
+ /* 171-180 */
+ { 1, 1, -2, -4, -2 },
+ { 0, 1, 0, -2, -1 },
+ { 0, 0, 0, 4, 1 },
+ { 3, 0, 2, -2, 1 },
+ { 1, 0, 2, 4, 2 },
+ { 1, 1, -2, 0, -2 },
+ { 0, 0, 4, -2, 1 },
+ { 2, -2, 0, -2, 0 },
+ { 2, 1, 0, -2, -1 },
+ { 0, 2, 0, -2, 0 },
+
+ /* 181-190 */
+ { 1, 0, 0, -1, 1 },
+ { 1, 1, 2, 2, 2 },
+ { 3, 0, 0, 0, -1 },
+ { 2, 0, 0, -4, -1 },
+ { 3, 0, 2, 2, 2 },
+ { 0, 0, 2, 4, 1 },
+ { 0, 2, -2, -2, -2 },
+ { 1, -1, 0, -2, -1 },
+ { 0, 0, 2, -1, 1 },
+ { 2, 0, 0, 2, 1 },
+
+ /* 191-200 */
+ { 1, -1, -2, 2, -1 },
+ { 0, 0, 0, 2, -2 },
+ { 2, 0, 0, -4, 1 },
+ { 1, 0, 0, -4, 1 },
+ { 2, 0, 2, -4, 1 },
+ { 4, 0, 2, -2, 2 },
+ { 2, 1, -2, 0, -1 },
+ { 2, 1, -2, -4, -2 },
+ { 3, 0, 0, -4, 0 },
+ { 1, -1, 2, 2, 1 },
+
+ /* 201-210 */
+ { 1, -1, -2, 0, -1 },
+ { 0, 2, 0, 0, 1 },
+ { 1, 2, -2, -2, -2 },
+ { 1, 1, 0, -4, 0 },
+ { 2, 0, 0, -2, 2 },
+ { 0, 2, 2, -2, 1 },
+ { 1, 0, 2, 0, -1 },
+ { 2, 1, 0, -2, 1 },
+ { 2, -1, -2, 0, -1 },
+ { 1, -1, -2, -2, -1 },
+
+ /* 211-220 */
+ { 0, 1, -2, 1, -2 },
+ { 1, 0, -4, 2, -2 },
+ { 0, 1, 2, 2, 1 },
+ { 3, 0, 0, 0, 1 },
+ { 2, -1, 2, 2, 2 },
+ { 0, 1, -2, -4, -2 },
+ { 1, 0, -2, -3, -2 },
+ { 2, 0, 0, 0, 2 },
+ { 1, -1, 0, -2, -2 },
+ { 2, 0, -2, 2, -1 },
+
+ /* 221-230 */
+ { 0, 2, -2, 0, -2 },
+ { 3, 0, -2, 0, -1 },
+ { 2, -1, 2, 0, 1 },
+ { 1, 0, -2, -1, -2 },
+ { 0, 0, 2, 0, 3 },
+ { 2, 0, -4, 0, -2 },
+ { 2, 1, 0, -4, 0 },
+ { 1, 1, -2, 1, -1 },
+ { 0, 2, 2, 0, 2 },
+ { 1, -1, 2, -2, 2 },
+
+ /* 231-240 */
+ { 1, -1, 0, -2, 1 },
+ { 2, 1, 2, 0, 1 },
+ { 1, 0, 2, -4, 2 },
+ { 1, 1, -2, 0, -1 },
+ { 1, 1, 0, 2, 0 },
+ { 1, 0, 0, -3, 0 },
+ { 2, 0, 2, -1, 2 },
+ { 0, 2, 0, 0, -1 },
+ { 2, -1, 0, -2, 0 },
+ { 4, 0, 0, 0, 0 },
+
+ /* 241-250 */
+ { 2, 1, -2, -2, -2 },
+ { 0, 2, -2, 2, 0 },
+ { 1, 0, 2, 1, 1 },
+ { 1, 0, -1, 0, -3 },
+ { 3, -1, 2, 0, 2 },
+ { 2, 0, 2, -2, 0 },
+ { 1, -2, 0, 0, 0 },
+ { 2, 0, 0, 0, -2 },
+ { 1, 0, 0, 4, 0 },
+ { 0, 1, 0, 1, 1 },
+
+ /* 251-260 */
+ { 1, 0, 2, 2, 0 },
+ { 0, 1, 0, 2, -1 },
+ { 0, 1, 0, 1, -1 },
+ { 0, 0, 2, -2, 3 },
+ { 3, 1, 2, 0, 2 },
+ { 1, 1, 2, 1, 2 },
+ { 1, 1, -2, 2, -1 },
+ { 2, -1, 2, -2, 2 },
+ { 1, -2, 2, 0, 2 },
+ { 1, 0, 2, -4, 0 },
+
+ /* 261-270 */
+ { 0, 0, 1, 0, 0 },
+ { 1, 0, 2, -3, 1 },
+ { 1, -2, 0, -2, 0 },
+ { 2, 0, 0, 2, -1 },
+ { 1, 1, 2, -4, 1 },
+ { 4, 0, 2, 0, 1 },
+ { 0, 1, 2, 1, 1 },
+ { 1, 2, 2, -2, 2 },
+ { 2, 0, 2, 1, 2 },
+ { 2, 1, 2, -2, 1 },
+
+ /* 271-280 */
+ { 1, 0, 2, -1, 1 },
+ { 1, 0, 4, -2, 1 },
+ { 1, -1, 2, -2, 1 },
+ { 0, 1, 0, -4, 0 },
+ { 3, 0, -2, -2, -2 },
+ { 0, 0, 4, -4, 2 },
+ { 2, 0, -4, -2, -2 },
+ { 2, -2, 0, -2, -1 },
+ { 1, 0, 2, -2, -1 },
+ { 2, 0, -2, -6, -2 },
+
+ /* 281-290 */
+ { 1, 0, -2, 1, -2 },
+ { 1, 0, -2, 2, 1 },
+ { 1, -1, 0, 2, -1 },
+ { 1, 0, -2, 1, 0 },
+ { 2, -1, 0, -2, 1 },
+ { 1, -1, 0, 2, 1 },
+ { 2, 0, -2, -2, 0 },
+ { 1, 0, 2, -3, 2 },
+ { 0, 0, 0, 4, -1 },
+ { 2, -1, 0, 0, 1 },
+
+ /* 291-300 */
+ { 2, 0, 4, -2, 2 },
+ { 0, 0, 2, 3, 2 },
+ { 0, 1, 4, -2, 2 },
+ { 0, 1, -2, 2, 1 },
+ { 1, 1, 0, 2, 1 },
+ { 1, 0, 0, 4, 1 },
+ { 0, 0, 4, 0, 1 },
+ { 2, 0, 0, -3, 0 },
+ { 1, 0, 0, -1, -2 },
+ { 1, -2, -2, -2, -2 },
+
+ /* 301-310 */
+ { 3, 0, 0, 2, 0 },
+ { 2, 0, 2, -4, 2 },
+ { 1, 1, -2, -4, -1 },
+ { 1, 0, -2, -6, -2 },
+ { 2, -1, 0, 0, -1 },
+ { 2, -1, 0, 2, 0 },
+ { 0, 1, 2, -2, -1 },
+ { 1, 1, 0, 1, 0 },
+ { 1, 2, 0, -2, -1 },
+ { 1, 0, 0, 1, -1 },
+
+ /* 311-320 */
+ { 0, 0, 1, 0, 2 },
+ { 3, 1, 2, -2, 2 },
+ { 1, 0, -4, -2, -2 },
+ { 1, 0, 2, 4, 1 },
+ { 1, -2, 2, 2, 2 },
+ { 1, -1, -2, -4, -2 },
+ { 0, 0, 2, -4, 2 },
+ { 0, 0, 2, -3, 1 },
+ { 2, 1, -2, 0, 0 },
+ { 3, 0, -2, -2, -1 },
+
+ /* 321-330 */
+ { 2, 0, 2, 4, 2 },
+ { 0, 0, 0, 0, 3 },
+ { 2, -1, -2, -2, -2 },
+ { 2, 0, 0, -1, 0 },
+ { 3, 0, 2, -4, 2 },
+ { 2, 1, 2, 2, 2 },
+ { 0, 0, 3, 0, 3 },
+ { 1, 1, 2, 2, 1 },
+ { 2, 1, 0, 0, -1 },
+ { 1, 2, 0, -2, 1 },
+
+ /* 331-340 */
+ { 3, 0, 2, 2, 1 },
+ { 1, -1, -2, 2, -2 },
+ { 1, 1, 0, -1, 0 },
+ { 1, 2, 0, 0, 0 },
+ { 1, 0, 4, 0, 2 },
+ { 1, -1, 2, 4, 2 },
+ { 2, 1, 0, 0, 1 },
+ { 1, 0, 0, 2, 2 },
+ { 1, -1, -2, 2, 0 },
+ { 0, 2, -2, -2, -1 },
+
+ /* 341-350 */
+ { 2, 0, -2, 0, 2 },
+ { 5, 0, 2, 0, 2 },
+ { 3, 0, -2, -6, -2 },
+ { 1, -1, 2, -1, 2 },
+ { 3, 0, 0, -4, -1 },
+ { 1, 0, 0, 1, 1 },
+ { 1, 0, -4, 2, -1 },
+ { 0, 1, 2, -4, 1 },
+ { 1, 2, 2, 0, 2 },
+ { 0, 1, 0, -2, -2 },
+
+ /* 351-360 */
+ { 0, 0, 2, -1, 0 },
+ { 1, 0, 1, 0, 1 },
+ { 0, 2, 0, -2, 1 },
+ { 3, 0, 2, 0, 0 },
+ { 1, 1, -2, 1, 0 },
+ { 2, 1, -2, -4, -1 },
+ { 3, -1, 0, 0, 0 },
+ { 2, -1, -2, 0, 0 },
+ { 4, 0, 2, -2, 1 },
+ { 2, 0, -2, 2, 0 },
+
+ /* 361-370 */
+ { 1, 1, 2, -2, 0 },
+ { 1, 0, -2, 4, -1 },
+ { 1, 0, -2, -2, 1 },
+ { 2, 0, 2, -4, 0 },
+ { 1, 1, 0, -2, -2 },
+ { 1, 1, -2, -2, 0 },
+ { 1, 0, 1, -2, 1 },
+ { 2, -1, -2, -4, -2 },
+ { 3, 0, -2, 0, -2 },
+ { 0, 1, -2, -2, 0 },
+
+ /* 371-380 */
+ { 3, 0, 0, -2, -1 },
+ { 1, 0, -2, -3, -1 },
+ { 0, 1, 0, -4, -1 },
+ { 1, -2, 2, -2, 1 },
+ { 0, 1, -2, 1, -1 },
+ { 1, -1, 0, 0, 2 },
+ { 2, 0, 0, 1, 0 },
+ { 1, -2, 0, 2, 0 },
+ { 1, 2, -2, -2, -1 },
+ { 0, 0, 4, -4, 1 },
+
+ /* 381-390 */
+ { 0, 1, 2, 4, 2 },
+ { 0, 1, -4, 2, -2 },
+ { 3, 0, -2, 0, 0 },
+ { 2, -1, 2, 2, 1 },
+ { 0, 1, -2, -4, -1 },
+ { 4, 0, 2, 2, 2 },
+ { 2, 0, -2, -3, -2 },
+ { 2, 0, 0, -6, 0 },
+ { 1, 0, 2, 0, 3 },
+ { 3, 1, 0, 0, 0 },
+
+ /* 391-400 */
+ { 3, 0, 0, -4, 1 },
+ { 1, -1, 2, 0, 0 },
+ { 1, -1, 0, -4, 0 },
+ { 2, 0, -2, 2, -2 },
+ { 1, 1, 0, -2, 2 },
+ { 4, 0, 0, -2, 0 },
+ { 2, 2, 0, -2, 0 },
+ { 0, 1, 2, 0, 0 },
+ { 1, 1, 0, -4, 1 },
+ { 1, 0, 0, -4, -2 },
+
+ /* 401-410 */
+ { 0, 0, 0, 1, 2 },
+ { 3, 0, 0, 2, 1 },
+ { 1, 1, 0, -4, -1 },
+ { 0, 0, 2, 2, -1 },
+ { 1, 1, 2, 0, 0 },
+ { 1, -1, 2, -4, 1 },
+ { 1, 1, 0, 0, 2 },
+ { 0, 0, 2, 6, 2 },
+ { 4, 0, -2, -2, -1 },
+ { 2, 1, 0, -4, -1 },
+
+ /* 411-420 */
+ { 0, 0, 0, 3, 1 },
+ { 1, -1, -2, 0, 0 },
+ { 0, 0, 2, 1, 0 },
+ { 1, 0, 0, 2, -2 },
+ { 3, -1, 2, 2, 2 },
+ { 3, -1, 2, -2, 2 },
+ { 1, 0, 0, -1, 2 },
+ { 1, -2, 2, -2, 2 },
+ { 0, 1, 0, 2, 2 },
+ { 0, 1, -2, -1, -2 },
+
+ /* 421-430 */
+ { 1, 1, -2, 0, 0 },
+ { 0, 2, 2, -2, 0 },
+ { 3, -1, -2, -1, -2 },
+ { 1, 0, 0, -6, 0 },
+ { 1, 0, -2, -4, 0 },
+ { 2, 1, 0, -4, 1 },
+ { 2, 0, 2, 0, -1 },
+ { 2, 0, -4, 0, -1 },
+ { 0, 0, 3, 0, 2 },
+ { 2, 1, -2, -2, -1 },
+
+ /* 431-440 */
+ { 1, -2, 0, 0, 1 },
+ { 2, -1, 0, -4, 0 },
+ { 0, 0, 0, 3, 0 },
+ { 5, 0, 2, -2, 2 },
+ { 1, 2, -2, -4, -2 },
+ { 1, 0, 4, -4, 2 },
+ { 0, 0, 4, -1, 2 },
+ { 3, 1, 0, -4, 0 },
+ { 3, 0, 0, -6, 0 },
+ { 2, 0, 0, 2, 2 },
+
+ /* 441-450 */
+ { 2, -2, 2, 0, 2 },
+ { 1, 0, 0, -3, 1 },
+ { 1, -2, -2, 0, -2 },
+ { 1, -1, -2, -3, -2 },
+ { 0, 0, 2, -2, -2 },
+ { 2, 0, -2, -4, 0 },
+ { 1, 0, -4, 0, 0 },
+ { 0, 1, 0, -1, 0 },
+ { 4, 0, 0, 0, -1 },
+ { 3, 0, 2, -1, 2 },
+
+ /* 451-460 */
+ { 3, -1, 2, 0, 1 },
+ { 2, 0, 2, -1, 1 },
+ { 1, 2, 2, -2, 1 },
+ { 1, 1, 0, 2, -1 },
+ { 0, 2, 2, 0, 1 },
+ { 3, 1, 2, 0, 1 },
+ { 1, 1, 2, 1, 1 },
+ { 1, 1, 0, -1, 1 },
+ { 1, -2, 0, -2, -1 },
+ { 4, 0, 0, -4, 0 },
+
+ /* 461-470 */
+ { 2, 1, 0, 2, 0 },
+ { 1, -1, 0, 4, 0 },
+ { 0, 1, 0, -2, 2 },
+ { 0, 0, 2, 0, -2 },
+ { 1, 0, -1, 0, 1 },
+ { 3, 0, 2, -2, 0 },
+ { 2, 0, 2, 2, 0 },
+ { 1, 2, 0, -4, 0 },
+ { 1, -1, 0, -3, 0 },
+ { 0, 1, 0, 4, 0 },
+
+ /* 471 - 480 */
+ { 0, 1, -2, 0, 0 },
+ { 2, 2, 2, -2, 2 },
+ { 0, 0, 0, 1, -2 },
+ { 0, 2, -2, 0, -1 },
+ { 4, 0, 2, -4, 2 },
+ { 2, 0, -4, 2, -2 },
+ { 2, -1, -2, 0, -2 },
+ { 1, 1, 4, -2, 2 },
+ { 1, 1, 2, -4, 2 },
+ { 1, 0, 2, 3, 2 },
+
+ /* 481-490 */
+ { 1, 0, 0, 4, -1 },
+ { 0, 0, 0, 4, 2 },
+ { 2, 0, 0, 4, 0 },
+ { 1, 1, -2, 2, 0 },
+ { 2, 1, 2, 1, 2 },
+ { 2, 1, 2, -4, 1 },
+ { 2, 0, 2, 1, 1 },
+ { 2, 0, -4, -2, -1 },
+ { 2, 0, -2, -6, -1 },
+ { 2, -1, 2, -1, 2 },
+
+ /* 491-500 */
+ { 1, -2, 2, 0, 1 },
+ { 1, -2, 0, -2, 1 },
+ { 1, -1, 0, -4, -1 },
+ { 0, 2, 2, 2, 2 },
+ { 0, 2, -2, -4, -2 },
+ { 0, 1, 2, 3, 2 },
+ { 0, 1, 0, -4, 1 },
+ { 3, 0, 0, -2, 1 },
+ { 2, 1, -2, 0, 1 },
+ { 2, 0, 4, -2, 1 },
+
+ /* 501-510 */
+ { 2, 0, 0, -3, -1 },
+ { 2, -2, 0, -2, 1 },
+ { 2, -1, 2, -2, 1 },
+ { 1, 0, 0, -6, -1 },
+ { 1, -2, 0, 0, -1 },
+ { 1, -2, -2, -2, -1 },
+ { 0, 1, 4, -2, 1 },
+ { 0, 0, 2, 3, 1 },
+ { 2, -1, 0, -1, 0 },
+ { 1, 3, 0, -2, 0 },
+
+ /* 511-520 */
+ { 0, 3, 0, -2, 0 },
+ { 2, -2, 2, -2, 2 },
+ { 0, 0, 4, -2, 0 },
+ { 4, -1, 2, 0, 2 },
+ { 2, 2, -2, -4, -2 },
+ { 4, 1, 2, 0, 2 },
+ { 4, -1, -2, -2, -2 },
+ { 2, 1, 0, -2, -2 },
+ { 2, 1, -2, -6, -2 },
+ { 2, 0, 0, -1, 1 },
+
+ /* 521-530 */
+ { 2, -1, -2, 2, -1 },
+ { 1, 1, -2, 2, -2 },
+ { 1, 1, -2, -3, -2 },
+ { 1, 0, 3, 0, 3 },
+ { 1, 0, -2, 1, 1 },
+ { 1, 0, -2, 0, 2 },
+ { 1, -1, 2, 1, 2 },
+ { 1, -1, 0, 0, -2 },
+ { 1, -1, -4, 2, -2 },
+ { 0, 3, -2, -2, -2 },
+
+ /* 531-540 */
+ { 0, 1, 0, 4, 1 },
+ { 0, 0, 4, 2, 2 },
+ { 3, 0, -2, -2, 0 },
+ { 2, -2, 0, 0, 0 },
+ { 1, 1, 2, -4, 0 },
+ { 1, 1, 0, -3, 0 },
+ { 1, 0, 2, -3, 0 },
+ { 1, -1, 2, -2, 0 },
+ { 0, 2, 0, 2, 0 },
+ { 0, 0, 2, 4, 0 },
+
+ /* 541-550 */
+ { 1, 0, 1, 0, 0 },
+ { 3, 1, 2, -2, 1 },
+ { 3, 0, 4, -2, 2 },
+ { 3, 0, 2, 1, 2 },
+ { 3, 0, 0, 2, -1 },
+ { 3, 0, 0, 0, 2 },
+ { 3, 0, -2, 2, -1 },
+ { 2, 0, 4, -4, 2 },
+ { 2, 0, 2, -3, 2 },
+ { 2, 0, 0, 4, 1 },
+
+ /* 551-560 */
+ { 2, 0, 0, -3, 1 },
+ { 2, 0, -4, 2, -1 },
+ { 2, 0, -2, -2, 1 },
+ { 2, -2, 2, 2, 2 },
+ { 2, -2, 0, -2, -2 },
+ { 2, -1, 0, 2, 1 },
+ { 2, -1, 0, 2, -1 },
+ { 1, 1, 2, 4, 2 },
+ { 1, 1, 0, 1, 1 },
+ { 1, 1, 0, 1, -1 },
+
+ /* 561-570 */
+ { 1, 1, -2, -6, -2 },
+ { 1, 0, 0, -3, -1 },
+ { 1, 0, -4, -2, -1 },
+ { 1, 0, -2, -6, -1 },
+ { 1, -2, 2, 2, 1 },
+ { 1, -2, -2, 2, -1 },
+ { 1, -1, -2, -4, -1 },
+ { 0, 2, 0, 0, 2 },
+ { 0, 1, 2, -4, 2 },
+ { 0, 1, -2, 4, -1 },
+
+ /* 571-580 */
+ { 5, 0, 0, 0, 0 },
+ { 3, 0, 0, -3, 0 },
+ { 2, 2, 0, -4, 0 },
+ { 1, -1, 2, 2, 0 },
+ { 0, 1, 0, 3, 0 },
+ { 4, 0, -2, 0, -1 },
+ { 3, 0, -2, -6, -1 },
+ { 3, 0, -2, -1, -1 },
+ { 2, 1, 2, 2, 1 },
+ { 2, 1, 0, 2, 1 },
+
+ /* 581-590 */
+ { 2, 0, 2, 4, 1 },
+ { 2, 0, 2, -6, 1 },
+ { 2, 0, 2, -2, -1 },
+ { 2, 0, 0, -6, -1 },
+ { 2, -1, -2, -2, -1 },
+ { 1, 2, 2, 0, 1 },
+ { 1, 2, 0, 0, 1 },
+ { 1, 0, 4, 0, 1 },
+ { 1, 0, 2, -6, 1 },
+ { 1, 0, 2, -4, -1 },
+
+ /* 591-600 */
+ { 1, 0, -1, -2, -1 },
+ { 1, -1, 2, 4, 1 },
+ { 1, -1, 2, -3, 1 },
+ { 1, -1, 0, 4, 1 },
+ { 1, -1, -2, 1, -1 },
+ { 0, 1, 2, -2, 3 },
+ { 3, 0, 0, -2, 0 },
+ { 1, 0, 1, -2, 0 },
+ { 0, 2, 0, -4, 0 },
+ { 0, 0, 2, -4, 0 },
+
+ /* 601-610 */
+ { 0, 0, 1, -1, 0 },
+ { 0, 0, 0, 6, 0 },
+ { 0, 2, 0, 0, -2 },
+ { 0, 1, -2, 2, -3 },
+ { 4, 0, 0, 2, 0 },
+ { 3, 0, 0, -1, 0 },
+ { 3, -1, 0, 2, 0 },
+ { 2, 1, 0, 1, 0 },
+ { 2, 1, 0, -6, 0 },
+ { 2, -1, 2, 0, 0 },
+
+ /* 611-620 */
+ { 1, 0, 2, -1, 0 },
+ { 1, -1, 0, 1, 0 },
+ { 1, -1, -2, -2, 0 },
+ { 0, 1, 2, 2, 0 },
+ { 0, 0, 2, -3, 0 },
+ { 2, 2, 0, -2, -1 },
+ { 2, -1, -2, 0, 1 },
+ { 1, 2, 2, -4, 1 },
+ { 0, 1, 4, -4, 2 },
+ { 0, 0, 0, 3, 2 },
+
+ /* 621-630 */
+ { 5, 0, 2, 0, 1 },
+ { 4, 1, 2, -2, 2 },
+ { 4, 0, -2, -2, 0 },
+ { 3, 1, 2, 2, 2 },
+ { 3, 1, 0, -2, 0 },
+ { 3, 1, -2, -6, -2 },
+ { 3, 0, 0, 0, -2 },
+ { 3, 0, -2, -4, -2 },
+ { 3, -1, 0, -3, 0 },
+ { 3, -1, 0, -2, 0 },
+
+ /* 631-640 */
+ { 2, 1, 2, 0, 0 },
+ { 2, 1, 2, -4, 2 },
+ { 2, 1, 2, -2, 0 },
+ { 2, 1, 0, -3, 0 },
+ { 2, 1, -2, 0, -2 },
+ { 2, 0, 0, -4, 2 },
+ { 2, 0, 0, -4, -2 },
+ { 2, 0, -2, -5, -2 },
+ { 2, -1, 2, 4, 2 },
+ { 2, -1, 0, -2, 2 },
+
+ /* 641-650 */
+ { 1, 3, -2, -2, -2 },
+ { 1, 1, 0, 0, -2 },
+ { 1, 1, 0, -6, 0 },
+ { 1, 1, -2, 1, -2 },
+ { 1, 1, -2, -1, -2 },
+ { 1, 0, 2, 1, 0 },
+ { 1, 0, 0, 3, 0 },
+ { 1, 0, 0, -4, 2 },
+ { 1, 0, -2, 4, -2 },
+ { 1, -2, 0, -1, 0 },
+
+ /* 651-NFLS */
+ { 0, 1, -4, 2, -1 },
+ { 1, 0, -2, 0, -3 },
+ { 0, 0, 4, -4, 4 }
+ };
+
+/* Number of frequencies: luni-solar */
+ static const int NFLS = (int) (sizeof mfals / sizeof (int) / 5);
+
+/* Fundamental-argument multipliers: planetary terms */
+ static const int mfapl[][14] = {
+
+ /* 1-10 */
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, -2, 5, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, -5, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 3, -5, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 1, -1, 1, 0, -8, 12, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -8, 3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 1, -1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 8,-16, 4, 5, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -1, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, -1, 2, 0, 0, 0, 0, 0 },
+
+ /* 11-20 */
+ { 0, 0, 0, 0, 0, 0, 8,-13, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 2, -5, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, -5, 6, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 4, -6, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, -1, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, -8, 3, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 2, -4, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 6, -8, 3, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, -2, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 2, -3, 0, 0, 0, 0, 0, 0 },
+
+ /* 21-30 */
+ { 0, 0, 0, 0, 0, 0, 2, -2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 1, 0, 0, -4, 8, -3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, 4, -8, 3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, -5, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 1, 1, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 1, -1, 1, 0, 0, 0, -2, 0, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, -1, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 1 },
+ { 2, 0, 0, -2, 0, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+
+ /* 31-40 */
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, -2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 8,-13, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 1, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 5, -8, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, -2, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, -5, 0, 0, 1 },
+ { 2, 0, 0, -2, 0, 0, 0, -2, 0, 3, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, -1, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 3, -4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 0, -1, 0, 0, 0 },
+
+ /* 41-50 */
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 5, -7, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 1, -1, 0, 0, 0, 0, -2, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, 0, -2, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 8,-13, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 2, -1, 0, 0, 0, 0, 0, 2 },
+ { 1, 0, 0, 0, 0, 0,-18, 16, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 1, 0, 0, 0, 2 },
+
+ /* 51-60 */
+ { 0, 0, 1, -1, 1, 0, -5, 7, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, 0, 0, 0,-10, 3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 0, 0, -5, 6, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, -1, 0, 0, 0, 2 },
+ { 1, 0, 2, 0, 2, 0, 0, 1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -2, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 1 },
+ { 1, 0, -2, 0, -2, 0, 0, 4, -8, 3, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 0, 2, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, -3, 3, 0, 0, 0, 0, 0, 0 },
+
+ /* 61-70 */
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 8,-16, 4, 5, 0, 0, -2 },
+ { 0, 0, 1, -1, 1, 0, 0, 3, -8, 3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 8,-11, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 8,-16, 4, 5, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 1, -1, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 4, -6, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -3, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, -4, 0, 0, 0, 0, 0 },
+
+ /* 71-80 */
+ { 0, 0, 0, 0, 0, 0, 6, -8, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 3, -2, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 8,-15, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 2, -5, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 1, -3, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, -2, 0, 0, 0, 2 },
+ { 0, 0, 1, -1, 1, 0, 0, -5, 8, -3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 2, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -2, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 3, -5, 0, 0, 0, 0, 0, 0 },
+
+ /* 81-90 */
+ { 2, 0, 0, -2, 1, 0, 0, -2, 0, 3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 5, -8, 0, 0, 0, 0, 0, -1 },
+ { 2, 0, 0, -2, 0, 0, -3, 3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 8,-13, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, 0, 0, -2, 5, 0, 0, 0 },
+ { 1, 0, 0, -1, 0, 0, -3, 4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 2 },
+ { 1, 0, 0, 0, -1, 0,-18, 16, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, 0, 0, 2, -5, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, 0, 0, 1, 0, 0, 0, 0 },
+
+ /* 91-100 */
+ { 1, 0, 0, -2, 0, 0, 19,-21, 3, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, -8, 13, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 0, 1, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 7, -9, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 2 },
+ { 1, 0, 0, 0, 1, 0,-18, 16, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 2, -4, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 6,-16, 4, 5, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 4, -7, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 3, -7, 0, 0, 0, 0, 0, -2 },
+
+ /* 101-110 */
+ { 0, 0, 0, 0, 0, 0, 2, -2, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 1 },
+ { 2, 0, 0, -2, 1, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -4, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 1, -2, 0, 0, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, -1, 0, 0, -2, 0, 3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 3, -3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 2, 0, 0, 0, 2 },
+
+ /* 111-120 */
+ { 0, 0, 0, 0, 1, 0, 0, 1, -2, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 2 },
+ { 0, 0, 2, -2, 1, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, -3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 3, -5, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 3, -3, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 4, -4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, 0, -1, 0, -1, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, 0, 0, -6, 8, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -2, 2, 0, 0, 0, 0, 0 },
+
+ /* 121-130 */
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 1 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 1, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, -2, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, -3, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, -4, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, -1, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 8,-10, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 1, -1, 1, 0, -3, 4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 6, -9, 0, 0, 0, 0, 0, -2 },
+ { 1, 0, 0, -1, 1, 0, 0, -1, 0, 2, 0, 0, 0, 0 },
+
+ /* 131-140 */
+ { 0, 0, 0, 0, 0, 0, 5, -7, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 5, -5, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 3, -3, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 4, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, 0, -3, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 1, -1, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 1, 0, 2, -3, 0, 0, 0, 0, 0, 0 },
+
+ /* 141-150 */
+ { 1, 0, 0, -1, 0, 0, 0, -1, 0, 1, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 1, -3, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -4, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -4, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 9,-11, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 2, -3, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 8,-15, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, -4, 5, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 4, -6, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, 0, -1, 0, 0, 0, 2 },
+
+ /* 151-160 */
+ { 1, 0, 0, -1, 1, 0, -3, 4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, 1, 1, 0, 0, 1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, -4, 10, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 1, -1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, 0, -1, 0, 0, -1, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 3, -1, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -4, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, -5, 0, 0, -2 },
+ { 0, 0, 2, -2, 1, 0, -4, 4, 0, 0, 0, 0, 0, 0 },
+
+ /* 161-170 */
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, -1, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -3, 0, 0, 0, 0, 2 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 0, 0, 0, 2, 0 },
+ { 0, 0, 0, 0, 0, 0, 4, -4, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, -4, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 5, -8, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, -2, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 1, 0, 0, 0, 0, 0, 1, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0, -9, 13, 0, 0, 0, 0, 0 },
+ { 2, 0, 2, 0, 2, 0, 0, 2, 0, -3, 0, 0, 0, 0 },
+
+ /* 171-180 */
+ { 0, 0, 0, 0, 0, 0, 3, -6, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 1, -1, 2, 0, 0, -1, 0, 0, 2, 0, 0, 0 },
+ { 1, 0, 0, -1, -1, 0, -3, 4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -6, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 6, -6, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, 0, 1 },
+ { 1, 0, 2, 0, 1, 0, 0, -2, 0, 3, 0, 0, 0, 0 },
+ { 1, 0, -2, 0, -1, 0, 0, -1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, -2, 4, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -5, 0, 0, 0, 0, 0 },
+
+ /* 181-190 */
+ { 0, 0, 0, 0, 0, 0, 2, 1, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 1, 1, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 2, 0, 2, 0, 0, 1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, -8, 3, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 6,-10, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 7, -8, 3, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 1, 0, -3, 5, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, -1, 0, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, -5, 7, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, -2, 0, 0, 0, 1 },
+
+ /* 191-200 */
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, -1, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 7,-10, 0, 0, 0, 0, 0, -2 },
+ { 1, 0, 0, -2, 0, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 2, -5, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 6, -8, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 1, -1, 1, 0, 0, -9, 15, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, -2, 3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, -1, 1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -6, 0, 0, 0, 0, 0 },
+
+ /* 201-210 */
+ { 0, 0, 0, 0, 0, 0, 0, 1, -4, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, -1, 0, 0, 2 },
+ { 2, 0, 0, -2, 1, 0, -6, 8, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 5, -5, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 1, -1, 1, 0, 3, -6, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, -2, 2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 8,-14, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 0, 0, 0 },
+
+ /* 211-220 */
+ { 0, 0, 0, 0, 1, 0, 0, 8,-15, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -6, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 7, -7, 0, 0, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, 1, 0, -3, 3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -1, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 1, 0, 0, 2 },
+ { 2, 0, -1, -1, 0, 0, 0, 3, -7, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -7, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -3, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -3, 4, 0, 0, 0, 0, 0 },
+
+ /* 221-230 */
+ { 2, 0, 0, -2, 0, 0, 0, -6, 8, 0, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, 0, 0, 0, -5, 6, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, 0, 0, -1, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 2, 1, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 1, 2, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 1, 0, 0, 1, 0, -1, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, -1, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 3, -9, 4, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -5, 0, 0, 0, 0, -2 },
+
+ /* 231-240 */
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, -4, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 1 },
+ { 0, 0, 0, 0, 0, 0, 7,-11, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 3, -5, 4, 0, 0, 0, 0, 2 },
+ { 0, 0, 1, -1, 0, 0, 0, -1, 0, -1, 1, 0, 0, 0 },
+ { 2, 0, 0, 0, 0, 0, 0, -2, 0, 3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 8,-15, 0, 0, 0, 0, -2 },
+ { 0, 0, 1, -1, 2, 0, 0, -2, 2, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 6, -6, 0, 0, 0, 0, 0, -1 },
+
+ /* 241-250 */
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, -1, 1, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 2, -2, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -7, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -8, 3, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 2, -4, 0, -3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 3, -5, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, -3, 0, 0, 0, 2 },
+ { 0, 0, 2, -2, 2, 0, -8, 11, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -8, 3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, -2, 0, 0, 0 },
+
+ /* 251-260 */
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 1, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -9, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -5, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 7, -9, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 4, -7, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 2, -1, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, -2, -2, -2, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 1, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, -2, 5, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 3, -3, 0, 0, 0, 0, 0, 1 },
+
+ /* 261-270 */
+ { 0, 0, 0, 0, 0, 0, 0, 6, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 2, -5, 0, 0, 2 },
+ { 2, 0, 0, -2, -1, 0, 0, -2, 0, 0, 5, 0, 0, 0 },
+ { 2, 0, 0, -2, -1, 0, -6, 8, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, -2, 0, 0, -3, 3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 8, -8, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, 2, -5, 0, 0, 2 },
+ { 0, 0, 0, 0, 1, 0, 3, -7, 4, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, -2, 2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, -1, 0, 1, 0, 0, 0, 0 },
+
+ /* 271-280 */
+ { 0, 0, 1, -1, 0, 0, 0, -1, 0, -2, 5, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, -3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 3, -1, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 2, -3, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 11, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 6,-15, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, 1, 0, 0, 0, 2 },
+ { 1, 0, 0, -1, 0, 0, 0, -3, 4, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, -3, 7, -4, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, 0, -2, 0, 0, 0, 2 },
+
+ /* 281-290 */
+ { 0, 0, 0, 0, 0, 0, 3, -5, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 2, -2, 2, 0, -5, 6, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 2, 0, -3, 3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 3, 0, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 6, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 4, -4, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -8, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -5, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 5, -7, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 6,-11, 0, 0, 0, 0, -2 },
+
+ /* 291-300 */
+ { 0, 0, 0, 0, 0, 0, 0, 1, -3, 0, 0, 0, 0, -2 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 3, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, 0, -1, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 1, -2, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 9,-12, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 4, -4, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 1, -1, 0, 0, -8, 12, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, -2, 3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 7, -7, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -6, 0, 0, 0, 0, -1 },
+
+ /* 301-310 */
+ { 0, 0, 0, 0, 0, 0, 0, 6, -6, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 1, 0, -4, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 1, -1, 1, 0, 0, 1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 6, -9, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 1, -1, -1, 0, 0, 0, -2, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, -5, 0, 0, 0, 0, -2 },
+ { 2, 0, 0, -2, 0, 0, 0, -2, 0, 3, -1, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, -2, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -9, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 5, -6, 0, 0, 0, 0, 0, 2 },
+
+ /* 311-320 */
+ { 0, 0, 0, 0, 0, 0, 9, -9, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 0, 3, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, 2, -4, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 5, -3, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, 1 },
+ { 0, 0, 1, -1, 2, 0, 0, -1, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 5, -9, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -3, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 4, 0, 0, 0, 2 },
+ { 0, 0, 2, 0, 2, 0, 0, 4, -8, 3, 0, 0, 0, 0 },
+
+ /* 321-330 */
+ { 0, 0, 2, 0, 2, 0, 0, -4, 8, -3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, 0, -3, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 1, 0, 0, 0, 0 },
+ { 2, 0, -1, -1, -1, 0, 0, -1, 0, 3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 4, -3, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 4, -2, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 5,-10, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 8,-13, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 2, -2, 1, -1, 0, 2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 0, 0, 2, 0, 0 },
+
+ /* 331-340 */
+ { 0, 0, 0, 0, 1, 0, 3, -5, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, -2, 0, 0, 0, -2, 0, 3, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 0, 0, -3, 3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 9, -9, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, 0, 2, 0, 1, -1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0, -8, 11, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0, -2, 0, 0, 2, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, -1, 2, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 5, -5, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 2, -6, 0, 0, 0, 0, 0, -2 },
+
+ /* 341-350 */
+ { 0, 0, 0, 0, 0, 0, 0, 8,-15, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -2, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 7,-13, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, -2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 3, 0, 0, 0, 2 },
+ { 0, 0, 2, -2, 1, 0, 0, -2, 0, 3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 8, -8, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 8,-10, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 4, -2, 0, 0, 0, 0, 0, 1 },
+
+ /* 351-360 */
+ { 0, 0, 0, 0, 0, 0, 3, -6, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 3, -4, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, -5, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, -4, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, -1, 0, 0, -5, 6, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, -5, 0, 0, 0, 0, -2 },
+ { 2, 0, -1, -1, -1, 0, 0, 3, -7, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -8, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, 0, 2, 0, -1, 1, 0, 0, 0, 0, 0, 0 },
+
+ /* 361-370 */
+ { 2, 0, 0, -2, 0, 0, 0, -2, 0, 4, -3, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 6,-11, 0, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, 1, 0, 0, -6, 8, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -8, 1, 5, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 6, -5, 0, 0, 0, 0, 2 },
+ { 1, 0, -2, -2, -2, 0, -3, 3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 2, 0, 0, 0, -2, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 2, 0, 0, 4, -8, 3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 2, 0, 0, -4, 8, -3, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 6, 0, 0, 0, 0, 0, 1 },
+
+ /* 371-380 */
+ { 0, 0, 0, 0, 0, 0, 0, 6, -7, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, 0, 0, -2, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, -2, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -1, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, -6, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 4, -5, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 3, -5, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 7,-13, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, -2, 0, 0, 0, 2 },
+
+ /* 381-390 */
+ { 0, 0, 1, -1, 0, 0, 0, -1, 0, 0, 2, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, -8, 15, 0, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, -2, 0, -3, 3, 0, 0, 0, 0, 0, 0 },
+ { 2, 0, -1, -1, -1, 0, 0, -1, 0, 2, 0, 0, 0, 0 },
+ { 1, 0, 2, -2, 2, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+ { 1, 0, -1, 1, -1, 0,-18, 17, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, 0, 2, 0, 0, 1, 0, -1, 0, 0, 0, 0 },
+ { 0, 0, 2, 0, 2, 0, 0, -1, 0, 1, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, -1, 0, -5, 6, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 2, 0, 0, -1, 0, 1, 0, 0, 0, 0 },
+
+ /* 391-400 */
+ { 0, 0, 0, 0, 1, 0, 2, -2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 8,-16, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 5, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 2 },
+ { 0, 0, 0, 0, 2, 0, 0, -1, 2, 0, 0, 0, 0, 0 },
+ { 2, 0, -1, -1, -2, 0, 0, -1, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 6,-10, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, -2, 4, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 2, 0, 0, 0, 0, 2 },
+ { 2, 0, 0, -2, -1, 0, 0, -2, 0, 4, -5, 0, 0, 0 },
+
+ /* 401-410 */
+ { 2, 0, 0, -2, -1, 0, -3, 3, 0, 0, 0, 0, 0, 0 },
+ { 2, 0, -1, -1, -1, 0, 0, -1, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 1, -1, 1, 0, 0, -1, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, -1, -1, 0, 0, -2, 2, 0, 0, 0, 0, 0 },
+ { 1, 0, -1, -1, -1, 0, 20,-20, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0, -1, 0, 1, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 1, -2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, -2, 1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 5, -8, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, 0, 0, 0, -1, 0, 0, 0 },
+
+ /* 411-420 */
+ { 0, 0, 0, 0, 0, 0, 9,-11, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 5, -3, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -3, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 6, -7, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -2, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 1, -2, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 0, -2, 0, 0, 0 },
+ { 0, 0, 1, -1, 2, 0, 0, -1, 0, -2, 5, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -7, 0, 0, 0, 0, 0 },
+
+ /* 421-430 */
+ { 0, 0, 0, 0, 0, 0, 1, -3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -8, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, -6, 0, 0, 0, 0, -2 },
+ { 1, 0, 0, -2, 0, 0, 20,-21, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 8,-12, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 5, -6, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -4, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 2, 0, 0, -1, 0, -1, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 8,-12, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 9,-17, 0, 0, 0, 0, 0 },
+
+ /* 431-440 */
+ { 0, 0, 0, 0, 0, 0, 0, 5, -6, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -8, 1, 5, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -6, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, -7, 0, 0, 0, 0, -2 },
+ { 1, 0, 0, -1, 1, 0, 0, -3, 4, 0, 0, 0, 0, 0 },
+ { 1, 0, -2, 0, -2, 0,-10, 3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, -9, 17, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 1, -4, 0, 0, 0, 0, 0, -2 },
+ { 1, 0, -2, -2, -2, 0, 0, -2, 0, 3, 0, 0, 0, 0 },
+ { 1, 0, -1, 1, -1, 0, 0, 1, 0, 0, 0, 0, 0, 0 },
+
+ /* 441-450 */
+ { 0, 0, 2, -2, 2, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 2, 0, 0, -1, 0, 0, 1, 0, 0, 0 },
+ { 0, 0, 1, -1, 2, 0, -5, 7, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, 2, -2, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 4, -5, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 3, -4, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 2, -4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 5,-10, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, 0, -4, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, -5, 0, 0, 0, -2 },
+
+ /* 451-460 */
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -5, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -2, 5, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -2, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 2, -3, 0, 0, 0, 0, 0, 1 },
+ { 1, 0, 0, -2, 0, 0, 0, 1, 0, -1, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 3, -7, 4, 0, 0, 0, 0, 0 },
+ { 2, 0, 2, 0, 1, 0, 0, 1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, -1, 0, 0, -1, 0, -1, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, 1, 0, -2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 6,-10, 0, 0, 0, 0, -2 },
+
+ /* 461-470 */
+ { 1, 0, 0, -1, 1, 0, 0, -1, 0, 1, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0, 4, -8, 3, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0, 1, 0, -1, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0, -4, 8, -3, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0, -3, 0, 3, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, -5, 5, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 1, -3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -4, 6, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 0, 0, -1, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, -5, 6, 0, 0, 0, 0, 0, 0 },
+
+ /* 471-480 */
+ { 0, 0, 0, 0, 1, 0, 3, -4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, -2, 2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 7,-10, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 5, -5, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 4, -5, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 3, -8, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 2, -5, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 1, -2, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 7, -9, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 7, -8, 0, 0, 0, 0, 2 },
+
+ /* 481-490 */
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -8, 3, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, -2, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, -4, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -1, 0, 0, 0, -1 },
+ { 2, 0, 0, -2, -1, 0, 0, -6, 8, 0, 0, 0, 0, 0 },
+ { 2, 0, -1, -1, 1, 0, 0, 3, -7, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0, -7, 9, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -5, 0, 0, 0, 0, -1 },
+
+ /* 491-500 */
+ { 0, 0, 1, -1, 2, 0, -8, 12, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, 0, 0, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+ { 1, 0, 0, -2, 0, 0, 2, -2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 7, -8, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, 1, 0, 0, -5, 6, 0, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, -1, 0, 0, -2, 0, 3, -1, 0, 0, 0 },
+ { 1, 0, 1, 1, 1, 0, 0, 1, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, -2, 1, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+ { 1, 0, 0, -2, -1, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+
+ /* 501-510 */
+ { 1, 0, 0, -1, -1, 0, 0, -3, 4, 0, 0, 0, 0, 0 },
+ { 1, 0, -1, 0, -1, 0, -3, 5, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0, -4, 4, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0, -2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, -8, 11, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 0, 0, 0, -9, 13, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, 1, 2, 0, 0, 1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, 1, -4, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, 0, -1, 0, 1, -3, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, 7,-13, 0, 0, 0, 0, 0 },
+
+ /* 511-520 */
+ { 0, 0, 0, 0, 1, 0, 0, 2, 0, -2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, -2, 2, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, -3, 4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 1, 0, -4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 7,-11, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 6, -6, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 6, -4, 0, 0, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 5, -6, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 4, -2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 3, -4, 0, 0, 0, 0, 0, 1 },
+
+ /* 521-530 */
+ { 0, 0, 0, 0, 0, 0, 1, -4, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 9,-17, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 7, -7, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -8, 3, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -8, 3, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -8, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, -7, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 1, 0, 0, 0, 1 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -4, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, 0, 0, 0, -4, 8, -3, 0, 0, 0, 0 },
+
+ /* 531-540 */
+ { 2, 0, 0, -2, 0, 0, -2, 2, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, 0, 0, 0, 0, 4, -8, 3, 0, 0, 0, 0 },
+ { 1, 0, 0, 0, 0, 0, 0, -4, 8, -3, 0, 0, 0, 0 },
+ { 1, 0, 0, 0, 0, 0, -1, 1, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, -2, 0, 0, 17,-16, 0, -2, 0, 0, 0, 0 },
+ { 1, 0, 0, -1, 0, 0, 0, -2, 2, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 0, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 6, -9, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, -4, 0, 0, 0, 0 },
+
+ /* 541-550 */
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, -2, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 1, 0, 0, 0, 0, 2 },
+ { 2, 0, 0, -2, 0, 0, 0, -4, 4, 0, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, 0, 0, 0, -2, 0, 2, 2, 0, 0, 0 },
+ { 1, 0, 0, 0, 0, 0, 1, -1, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, 0, 0, 0, 0, -1, 0, 1, 0, 0, 0, 0 },
+ { 1, 0, 0, 0, 0, 0, -3, 3, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, -2, 0, 0, 1, -1, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, -2, 0, 0, 0, 4, -8, 3, 0, 0, 0, 0 },
+ { 1, 0, 0, -2, 0, 0, 0, -4, 8, -3, 0, 0, 0, 0 },
+
+ /* 551-560 */
+ { 1, 0, 0, -2, 0, 0, -2, 2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 0, 0, -4, 4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, 1, 0, 0, 0, 1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, 3, -6, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, 0, -2, 2, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, 0, -1, 0, 1, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, 0, -1, 0, 0, 1, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, -4, 5, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, -3, 4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 2, 0, 0, 0, -1, 0, 1, 0, 0, 0, 0 },
+
+ /* 561-570 */
+ { 0, 0, 0, 0, 0, 0, 8, -9, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 3, -6, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 1, 1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 3, -5, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, -2, 0, 0, 0 },
+ { 2, 0, -2, -2, -2, 0, 0, -2, 0, 2, 0, 0, 0, 0 },
+ { 1, 0, 0, 0, 1, 0,-10, 3, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, 0, -1, 0,-10, 3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, 0, 2, 0, 2, -3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, 0, 2, 0, 2, -2, 0, 0, 0, 0, 0, 0 },
+
+ /* 571-580 */
+ { 0, 0, 2, 0, 2, 0, -2, 3, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, 0, 2, 0, -2, 2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 2, 0, 0, 0, 0, 1, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, 0, -1, 0, 2, 0, 0, 0, 0 },
+ { 2, 0, 2, -2, 2, 0, 0, -2, 0, 3, 0, 0, 0, 0 },
+ { 2, 0, 1, -3, 1, 0, -6, 7, 0, 0, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, 0, 0, 2, -5, 0, 0, 0, 0, 0, 0 },
+ { 2, 0, 0, -2, 0, 0, 0, -2, 0, 5, -5, 0, 0, 0 },
+ { 2, 0, 0, -2, 0, 0, 0, -2, 0, 1, 5, 0, 0, 0 },
+ { 2, 0, 0, -2, 0, 0, 0, -2, 0, 0, 5, 0, 0, 0 },
+
+ /* 581-590 */
+ { 2, 0, 0, -2, 0, 0, 0, -2, 0, 0, 2, 0, 0, 0 },
+ { 2, 0, 0, -2, 0, 0, -4, 4, 0, 0, 0, 0, 0, 0 },
+ { 2, 0, -2, 0, -2, 0, 0, 5, -9, 0, 0, 0, 0, 0 },
+ { 2, 0, -1, -1, 0, 0, 0, -1, 0, 3, 0, 0, 0, 0 },
+ { 1, 0, 2, 0, 2, 0, 1, -1, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 2, 0, 2, 0, 0, 4, -8, 3, 0, 0, 0, 0 },
+ { 1, 0, 2, 0, 2, 0, 0, -4, 8, -3, 0, 0, 0, 0 },
+ { 1, 0, 2, 0, 2, 0, -1, 1, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 2, -2, 2, 0, -3, 3, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, 0, 0, 0, 0, 0, 1, 0, -1, 0, 0, 0, 0 },
+
+ /* 591-600 */
+ { 1, 0, 0, 0, 0, 0, 0, -2, 0, 3, 0, 0, 0, 0 },
+ { 1, 0, 0, -2, 0, 0, 0, 2, 0, -2, 0, 0, 0, 0 },
+ { 1, 0, -2, -2, -2, 0, 0, 1, 0, -1, 0, 0, 0, 0 },
+ { 1, 0, -1, 1, 0, 0, 0, 1, 0, 0, 0, 0, 0, 0 },
+ { 1, 0, -1, -1, 0, 0, 0, 8,-15, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, 2, 2, 0, 0, 2, 0, -2, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 1, -1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0, -2, 0, 1, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 1, 0, 0,-10, 15, 0, 0, 0, 0, 0 },
+ { 0, 0, 2, -2, 0, -1, 0, 2, 0, 0, 0, 0, 0, 0 },
+
+ /* 601-610 */
+ { 0, 0, 1, -1, 2, 0, 0, -1, 0, 0, -1, 0, 0, 0 },
+ { 0, 0, 1, -1, 2, 0, -3, 4, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, -4, 6, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 1, 0, -1, 2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, 0, 1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, 0, -1, 0, 0, -2, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, -2, 2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, 0, 0, -1, 0, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 1, -1, -1, 0, -5, 7, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 2, 0, 0, 0, 2, 0, -2, 0, 0, 0, 0 },
+
+ /* 611-620 */
+ { 0, 0, 0, 2, 0, 0, -2, 2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 2, 0, -3, 5, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 1, 0, -1, 2, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 9,-13, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 8,-14, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 8,-11, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 6, -9, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 6, -8, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 6, -7, 0, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 5, -6, 0, 0, 0, 0, 0, -2 },
+
+ /* 621-630 */
+ { 0, 0, 0, 0, 0, 0, 5, -6, -4, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 5, -4, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 4, -8, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 4, -5, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 3, -3, 0, 2, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 3, -1, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 2, 0, 0, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 1, -1, 0, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 7,-12, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 6, -9, 0, 0, 0, 0, -2 },
+
+ /* 631-640 */
+ { 0, 0, 0, 0, 0, 0, 0, 6, -8, 1, 5, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 6, -4, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 6,-10, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, 0, -4, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -9, 0, 0, 0, 0, -1 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -8, 3, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -7, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 5, -6, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 5,-16, 4, 5, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 5,-13, 0, 0, 0, 0, -2 },
+
+ /* 641-650 */
+ { 0, 0, 0, 0, 0, 0, 0, 3, 0, -5, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -9, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 3, -7, 0, 0, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 2, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, -3, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 2, -8, 1, 5, 0, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 1, -5, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 2, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, -3, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 1, 0, -3, 5, 0, 0, 0 },
+
+ /* 651-NFPL */
+ { 0, 0, 0, 0, 0, 0, 0, 1, -3, 0, 0, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, -6, 3, 0, -2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, -2, 0, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2 },
+ { 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 0, 0, 0 }
+ };
+
+/* Number of frequencies: planetary */
+ static const int NFPL = (int) (sizeof mfapl / sizeof (int) / 14);
+
+/* Pointers into amplitudes array, one pointer per frequency */
+ static const int nc[] = {
+
+ /* 1-100 */
+ 1, 21, 37, 51, 65, 79, 91, 103, 115, 127,
+ 139, 151, 163, 172, 184, 196, 207, 219, 231, 240,
+ 252, 261, 273, 285, 297, 309, 318, 327, 339, 351,
+ 363, 372, 384, 396, 405, 415, 423, 435, 444, 452,
+ 460, 467, 474, 482, 490, 498, 506, 513, 521, 528,
+ 536, 543, 551, 559, 566, 574, 582, 590, 597, 605,
+ 613, 620, 628, 636, 644, 651, 658, 666, 674, 680,
+ 687, 695, 702, 710, 717, 725, 732, 739, 746, 753,
+ 760, 767, 774, 782, 790, 798, 805, 812, 819, 826,
+ 833, 840, 846, 853, 860, 867, 874, 881, 888, 895,
+
+ /* 101-200 */
+ 901, 908, 914, 921, 928, 934, 941, 948, 955, 962,
+ 969, 976, 982, 989, 996, 1003, 1010, 1017, 1024, 1031,
+ 1037, 1043, 1050, 1057, 1064, 1071, 1078, 1084, 1091, 1098,
+ 1104, 1112, 1118, 1124, 1131, 1138, 1145, 1151, 1157, 1164,
+ 1171, 1178, 1185, 1192, 1199, 1205, 1212, 1218, 1226, 1232,
+ 1239, 1245, 1252, 1259, 1266, 1272, 1278, 1284, 1292, 1298,
+ 1304, 1310, 1316, 1323, 1329, 1335, 1341, 1347, 1353, 1359,
+ 1365, 1371, 1377, 1383, 1389, 1396, 1402, 1408, 1414, 1420,
+ 1426, 1434, 1440, 1446, 1452, 1459, 1465, 1471, 1477, 1482,
+ 1488, 1493, 1499, 1504, 1509, 1514, 1520, 1527, 1532, 1538,
+
+ /* 201-300 */
+ 1543, 1548, 1553, 1558, 1564, 1569, 1574, 1579, 1584, 1589,
+ 1594, 1596, 1598, 1600, 1602, 1605, 1608, 1610, 1612, 1617,
+ 1619, 1623, 1625, 1627, 1629, 1632, 1634, 1640, 1642, 1644,
+ 1646, 1648, 1650, 1652, 1654, 1658, 1660, 1662, 1664, 1668,
+ 1670, 1672, 1673, 1675, 1679, 1681, 1683, 1684, 1686, 1688,
+ 1690, 1693, 1695, 1697, 1701, 1703, 1705, 1707, 1709, 1711,
+ 1712, 1715, 1717, 1721, 1723, 1725, 1727, 1729, 1731, 1733,
+ 1735, 1737, 1739, 1741, 1743, 1745, 1747, 1749, 1751, 1753,
+ 1755, 1757, 1759, 1761, 1762, 1764, 1766, 1768, 1769, 1771,
+ 1773, 1775, 1777, 1779, 1781, 1783, 1785, 1787, 1788, 1790,
+
+ /* 301-400 */
+ 1792, 1794, 1796, 1798, 1800, 1802, 1804, 1806, 1807, 1809,
+ 1811, 1815, 1817, 1819, 1821, 1823, 1825, 1827, 1829, 1831,
+ 1833, 1835, 1837, 1839, 1840, 1842, 1844, 1848, 1850, 1852,
+ 1854, 1856, 1858, 1859, 1860, 1862, 1864, 1866, 1868, 1869,
+ 1871, 1873, 1875, 1877, 1879, 1881, 1883, 1885, 1887, 1889,
+ 1891, 1892, 1896, 1898, 1900, 1901, 1903, 1905, 1907, 1909,
+ 1910, 1911, 1913, 1915, 1919, 1921, 1923, 1927, 1929, 1931,
+ 1933, 1935, 1937, 1939, 1943, 1945, 1947, 1948, 1949, 1951,
+ 1953, 1955, 1957, 1958, 1960, 1962, 1964, 1966, 1968, 1970,
+ 1971, 1973, 1974, 1975, 1977, 1979, 1980, 1981, 1982, 1984,
+
+ /* 401-500 */
+ 1986, 1988, 1990, 1992, 1994, 1995, 1997, 1999, 2001, 2003,
+ 2005, 2007, 2008, 2009, 2011, 2013, 2015, 2017, 2019, 2021,
+ 2023, 2024, 2025, 2027, 2029, 2031, 2033, 2035, 2037, 2041,
+ 2043, 2045, 2046, 2047, 2049, 2051, 2053, 2055, 2056, 2057,
+ 2059, 2061, 2063, 2065, 2067, 2069, 2070, 2071, 2072, 2074,
+ 2076, 2078, 2080, 2082, 2084, 2086, 2088, 2090, 2092, 2094,
+ 2095, 2096, 2097, 2099, 2101, 2105, 2106, 2107, 2108, 2109,
+ 2110, 2111, 2113, 2115, 2119, 2121, 2123, 2125, 2127, 2129,
+ 2131, 2133, 2135, 2136, 2137, 2139, 2141, 2143, 2145, 2147,
+ 2149, 2151, 2153, 2155, 2157, 2159, 2161, 2163, 2165, 2167,
+
+ /* 501-600 */
+ 2169, 2171, 2173, 2175, 2177, 2179, 2181, 2183, 2185, 2186,
+ 2187, 2188, 2192, 2193, 2195, 2197, 2199, 2201, 2203, 2205,
+ 2207, 2209, 2211, 2213, 2217, 2219, 2221, 2223, 2225, 2227,
+ 2229, 2231, 2233, 2234, 2235, 2236, 2237, 2238, 2239, 2240,
+ 2241, 2244, 2246, 2248, 2250, 2252, 2254, 2256, 2258, 2260,
+ 2262, 2264, 2266, 2268, 2270, 2272, 2274, 2276, 2278, 2280,
+ 2282, 2284, 2286, 2288, 2290, 2292, 2294, 2296, 2298, 2300,
+ 2302, 2303, 2304, 2305, 2306, 2307, 2309, 2311, 2313, 2315,
+ 2317, 2319, 2321, 2323, 2325, 2327, 2329, 2331, 2333, 2335,
+ 2337, 2341, 2343, 2345, 2347, 2349, 2351, 2352, 2355, 2356,
+
+ /* 601-700 */
+ 2357, 2358, 2359, 2361, 2363, 2364, 2365, 2366, 2367, 2368,
+ 2369, 2370, 2371, 2372, 2373, 2374, 2376, 2378, 2380, 2382,
+ 2384, 2385, 2386, 2387, 2388, 2389, 2390, 2391, 2392, 2393,
+ 2394, 2395, 2396, 2397, 2398, 2399, 2400, 2401, 2402, 2403,
+ 2404, 2405, 2406, 2407, 2408, 2409, 2410, 2411, 2412, 2413,
+ 2414, 2415, 2417, 2418, 2430, 2438, 2445, 2453, 2460, 2468,
+ 2474, 2480, 2488, 2496, 2504, 2512, 2520, 2527, 2535, 2543,
+ 2550, 2558, 2566, 2574, 2580, 2588, 2596, 2604, 2612, 2619,
+ 2627, 2634, 2642, 2648, 2656, 2664, 2671, 2679, 2685, 2693,
+ 2701, 2709, 2717, 2725, 2733, 2739, 2747, 2753, 2761, 2769,
+
+ /* 701-800 */
+ 2777, 2785, 2793, 2801, 2809, 2817, 2825, 2833, 2841, 2848,
+ 2856, 2864, 2872, 2878, 2884, 2892, 2898, 2906, 2914, 2922,
+ 2930, 2938, 2944, 2952, 2958, 2966, 2974, 2982, 2988, 2996,
+ 3001, 3009, 3017, 3025, 3032, 3039, 3045, 3052, 3059, 3067,
+ 3069, 3076, 3083, 3090, 3098, 3105, 3109, 3111, 3113, 3120,
+ 3124, 3128, 3132, 3136, 3140, 3144, 3146, 3150, 3158, 3161,
+ 3165, 3166, 3168, 3172, 3176, 3180, 3182, 3185, 3189, 3193,
+ 3194, 3197, 3200, 3204, 3208, 3212, 3216, 3219, 3221, 3222,
+ 3226, 3230, 3234, 3238, 3242, 3243, 3247, 3251, 3254, 3258,
+ 3262, 3266, 3270, 3274, 3275, 3279, 3283, 3287, 3289, 3293,
+
+ /* 801-900 */
+ 3296, 3300, 3303, 3307, 3311, 3315, 3319, 3321, 3324, 3327,
+ 3330, 3334, 3338, 3340, 3342, 3346, 3350, 3354, 3358, 3361,
+ 3365, 3369, 3373, 3377, 3381, 3385, 3389, 3393, 3394, 3398,
+ 3402, 3406, 3410, 3413, 3417, 3421, 3425, 3429, 3433, 3435,
+ 3439, 3443, 3446, 3450, 3453, 3457, 3458, 3461, 3464, 3468,
+ 3472, 3476, 3478, 3481, 3485, 3489, 3493, 3497, 3501, 3505,
+ 3507, 3511, 3514, 3517, 3521, 3524, 3525, 3527, 3529, 3533,
+ 3536, 3540, 3541, 3545, 3548, 3551, 3555, 3559, 3563, 3567,
+ 3569, 3570, 3574, 3576, 3578, 3582, 3586, 3590, 3593, 3596,
+ 3600, 3604, 3608, 3612, 3616, 3620, 3623, 3626, 3630, 3632,
+
+ /* 901-1000 */
+ 3636, 3640, 3643, 3646, 3648, 3652, 3656, 3660, 3664, 3667,
+ 3669, 3671, 3675, 3679, 3683, 3687, 3689, 3693, 3694, 3695,
+ 3699, 3703, 3705, 3707, 3710, 3713, 3717, 3721, 3725, 3729,
+ 3733, 3736, 3740, 3744, 3748, 3752, 3754, 3757, 3759, 3763,
+ 3767, 3770, 3773, 3777, 3779, 3783, 3786, 3790, 3794, 3798,
+ 3801, 3805, 3809, 3813, 3817, 3821, 3825, 3827, 3831, 3835,
+ 3836, 3837, 3840, 3844, 3848, 3852, 3856, 3859, 3863, 3867,
+ 3869, 3871, 3875, 3879, 3883, 3887, 3890, 3894, 3898, 3901,
+ 3905, 3909, 3913, 3917, 3921, 3922, 3923, 3924, 3926, 3930,
+ 3932, 3936, 3938, 3940, 3944, 3948, 3952, 3956, 3959, 3963,
+
+ /* 1001-1100 */
+ 3965, 3969, 3973, 3977, 3979, 3981, 3982, 3986, 3989, 3993,
+ 3997, 4001, 4004, 4006, 4009, 4012, 4016, 4020, 4024, 4026,
+ 4028, 4032, 4036, 4040, 4044, 4046, 4050, 4054, 4058, 4060,
+ 4062, 4063, 4064, 4068, 4071, 4075, 4077, 4081, 4083, 4087,
+ 4089, 4091, 4095, 4099, 4101, 4103, 4105, 4107, 4111, 4115,
+ 4119, 4123, 4127, 4129, 4131, 4135, 4139, 4141, 4143, 4145,
+ 4149, 4153, 4157, 4161, 4165, 4169, 4173, 4177, 4180, 4183,
+ 4187, 4191, 4195, 4198, 4201, 4205, 4209, 4212, 4213, 4216,
+ 4217, 4221, 4223, 4226, 4230, 4234, 4236, 4240, 4244, 4248,
+ 4252, 4256, 4258, 4262, 4264, 4266, 4268, 4270, 4272, 4276,
+
+ /* 1101-1200 */
+ 4279, 4283, 4285, 4287, 4289, 4293, 4295, 4299, 4300, 4301,
+ 4305, 4309, 4313, 4317, 4319, 4323, 4325, 4329, 4331, 4333,
+ 4335, 4337, 4341, 4345, 4349, 4351, 4353, 4357, 4361, 4365,
+ 4367, 4369, 4373, 4377, 4381, 4383, 4387, 4389, 4391, 4395,
+ 4399, 4403, 4407, 4411, 4413, 4414, 4415, 4418, 4419, 4421,
+ 4423, 4427, 4429, 4431, 4433, 4435, 4437, 4439, 4443, 4446,
+ 4450, 4452, 4456, 4458, 4460, 4462, 4466, 4469, 4473, 4477,
+ 4481, 4483, 4487, 4489, 4491, 4493, 4497, 4499, 4501, 4504,
+ 4506, 4510, 4513, 4514, 4515, 4518, 4521, 4522, 4525, 4526,
+ 4527, 4530, 4533, 4534, 4537, 4541, 4542, 4543, 4544, 4545,
+
+ /* 1201-1300 */
+ 4546, 4547, 4550, 4553, 4554, 4555, 4558, 4561, 4564, 4567,
+ 4568, 4571, 4574, 4575, 4578, 4581, 4582, 4585, 4586, 4588,
+ 4590, 4592, 4596, 4598, 4602, 4604, 4608, 4612, 4613, 4616,
+ 4619, 4622, 4623, 4624, 4625, 4626, 4629, 4632, 4633, 4636,
+ 4639, 4640, 4641, 4642, 4643, 4644, 4645, 4648, 4649, 4650,
+ 4651, 4652, 4653, 4656, 4657, 4660, 4661, 4664, 4667, 4670,
+ 4671, 4674, 4675, 4676, 4677, 4678, 4681, 4682, 4683, 4684,
+ 4687, 4688, 4689, 4692, 4693, 4696, 4697, 4700, 4701, 4702,
+ 4703, 4704, 4707, 4708, 4711, 4712, 4715, 4716, 4717, 4718,
+ 4719, 4720, 4721, 4722, 4723, 4726, 4729, 4730, 4733, 4736,
+
+ /* 1301-(NFLS+NFPL) */
+ 4737, 4740, 4741, 4742, 4745, 4746, 4749, 4752, 4753
+ };
+
+/* Amplitude coefficients (microarcsec); indexed using the nc array. */
+ static const double a[] = {
+
+ /* 1-105 */
+ -6844318.44, 9205236.26,1328.67,1538.18, 205833.11,
+ 153041.79, -3309.73, 853.32,2037.98, -2301.27,
+ 81.46, 120.56, -20.39, -15.22, 1.73, -1.61, -0.10, 0.11,
+ -0.02, -0.02, -523908.04, 573033.42,-544.75,-458.66,
+ 12814.01, 11714.49, 198.97,-290.91, 155.74,-143.27,
+ -2.75, -1.03, -1.27, -1.16, 0.00, -0.01, -90552.22,
+ 97846.69, 111.23, 137.41,2187.91,2024.68, 41.44, -51.26,
+ 26.92, -24.46, -0.46, -0.28, -0.22, -0.20, 82168.76,
+ -89618.24, -27.64, -29.05, -2004.36, -1837.32,
+ -36.07, 48.00, -24.43, 22.41, 0.47, 0.24, 0.20, 0.18,
+ 58707.02,7387.02, 470.05,-192.40, 164.33, -1312.21,
+ -179.73, -28.93, -17.36, -1.83, -0.50, 3.57, 0.00, 0.13,
+ -20557.78, 22438.42, -20.84, -17.40, 501.82, 459.68,
+ 59.20, -67.30, 6.08, -5.61, -1.36, -1.19, 28288.28,
+ -674.99, -34.69, 35.80, -15.07,-632.54, -11.19, 0.78, -8.41,
+ 0.17, 0.01, 0.07, -15406.85, 20069.50, 15.12,
+
+ /* 106-219 */
+ 31.80, 448.76, 344.50, -5.77, 1.41, 4.59, -5.02, 0.17,
+ 0.24, -11991.74, 12902.66, 32.46, 36.70, 288.49,
+ 268.14, 5.70, -7.06, 3.57, -3.23, -0.06, -0.04,
+ -8584.95, -9592.72, 4.42, -13.20,-214.50, 192.06,
+ 23.87, 29.83, 2.54, 2.40, 0.60, -0.48,5095.50,
+ -6918.22, 7.19, 3.92,-154.91,-113.94, 2.86, -1.04,
+ -1.52, 1.73, -0.07, -0.10, -4910.93, -5331.13,
+ 0.76, 0.40,-119.21, 109.81, 2.16, 3.20, 1.46, 1.33,
+ 0.04, -0.02, -6245.02,-123.48, -6.68, -8.20, -2.76,
+ 139.64, 2.71, 0.15, 1.86,2511.85, -3323.89, 1.07,
+ -0.90, -74.33, -56.17, 1.16, -0.01, -0.75, 0.83, -0.02,
+ -0.04,2307.58,3143.98, -7.52, 7.50, 70.31, -51.60, 1.46,
+ 0.16, -0.69, -0.79, 0.02, -0.05,2372.58,2554.51, 5.93,
+ -6.60, 57.12, -53.05, -0.96, -1.24, -0.71, -0.64, -0.01,
+ -2053.16,2636.13, 5.13, 7.80, 58.94, 45.91, -0.42,
+ -0.12, 0.61, -0.66, 0.02, 0.03, -1825.49,
+
+ /* 220-339 */
+ -2423.59, 1.23, -2.00, -54.19, 40.82, -1.07, -1.02,
+ 0.54, 0.61, -0.04, 0.04,2521.07,-122.28, -5.97, 2.90,
+ -2.73, -56.37, -0.82, 0.13, -0.75, -1534.09,1645.01,
+ 6.29, 6.80, 36.78, 34.30, 0.92, -1.25, 0.46, -0.41,
+ -0.02, -0.01,1898.27, 47.70, -0.72, 2.50, 1.07, -42.45,
+ -0.94, 0.02, -0.56, -1292.02, -1387.00, 0.00,
+ 0.00, -31.01, 28.89, 0.68, 0.00, 0.38, 0.35, -0.01,
+ -0.01, -1234.96,1323.81, 5.21, 5.90, 29.60, 27.61,
+ 0.74, -1.22, 0.37, -0.33, -0.02, -0.01,1137.48,
+ -1233.89, -0.04, -0.30, -27.59, -25.43, -0.61, 1.00,
+ -0.34, 0.31, 0.01, 0.01,-813.13, -1075.60, 0.40,
+ 0.30, -24.05, 18.18, -0.40, -0.01, 0.24, 0.27, -0.01,
+ 0.01,1163.22, -60.90, -2.94, 1.30, -1.36, -26.01, -0.58,
+ 0.07, -0.35,1029.70, -55.55, -2.63, 1.10, -1.25, -23.02,
+ -0.52, 0.06, -0.31,-556.26, 852.85, 3.16, -4.48, 19.06,
+ 12.44, -0.81, -0.27, 0.17, -0.21, 0.00, 0.02,-603.52,
+
+ /* 340-467 */
+ -800.34, 0.44, 0.10, -17.90, 13.49, -0.08, -0.01, 0.18,
+ 0.20, -0.01, 0.01,-628.24, 684.99, -0.64, -0.50, 15.32,
+ 14.05, 3.18, -4.19, 0.19, -0.17, -0.09, -0.07,-866.48,
+ -16.26, 0.52, -1.30, -0.36, 19.37, 0.43, -0.01, 0.26,
+ -512.37, 695.54, -1.47, -1.40, 15.55, 11.46, -0.16, 0.03,
+ 0.15, -0.17, 0.01, 0.01, 506.65, 643.75, 2.54, -2.62,
+ 14.40, -11.33, -0.77, -0.06, -0.15, -0.16, 0.00, 0.01,
+ 664.57, 16.81, -0.40, 1.00, 0.38, -14.86, -3.71, -0.09,
+ -0.20, 405.91, 522.11, 0.99, -1.50, 11.67, -9.08, -0.25,
+ -0.02, -0.12, -0.13,-305.78, 326.60, 1.75, 1.90, 7.30,
+ 6.84, 0.20, -0.04, 300.99,-325.03, -0.44, -0.50, -7.27,
+ -6.73, -1.01, 0.01, 0.00, 0.08, 0.00, 0.02, 438.51,
+ 10.47, -0.56, -0.20, 0.24, -9.81, -0.24, 0.01, -0.13,
+ -264.02, 335.24, 0.99, 1.40, 7.49, 5.90, -0.27, -0.02,
+ 284.09, 307.03, 0.32, -0.40, 6.87, -6.35, -0.99, -0.01,
+ -250.54, 327.11, 0.08, 0.40, 7.31, 5.60, -0.30, 230.72,
+
+ /* 468-595 */
+ -304.46, 0.08, -0.10, -6.81, -5.16, 0.27, 229.78, 304.17,
+ -0.60, 0.50, 6.80, -5.14, 0.33, 0.01, 256.30,-276.81,
+ -0.28, -0.40, -6.19, -5.73, -0.14, 0.01,-212.82, 269.45,
+ 0.84, 1.20, 6.02, 4.76, 0.14, -0.02, 196.64, 272.05,
+ -0.84, 0.90, 6.08, -4.40, 0.35, 0.02, 188.95, 272.22,
+ -0.12, 0.30, 6.09, -4.22, 0.34,-292.37, -5.10, -0.32,
+ -0.40, -0.11, 6.54, 0.14, 0.01, 161.79,-220.67, 0.24,
+ 0.10, -4.93, -3.62, -0.08, 261.54, -19.94, -0.95, 0.20,
+ -0.45, -5.85, -0.13, 0.02, 142.16,-190.79, 0.20, 0.10,
+ -4.27, -3.18, -0.07, 187.95, -4.11, -0.24, 0.30, -0.09,
+ -4.20, -0.09, 0.01, 0.00, 0.00, -79.08, 167.90, 0.04,
+ 0.00, 3.75, 1.77, 121.98, 131.04, -0.08, 0.10, 2.93,
+ -2.73, -0.06,-172.95, -8.11, -0.40, -0.20, -0.18, 3.87,
+ 0.09, 0.01,-160.15, -55.30, -14.04, 13.90, -1.23, 3.58,
+ 0.40, 0.31,-115.40, 123.20, 0.60, 0.70, 2.75, 2.58,
+ 0.08, -0.01,-168.26, -2.00, 0.20, -0.20, -0.04, 3.76,
+
+ /* 596-723 */
+ 0.08,-114.49, 123.20, 0.32, 0.40, 2.75, 2.56, 0.07,
+ -0.01, 112.14, 120.70, 0.28, -0.30, 2.70, -2.51, -0.07,
+ -0.01, 161.34, 4.03, 0.20, 0.20, 0.09, -3.61, -0.08,
+ 91.31, 126.64, -0.40, 0.40, 2.83, -2.04, -0.04, 0.01,
+ 105.29, 112.90, 0.44, -0.50, 2.52, -2.35, -0.07, -0.01,
+ 98.69,-106.20, -0.28, -0.30, -2.37, -2.21, -0.06, 0.01,
+ 86.74,-112.94, -0.08, -0.20, -2.53, -1.94, -0.05,-134.81,
+ 3.51, 0.20, -0.20, 0.08, 3.01, 0.07, 79.03, 107.31,
+ -0.24, 0.20, 2.40, -1.77, -0.04, 0.01, 132.81, -10.77,
+ -0.52, 0.10, -0.24, -2.97, -0.07, 0.01,-130.31, -0.90,
+ 0.04, 0.00, 0.00, 2.91, -78.56, 85.32, 0.00, 0.00,
+ 1.91, 1.76, 0.04, 0.00, 0.00, -41.53, 89.10, 0.02,
+ 0.00, 1.99, 0.93, 66.03, -71.00, -0.20, -0.20, -1.59,
+ -1.48, -0.04, 60.50, 64.70, 0.36, -0.40, 1.45, -1.35,
+ -0.04, -0.01, -52.27, -70.01, 0.00, 0.00, -1.57, 1.17,
+ 0.03, -52.95, 66.29, 0.32, 0.40, 1.48, 1.18, 0.04,
+
+ /* 724-851 */
+ -0.01, 51.02, 67.25, 0.00, 0.00, 1.50, -1.14, -0.03,
+ -55.66, -60.92, 0.16, -0.20, -1.36, 1.24, 0.03, -54.81,
+ -59.20, -0.08, 0.20, -1.32, 1.23, 0.03, 51.32, -55.60,
+ 0.00, 0.00, -1.24, -1.15, -0.03, 48.29, 51.80, 0.20,
+ -0.20, 1.16, -1.08, -0.03, -45.59, -49.00, -0.12, 0.10,
+ -1.10, 1.02, 0.03, 40.54, -52.69, -0.04, -0.10, -1.18,
+ -0.91, -0.02, -40.58, -49.51, -1.00, 1.00, -1.11, 0.91,
+ 0.04, 0.02, -43.76, 46.50, 0.36, 0.40, 1.04, 0.98,
+ 0.03, -0.01, 62.65, -5.00, -0.24, 0.00, -0.11, -1.40,
+ -0.03, 0.01, -38.57, 49.59, 0.08, 0.10, 1.11, 0.86,
+ 0.02, -33.22, -44.04, 0.08, -0.10, -0.98, 0.74, 0.02,
+ 37.15, -39.90, -0.12, -0.10, -0.89, -0.83, -0.02, 36.68,
+ -39.50, -0.04, -0.10, -0.88, -0.82, -0.02, -53.22, -3.91,
+ -0.20, 0.00, -0.09, 1.19, 0.03, 32.43, -42.19, -0.04,
+ -0.10, -0.94, -0.73, -0.02, -51.00, -2.30, -0.12, -0.10,
+ 0.00, 1.14, -29.53, -39.11, 0.04, 0.00, -0.87, 0.66,
+
+ /* 852-979 */
+ 0.02, 28.50, -38.92, -0.08, -0.10, -0.87, -0.64, -0.02,
+ 26.54, 36.95, -0.12, 0.10, 0.83, -0.59, -0.01, 26.54,
+ 34.59, 0.04, -0.10, 0.77, -0.59, -0.02, 28.35, -32.55,
+ -0.16, 0.20, -0.73, -0.63, -0.01, -28.00, 30.40, 0.00,
+ 0.00, 0.68, 0.63, 0.01, -27.61, 29.40, 0.20, 0.20,
+ 0.66, 0.62, 0.02, 40.33, 0.40, -0.04, 0.10, 0.00,
+ -0.90, -23.28, 31.61, -0.08, -0.10, 0.71, 0.52, 0.01,
+ 37.75, 0.80, 0.04, 0.10, 0.00, -0.84, 23.66, 25.80,
+ 0.00, 0.00, 0.58, -0.53, -0.01, 21.01, -27.91, 0.00,
+ 0.00, -0.62, -0.47, -0.01, -34.81, 2.89, 0.04, 0.00,
+ 0.00, 0.78, -23.49, -25.31, 0.00, 0.00, -0.57, 0.53,
+ 0.01, -23.47, 25.20, 0.16, 0.20, 0.56, 0.52, 0.02,
+ 19.58, 27.50, -0.12, 0.10, 0.62, -0.44, -0.01, -22.67,
+ -24.40, -0.08, 0.10, -0.55, 0.51, 0.01, -19.97, 25.00,
+ 0.12, 0.20, 0.56, 0.45, 0.01, 21.28, -22.80, -0.08,
+ -0.10, -0.51, -0.48, -0.01, -30.47, 0.91, 0.04, 0.00,
+
+ /* 980-1107 */
+ 0.00, 0.68, 18.58, 24.00, 0.04, -0.10, 0.54, -0.42,
+ -0.01, -18.02, 24.40, -0.04, -0.10, 0.55, 0.40, 0.01,
+ 17.74, 22.50, 0.08, -0.10, 0.50, -0.40, -0.01, -19.41,
+ 20.70, 0.08, 0.10, 0.46, 0.43, 0.01, -18.64, 20.11,
+ 0.00, 0.00, 0.45, 0.42, 0.01, -16.75, 21.60, 0.04,
+ 0.10, 0.48, 0.37, 0.01, -18.42, -20.00, 0.00, 0.00,
+ -0.45, 0.41, 0.01, -26.77, 1.41, 0.08, 0.00, 0.00,
+ 0.60, -26.17, -0.19, 0.00, 0.00, 0.00, 0.59, -15.52,
+ 20.51, 0.00, 0.00, 0.46, 0.35, 0.01, -25.42, -1.91,
+ -0.08, 0.00, -0.04, 0.57, 0.45, -17.42, 18.10, 0.00,
+ 0.00, 0.40, 0.39, 0.01, 16.39, -17.60, -0.08, -0.10,
+ -0.39, -0.37, -0.01, -14.37, 18.91, 0.00, 0.00, 0.42,
+ 0.32, 0.01, 23.39, -2.40, -0.12, 0.00, 0.00, -0.52,
+ 14.32, -18.50, -0.04, -0.10, -0.41, -0.32, -0.01, 15.69,
+ 17.08, 0.00, 0.00, 0.38, -0.35, -0.01, -22.99, 0.50,
+ 0.04, 0.00, 0.00, 0.51, 0.00, 0.00, 14.47, -17.60,
+
+ /* 1108-1235 */
+ -0.01, 0.00, -0.39, -0.32, -13.33, 18.40, -0.04, -0.10,
+ 0.41, 0.30, 22.47, -0.60, -0.04, 0.00, 0.00, -0.50,
+ -12.78, -17.41, 0.04, 0.00, -0.39, 0.29, 0.01, -14.10,
+ -15.31, 0.04, 0.00, -0.34, 0.32, 0.01, 11.98, 16.21,
+ -0.04, 0.00, 0.36, -0.27, -0.01, 19.65, -1.90, -0.08,
+ 0.00, 0.00, -0.44, 19.61, -1.50, -0.08, 0.00, 0.00,
+ -0.44, 13.41, -14.30, -0.04, -0.10, -0.32, -0.30, -0.01,
+ -13.29, 14.40, 0.00, 0.00, 0.32, 0.30, 0.01, 11.14,
+ -14.40, -0.04, 0.00, -0.32, -0.25, -0.01, 12.24, -13.38,
+ 0.04, 0.00, -0.30, -0.27, -0.01, 10.07, -13.81, 0.04,
+ 0.00, -0.31, -0.23, -0.01, 10.46, 13.10, 0.08, -0.10,
+ 0.29, -0.23, -0.01, 16.55, -1.71, -0.08, 0.00, 0.00,
+ -0.37, 9.75, -12.80, 0.00, 0.00, -0.29, -0.22, -0.01,
+ 9.11, 12.80, 0.00, 0.00, 0.29, -0.20, 0.00, 0.00,
+ -6.44, -13.80, 0.00, 0.00, -0.31, 0.14, -9.19, -12.00,
+ 0.00, 0.00, -0.27, 0.21, -10.30, 10.90, 0.08, 0.10,
+
+ /* 1236-1363 */
+ 0.24, 0.23, 0.01, 14.92, -0.80, -0.04, 0.00, 0.00,
+ -0.33, 10.02, -10.80, 0.00, 0.00, -0.24, -0.22, -0.01,
+ -9.75, 10.40, 0.04, 0.00, 0.23, 0.22, 0.01, 9.67,
+ -10.40, -0.04, 0.00, -0.23, -0.22, -0.01, -8.28, -11.20,
+ 0.04, 0.00, -0.25, 0.19, 13.32, -1.41, -0.08, 0.00,
+ 0.00, -0.30, 8.27, 10.50, 0.04, 0.00, 0.23, -0.19,
+ 0.00, 0.00, 13.13, 0.00, 0.00, 0.00, 0.00, -0.29,
+ -12.93, 0.70, 0.04, 0.00, 0.00, 0.29, 7.91, -10.20,
+ 0.00, 0.00, -0.23, -0.18, -7.84, -10.00, -0.04, 0.00,
+ -0.22, 0.18, 7.44, 9.60, 0.00, 0.00, 0.21, -0.17,
+ -7.64, 9.40, 0.08, 0.10, 0.21, 0.17, 0.01, -11.38,
+ 0.60, 0.04, 0.00, 0.00, 0.25, -7.48, 8.30, 0.00,
+ 0.00, 0.19, 0.17, -10.98, -0.20, 0.00, 0.00, 0.00,
+ 0.25, 10.98, 0.20, 0.00, 0.00, 0.00, -0.25, 7.40,
+ -7.90, -0.04, 0.00, -0.18, -0.17, -6.09, 8.40, -0.04,
+ 0.00, 0.19, 0.14, -6.94, -7.49, 0.00, 0.00, -0.17,
+
+ /* 1364-1491 */
+ 0.16, 6.92, 7.50, 0.04, 0.00, 0.17, -0.15, 6.20,
+ 8.09, 0.00, 0.00, 0.18, -0.14, -6.12, 7.80, 0.04,
+ 0.00, 0.17, 0.14, 5.85, -7.50, 0.00, 0.00, -0.17,
+ -0.13, -6.48, 6.90, 0.08, 0.10, 0.15, 0.14, 0.01,
+ 6.32, 6.90, 0.00, 0.00, 0.15, -0.14, 5.61, -7.20,
+ 0.00, 0.00, -0.16, -0.13, 9.07, 0.00, 0.00, 0.00,
+ 0.00, -0.20, 5.25, 6.90, 0.00, 0.00, 0.15, -0.12,
+ -8.47, -0.40, 0.00, 0.00, 0.00, 0.19, 6.32, -5.39,
+ -1.11, 1.10, -0.12, -0.14, 0.02, 0.02, 5.73, -6.10,
+ -0.04, 0.00, -0.14, -0.13, 4.70, 6.60, -0.04, 0.00,
+ 0.15, -0.11, -4.90, -6.40, 0.00, 0.00, -0.14, 0.11,
+ -5.33, 5.60, 0.04, 0.10, 0.13, 0.12, 0.01, -4.81,
+ 6.00, 0.04, 0.00, 0.13, 0.11, 5.13, 5.50, 0.04,
+ 0.00, 0.12, -0.11, 4.50, 5.90, 0.00, 0.00, 0.13,
+ -0.10, -4.22, 6.10, 0.00, 0.00, 0.14, -4.53, 5.70,
+ 0.00, 0.00, 0.13, 0.10, 4.18, 5.70, 0.00, 0.00,
+
+ /* 1492-1619 */
+ 0.13, -4.75, -5.19, 0.00, 0.00, -0.12, 0.11, -4.06,
+ 5.60, 0.00, 0.00, 0.13, -3.98, 5.60, -0.04, 0.00,
+ 0.13, 4.02, -5.40, 0.00, 0.00, -0.12, 4.49, -4.90,
+ -0.04, 0.00, -0.11, -0.10, -3.62, -5.40, -0.16, 0.20,
+ -0.12, 0.00, 0.01, 4.38, 4.80, 0.00, 0.00, 0.11,
+ -6.40, -0.10, 0.00, 0.00, 0.00, 0.14, -3.98, 5.00,
+ 0.04, 0.00, 0.11, -3.82, -5.00, 0.00, 0.00, -0.11,
+ -3.71, 5.07, 0.00, 0.00, 0.11, 4.14, 4.40, 0.00,
+ 0.00, 0.10, -6.01, -0.50, -0.04, 0.00, 0.00, 0.13,
+ -4.04, 4.39, 0.00, 0.00, 0.10, 3.45, -4.72, 0.00,
+ 0.00, -0.11, 3.31, 4.71, 0.00, 0.00, 0.11, 3.26,
+ -4.50, 0.00, 0.00, -0.10, -3.26, -4.50, 0.00, 0.00,
+ -0.10, -3.34, -4.40, 0.00, 0.00, -0.10, -3.74, -4.00,
+ 3.70, 4.00, 3.34, -4.30, 3.30, -4.30, -3.66, 3.90,
+ 0.04, 3.66, 3.90, 0.04, -3.62, -3.90, -3.61, 3.90,
+ -0.20, 5.30, 0.00, 0.00, 0.12, 3.06, 4.30, 3.30,
+
+ /* 1620-1747 */
+ 4.00, 0.40, 0.20, 3.10, 4.10, -3.06, 3.90, -3.30,
+ -3.60, -3.30, 3.36, 0.01, 3.14, 3.40, -4.57, -0.20,
+ 0.00, 0.00, 0.00, 0.10, -2.70, -3.60, 2.94, -3.20,
+ -2.90, 3.20, 2.47, -3.40, 2.55, -3.30, 2.80, -3.08,
+ 2.51, 3.30, -4.10, 0.30, -0.12, -0.10, 4.10, 0.20,
+ -2.74, 3.00, 2.46, 3.23, -3.66, 1.20, -0.20, 0.20,
+ 3.74, -0.40, -2.51, -2.80, -3.74, 2.27, -2.90, 0.00,
+ 0.00, -2.50, 2.70, -2.51, 2.60, -3.50, 0.20, 3.38,
+ -2.22, -2.50, 3.26, -0.40, 1.95, -2.60, 3.22, -0.40,
+ -0.04, -1.79, -2.60, 1.91, 2.50, 0.74, 3.05, -0.04,
+ 0.08, 2.11, -2.30, -2.11, 2.20, -1.87, -2.40, 2.03,
+ -2.20, -2.03, 2.20, 2.98, 0.00, 0.00, 2.98, -1.71,
+ 2.40, 2.94, -0.10, -0.12, 0.10, 1.67, 2.40, -1.79,
+ 2.30, -1.79, 2.20, -1.67, 2.20, 1.79, -2.00, 1.87,
+ -1.90, 1.63, -2.10, -1.59, 2.10, 1.55, -2.10, -1.55,
+ 2.10, -2.59, -0.20, -1.75, -1.90, -1.75, 1.90, -1.83,
+
+ /* 1748-1875 */
+ -1.80, 1.51, 2.00, -1.51, -2.00, 1.71, 1.80, 1.31,
+ 2.10, -1.43, 2.00, 1.43, 2.00, -2.43, -1.51, 1.90,
+ -1.47, 1.90, 2.39, 0.20, -2.39, 1.39, 1.90, 1.39,
+ -1.80, 1.47, -1.60, 1.47, -1.60, 1.43, -1.50, -1.31,
+ 1.60, 1.27, -1.60, -1.27, 1.60, 1.27, -1.60, 2.03,
+ 1.35, 1.50, -1.39, -1.40, 1.95, -0.20, -1.27, 1.49,
+ 1.19, 1.50, 1.27, 1.40, 1.15, 1.50, 1.87, -0.10,
+ -1.12, -1.50, 1.87, -1.11, -1.50, -1.11, -1.50, 0.00,
+ 0.00, 1.19, 1.40, 1.27, -1.30, -1.27, -1.30, -1.15,
+ 1.40, -1.23, 1.30, -1.23, -1.30, 1.22, -1.29, 1.07,
+ -1.40, 1.75, -0.20, -1.03, -1.40, -1.07, 1.20, -1.03,
+ 1.15, 1.07, 1.10, 1.51, -1.03, 1.10, 1.03, -1.10,
+ 0.00, 0.00, -1.03, -1.10, 0.91, -1.20, -0.88, -1.20,
+ -0.88, 1.20, -0.95, 1.10, -0.95, -1.10, 1.43, -1.39,
+ 0.95, -1.00, -0.95, 1.00, -0.80, 1.10, 0.91, -1.00,
+ -1.35, 0.88, 1.00, -0.83, 1.00, -0.91, 0.90, 0.91,
+
+ /* 1876-2003 */
+ 0.90, 0.88, -0.90, -0.76, -1.00, -0.76, 1.00, 0.76,
+ 1.00, -0.72, 1.00, 0.84, -0.90, 0.84, 0.90, 1.23,
+ 0.00, 0.00, -0.52, -1.10, -0.68, 1.00, 1.19, -0.20,
+ 1.19, 0.76, 0.90, 1.15, -0.10, 1.15, -0.10, 0.72,
+ -0.90, -1.15, -1.15, 0.68, 0.90, -0.68, 0.90, -1.11,
+ 0.00, 0.00, 0.20, 0.79, 0.80, -1.11, -0.10, 0.00,
+ 0.00, -0.48, -1.00, -0.76, -0.80, -0.72, -0.80, -1.07,
+ -0.10, 0.64, 0.80, -0.64, -0.80, 0.64, 0.80, 0.40,
+ 0.60, 0.52, -0.50, -0.60, -0.80, -0.71, 0.70, -0.99,
+ 0.99, 0.56, 0.80, -0.56, 0.80, 0.68, -0.70, 0.68,
+ 0.70, -0.95, -0.64, 0.70, 0.64, 0.70, -0.60, 0.70,
+ -0.60, -0.70, -0.91, -0.10, -0.51, 0.76, -0.91, -0.56,
+ 0.70, 0.88, 0.88, -0.63, -0.60, 0.55, -0.60, -0.80,
+ 0.80, -0.80, -0.52, 0.60, 0.52, 0.60, 0.52, -0.60,
+ -0.48, 0.60, 0.48, 0.60, 0.48, 0.60, -0.76, 0.44,
+ -0.60, 0.52, -0.50, -0.52, 0.50, 0.40, 0.60, -0.40,
+
+ /* 2004-2131 */
+ -0.60, 0.40, -0.60, 0.72, -0.72, -0.51, -0.50, -0.48,
+ 0.50, 0.48, -0.50, -0.48, 0.50, -0.48, 0.50, 0.48,
+ -0.50, -0.48, -0.50, -0.68, -0.68, 0.44, 0.50, -0.64,
+ -0.10, -0.64, -0.10, -0.40, 0.50, 0.40, 0.50, 0.40,
+ 0.50, 0.00, 0.00, -0.40, -0.50, -0.36, -0.50, 0.36,
+ -0.50, 0.60, -0.60, 0.40, -0.40, 0.40, 0.40, -0.40,
+ 0.40, -0.40, 0.40, -0.56, -0.56, 0.36, -0.40, -0.36,
+ 0.40, 0.36, -0.40, -0.36, -0.40, 0.36, 0.40, 0.36,
+ 0.40, -0.52, 0.52, 0.52, 0.32, 0.40, -0.32, 0.40,
+ -0.32, 0.40, -0.32, 0.40, 0.32, -0.40, -0.32, -0.40,
+ 0.32, -0.40, 0.28, -0.40, -0.28, 0.40, 0.28, -0.40,
+ 0.28, 0.40, 0.48, -0.48, 0.48, 0.36, -0.30, -0.36,
+ -0.30, 0.00, 0.00, 0.20, 0.40, -0.44, 0.44, -0.44,
+ -0.44, -0.44, -0.44, 0.32, -0.30, 0.32, 0.30, 0.24,
+ 0.30, -0.12, -0.10, -0.28, 0.30, 0.28, 0.30, 0.28,
+ 0.30, 0.28, -0.30, 0.28, -0.30, 0.28, -0.30, 0.28,
+
+ /* 2132-2259 */
+ 0.30, -0.28, 0.30, 0.40, 0.40, -0.24, 0.30, 0.24,
+ -0.30, 0.24, -0.30, -0.24, -0.30, 0.24, 0.30, 0.24,
+ -0.30, -0.24, 0.30, 0.24, -0.30, -0.24, -0.30, 0.24,
+ -0.30, 0.24, 0.30, -0.24, 0.30, -0.24, 0.30, 0.20,
+ -0.30, 0.20, -0.30, 0.20, -0.30, 0.20, 0.30, 0.20,
+ -0.30, 0.20, -0.30, 0.20, 0.30, 0.20, 0.30, -0.20,
+ -0.30, 0.20, -0.30, 0.20, -0.30, -0.36, -0.36, -0.36,
+ -0.04, 0.30, 0.12, -0.10, -0.32, -0.24, 0.20, 0.24,
+ 0.20, 0.20, -0.20, -0.20, -0.20, -0.20, -0.20, 0.20,
+ 0.20, 0.20, -0.20, 0.20, 0.20, 0.20, 0.20, -0.20,
+ -0.20, 0.00, 0.00, -0.20, -0.20, -0.20, 0.20, -0.20,
+ 0.20, 0.20, -0.20, -0.20, -0.20, 0.20, 0.20, 0.20,
+ 0.20, 0.20, -0.20, 0.20, -0.20, 0.28, 0.28, 0.28,
+ 0.28, 0.28, 0.28, -0.28, 0.28, 0.12, 0.00, 0.24,
+ 0.16, -0.20, 0.16, -0.20, 0.16, -0.20, 0.16, 0.20,
+ -0.16, 0.20, 0.16, 0.20, -0.16, 0.20, -0.16, 0.20,
+
+ /* 2260-2387 */
+ -0.16, 0.20, 0.16, -0.20, 0.16, 0.20, 0.16, -0.20,
+ -0.16, 0.20, -0.16, -0.20, -0.16, 0.20, 0.16, 0.20,
+ 0.16, -0.20, 0.16, -0.20, 0.16, 0.20, 0.16, 0.20,
+ 0.16, 0.20, -0.16, -0.20, 0.16, 0.20, -0.16, 0.20,
+ 0.16, 0.20, -0.16, -0.20, 0.16, -0.20, 0.16, -0.20,
+ -0.16, -0.20, 0.24, -0.24, -0.24, 0.24, 0.24, 0.12,
+ 0.20, 0.12, 0.20, -0.12, -0.20, 0.12, -0.20, 0.12,
+ -0.20, -0.12, 0.20, -0.12, 0.20, -0.12, -0.20, 0.12,
+ 0.20, 0.12, 0.20, 0.12, -0.20, -0.12, 0.20, 0.12,
+ -0.20, -0.12, 0.20, 0.12, 0.20, 0.00, 0.00, -0.12,
+ 0.20, -0.12, 0.20, 0.12, -0.20, -0.12, 0.20, 0.12,
+ 0.20, 0.00, -0.21, -0.20, 0.00, 0.00, 0.20, -0.20,
+ -0.20, -0.20, 0.20, -0.16, -0.10, 0.00, 0.17, 0.16,
+ 0.16, 0.16, 0.16, -0.16, 0.16, 0.16, -0.16, 0.16,
+ -0.16, 0.16, 0.12, 0.10, 0.12, -0.10, -0.12, 0.10,
+ -0.12, 0.10, 0.12, -0.10, -0.12, 0.12, -0.12, 0.12,
+
+ /* 2388-2515 */
+ -0.12, 0.12, -0.12, -0.12, -0.12, -0.12, -0.12, -0.12,
+ -0.12, 0.12, 0.12, 0.12, 0.12, -0.12, -0.12, 0.12,
+ 0.12, 0.12, -0.12, 0.12, -0.12, -0.12, -0.12, 0.12,
+ -0.12, -0.12, 0.12, 0.00, 0.11, 0.11,-122.67, 164.70,
+ 203.78, 273.50, 3.58, 2.74, 6.18, -4.56, 0.00, -0.04,
+ 0.00, -0.07, 57.44, -77.10, 95.82, 128.60, -1.77, -1.28,
+ 2.85, -2.14, 82.14, 89.50, 0.00, 0.00, 2.00, -1.84,
+ -0.04, 47.73, -64.10, 23.79, 31.90, -1.45, -1.07, 0.69,
+ -0.53, -46.38, 50.50, 0.00, 0.00, 1.13, 1.04, 0.02,
+ -18.38, 0.00, 63.80, 0.00, 0.00, 0.41, 0.00, -1.43,
+ 59.07, 0.00, 0.00, 0.00, 0.00, -1.32, 57.28, 0.00,
+ 0.00, 0.00, 0.00, -1.28, -48.65, 0.00, -1.15, 0.00,
+ 0.00, 1.09, 0.00, 0.03, -18.30, 24.60, -17.30, -23.20,
+ 0.56, 0.41, -0.51, 0.39, -16.91, 26.90, 8.43, 13.30,
+ 0.60, 0.38, 0.31, -0.19, 1.23, -1.70, -19.13, -25.70,
+ -0.03, -0.03, -0.58, 0.43, -0.72, 0.90, -17.34, -23.30,
+
+ /* 2516-2643 */
+ 0.03, 0.02, -0.52, 0.39, -19.49, -21.30, 0.00, 0.00,
+ -0.48, 0.44, 0.01, 20.57, -20.10, 0.64, 0.70, -0.45,
+ -0.46, 0.00, -0.01, 4.89, 5.90, -16.55, 19.90, 0.14,
+ -0.11, 0.44, 0.37, 18.22, 19.80, 0.00, 0.00, 0.44,
+ -0.41, -0.01, 4.89, -5.30, -16.51, -18.00, -0.11, -0.11,
+ -0.41, 0.37, -17.86, 0.00, 17.10, 0.00, 0.00, 0.40,
+ 0.00, -0.38, 0.32, 0.00, 24.42, 0.00, 0.00, -0.01,
+ 0.00, -0.55, -23.79, 0.00, 0.00, 0.00, 0.00, 0.53,
+ 14.72, -16.00, -0.32, 0.00, -0.36, -0.33, -0.01, 0.01,
+ 3.34, -4.50, 11.86, 15.90, -0.11, -0.07, 0.35, -0.27,
+ -3.26, 4.40, 11.62, 15.60, 0.09, 0.07, 0.35, -0.26,
+ -19.53, 0.00, 5.09, 0.00, 0.00, 0.44, 0.00, -0.11,
+ -13.48, 14.70, 0.00, 0.00, 0.33, 0.30, 0.01, 10.86,
+ -14.60, 3.18, 4.30, -0.33, -0.24, 0.09, -0.07, -11.30,
+ -15.10, 0.00, 0.00, -0.34, 0.25, 0.01, 2.03, -2.70,
+ 10.82, 14.50, -0.07, -0.05, 0.32, -0.24, 17.46, 0.00,
+
+ /* 2644-2771 */
+ 0.00, 0.00, 0.00, -0.39, 16.43, 0.00, 0.52, 0.00,
+ 0.00, -0.37, 0.00, -0.01, 9.35, 0.00, 13.29, 0.00,
+ 0.00, -0.21, 0.00, -0.30, -10.42, 11.40, 0.00, 0.00,
+ 0.25, 0.23, 0.01, 0.44, 0.50, -10.38, 11.30, 0.02,
+ -0.01, 0.25, 0.23, -14.64, 0.00, 0.00, 0.00, 0.00,
+ 0.33, 0.56, 0.80, -8.67, 11.70, 0.02, -0.01, 0.26,
+ 0.19, 13.88, 0.00, -2.47, 0.00, 0.00, -0.31, 0.00,
+ 0.06, -1.99, 2.70, 7.72, 10.30, 0.06, 0.04, 0.23,
+ -0.17, -0.20, 0.00, 13.05, 0.00, 0.00, 0.00, 0.00,
+ -0.29, 6.92, -9.30, 3.34, 4.50, -0.21, -0.15, 0.10,
+ -0.07, -6.60, 0.00, 10.70, 0.00, 0.00, 0.15, 0.00,
+ -0.24, -8.04, -8.70, 0.00, 0.00, -0.19, 0.18, -10.58,
+ 0.00, -3.10, 0.00, 0.00, 0.24, 0.00, 0.07, -7.32,
+ 8.00, -0.12, -0.10, 0.18, 0.16, 1.63, 1.70, 6.96,
+ -7.60, 0.03, -0.04, -0.17, -0.16, -3.62, 0.00, 9.86,
+ 0.00, 0.00, 0.08, 0.00, -0.22, 0.20, -0.20, -6.88,
+
+ /* 2772-2899 */
+ -7.50, 0.00, 0.00, -0.17, 0.15, -8.99, 0.00, 4.02,
+ 0.00, 0.00, 0.20, 0.00, -0.09, -1.07, 1.40, -5.69,
+ -7.70, 0.03, 0.02, -0.17, 0.13, 6.48, -7.20, -0.48,
+ -0.50, -0.16, -0.14, -0.01, 0.01, 5.57, -7.50, 1.07,
+ 1.40, -0.17, -0.12, 0.03, -0.02, 8.71, 0.00, 3.54,
+ 0.00, 0.00, -0.19, 0.00, -0.08, 0.40, 0.00, 9.27,
+ 0.00, 0.00, -0.01, 0.00, -0.21, -6.13, 6.70, -1.19,
+ -1.30, 0.15, 0.14, -0.03, 0.03, 5.21, -5.70, -2.51,
+ -2.60, -0.13, -0.12, -0.06, 0.06, 5.69, -6.20, -0.12,
+ -0.10, -0.14, -0.13, -0.01, 2.03, -2.70, 4.53, 6.10,
+ -0.06, -0.05, 0.14, -0.10, 5.01, 5.50, -2.51, 2.70,
+ 0.12, -0.11, 0.06, 0.06, -1.91, 2.60, -4.38, -5.90,
+ 0.06, 0.04, -0.13, 0.10, 4.65, -6.30, 0.00, 0.00,
+ -0.14, -0.10, -5.29, 5.70, 0.00, 0.00, 0.13, 0.12,
+ -2.23, -4.00, -4.65, 4.20, -0.09, 0.05, 0.10, 0.10,
+ -4.53, 6.10, 0.00, 0.00, 0.14, 0.10, 2.47, 2.70,
+
+ /* 2900-3027 */
+ -4.46, 4.90, 0.06, -0.06, 0.11, 0.10, -5.05, 5.50,
+ 0.84, 0.90, 0.12, 0.11, 0.02, -0.02, 4.97, -5.40,
+ -1.71, 0.00, -0.12, -0.11, 0.00, 0.04, -0.99, -1.30,
+ 4.22, -5.70, -0.03, 0.02, -0.13, -0.09, 0.99, 1.40,
+ 4.22, -5.60, 0.03, -0.02, -0.13, -0.09, -4.69, -5.20,
+ 0.00, 0.00, -0.12, 0.10, -3.42, 0.00, 6.09, 0.00,
+ 0.00, 0.08, 0.00, -0.14, -4.65, -5.10, 0.00, 0.00,
+ -0.11, 0.10, 0.00, 0.00, -4.53, -5.00, 0.00, 0.00,
+ -0.11, 0.10, -2.43, -2.70, -3.82, 4.20, -0.06, 0.05,
+ 0.10, 0.09, 0.00, 0.00, -4.53, 4.90, 0.00, 0.00,
+ 0.11, 0.10, -4.49, -4.90, 0.00, 0.00, -0.11, 0.10,
+ 2.67, -2.90, -3.62, -3.90, -0.06, -0.06, -0.09, 0.08,
+ 3.94, -5.30, 0.00, 0.00, -0.12, -3.38, 3.70, -2.78,
+ -3.10, 0.08, 0.08, -0.07, 0.06, 3.18, -3.50, -2.82,
+ -3.10, -0.08, -0.07, -0.07, 0.06, -5.77, 0.00, 1.87,
+ 0.00, 0.00, 0.13, 0.00, -0.04, 3.54, -4.80, -0.64,
+
+ /* 3028-3155 */
+ -0.90, -0.11, 0.00, -0.02, -3.50, -4.70, 0.68, -0.90,
+ -0.11, 0.00, -0.02, 5.49, 0.00, 0.00, 0.00, 0.00,
+ -0.12, 1.83, -2.50, 2.63, 3.50, -0.06, 0.00, 0.08,
+ 3.02, -4.10, 0.68, 0.90, -0.09, 0.00, 0.02, 0.00,
+ 0.00, 5.21, 0.00, 0.00, 0.00, 0.00, -0.12, -3.54,
+ 3.80, 2.70, 3.60, -1.35, 1.80, 0.08, 0.00, 0.04,
+ -2.90, 3.90, 0.68, 0.90, 0.09, 0.00, 0.02, 0.80,
+ -1.10, -2.78, -3.70, -0.02, 0.00, -0.08, 4.10, 0.00,
+ -2.39, 0.00, 0.00, -0.09, 0.00, 0.05, -1.59, 2.10,
+ 2.27, 3.00, 0.05, 0.00, 0.07, -2.63, 3.50, -0.48,
+ -0.60, -2.94, -3.20, -2.94, 3.20, 2.27, -3.00, -1.11,
+ -1.50, -0.07, 0.00, -0.03, -0.56, -0.80, -2.35, 3.10,
+ 0.00, -0.60, -3.42, 1.90, -0.12, -0.10, 2.63, -2.90,
+ 2.51, 2.80, -0.64, 0.70, -0.48, -0.60, 2.19, -2.90,
+ 0.24, -0.30, 2.15, 2.90, 2.15, -2.90, 0.52, 0.70,
+ 2.07, -2.80, -3.10, 0.00, 1.79, 0.00, 0.00, 0.07,
+
+ /* 3156-3283 */
+ 0.00, -0.04, 0.88, 0.00, -3.46, 2.11, 2.80, -0.36,
+ 0.50, 3.54, -0.20, -3.50, -1.39, 1.50, -1.91, -2.10,
+ -1.47, 2.00, 1.39, 1.90, 2.07, -2.30, 0.91, 1.00,
+ 1.99, -2.70, 3.30, 0.00, 0.60, -0.44, -0.70, -1.95,
+ 2.60, 2.15, -2.40, -0.60, -0.70, 3.30, 0.84, 0.00,
+ -3.10, -3.10, 0.00, -0.72, -0.32, 0.40, -1.87, -2.50,
+ 1.87, -2.50, 0.32, 0.40, -0.24, 0.30, -1.87, -2.50,
+ -0.24, -0.30, 1.87, -2.50, -2.70, 0.00, 1.55, 2.03,
+ 2.20, -2.98, -1.99, -2.20, 0.12, -0.10, -0.40, 0.50,
+ 1.59, 2.10, 0.00, 0.00, -1.79, 2.00, -1.03, 1.40,
+ -1.15, -1.60, 0.32, 0.50, 1.39, -1.90, 2.35, -1.27,
+ 1.70, 0.60, 0.80, -0.32, -0.40, 1.35, -1.80, 0.44,
+ 0.00, 2.23, -0.84, 0.90, -1.27, -1.40, -1.47, 1.60,
+ -0.28, -0.30, -0.28, 0.40, -1.27, -1.70, 0.28, -0.40,
+ -1.43, -1.50, 0.00, 0.00, -1.27, -1.70, 2.11, -0.32,
+ -0.40, -1.23, 1.60, 1.19, -1.30, -0.72, -0.80, 0.72,
+
+ /* 3284-3411 */
+ -0.80, -1.15, -1.30, -1.35, -1.50, -1.19, -1.60, -0.12,
+ 0.20, 1.79, 0.00, -0.88, -0.28, 0.40, 1.11, 1.50,
+ -1.83, 0.00, 0.56, -0.12, 0.10, -1.27, -1.40, 0.00,
+ 0.00, 1.15, 1.50, -0.12, 0.20, 1.11, 1.50, 0.36,
+ -0.50, -1.07, -1.40, -1.11, 1.50, 1.67, 0.00, 0.80,
+ -1.11, 0.00, 1.43, 1.23, -1.30, -0.24, -1.19, -1.30,
+ -0.24, 0.20, -0.44, -0.90, -0.95, 1.10, 1.07, -1.40,
+ 1.15, -1.30, 1.03, -1.10, -0.56, -0.60, -0.68, 0.90,
+ -0.76, -1.00, -0.24, -0.30, 0.95, -1.30, 0.56, 0.70,
+ 0.84, -1.10, -0.56, 0.00, -1.55, 0.91, -1.30, 0.28,
+ 0.30, 0.16, -0.20, 0.95, 1.30, 0.40, -0.50, -0.88,
+ -1.20, 0.95, -1.10, -0.48, -0.50, 0.00, 0.00, -1.07,
+ 1.20, 0.44, -0.50, 0.95, 1.10, 0.00, 0.00, 0.92,
+ -1.30, 0.95, 1.00, -0.52, 0.60, 1.59, 0.24, -0.40,
+ 0.91, 1.20, 0.84, -1.10, -0.44, -0.60, 0.84, 1.10,
+ -0.44, 0.60, -0.44, 0.60, -0.84, -1.10, -0.80, 0.00,
+
+ /* 3412-3539 */
+ 1.35, 0.76, 0.20, -0.91, -1.00, 0.20, -0.30, -0.91,
+ -1.20, -0.95, 1.00, -0.48, -0.50, 0.88, 1.00, 0.48,
+ -0.50, -0.95, -1.10, 0.20, -0.20, -0.99, 1.10, -0.84,
+ 1.10, -0.24, -0.30, 0.20, -0.30, 0.84, 1.10, -1.39,
+ 0.00, -0.28, -0.16, 0.20, 0.84, 1.10, 0.00, 0.00,
+ 1.39, 0.00, 0.00, -0.95, 1.00, 1.35, -0.99, 0.00,
+ 0.88, -0.52, 0.00, -1.19, 0.20, 0.20, 0.76, -1.00,
+ 0.00, 0.00, 0.76, 1.00, 0.00, 0.00, 0.76, 1.00,
+ -0.76, 1.00, 0.00, 0.00, 1.23, 0.76, 0.80, -0.32,
+ 0.40, -0.72, 0.80, -0.40, -0.40, 0.00, 0.00, -0.80,
+ -0.90, -0.68, 0.90, -0.16, -0.20, -0.16, -0.20, 0.68,
+ -0.90, -0.36, 0.50, -0.56, -0.80, 0.72, -0.90, 0.44,
+ -0.60, -0.48, -0.70, -0.16, 0.00, -1.11, 0.32, 0.00,
+ -1.07, 0.60, -0.80, -0.28, -0.40, -0.64, 0.00, 0.91,
+ 1.11, 0.64, -0.90, 0.76, -0.80, 0.00, 0.00, -0.76,
+ -0.80, 1.03, 0.00, -0.36, -0.64, -0.70, 0.36, -0.40,
+
+ /* 3540-3667 */
+ 1.07, 0.36, -0.50, -0.52, -0.70, 0.60, 0.00, 0.88,
+ 0.95, 0.00, 0.48, 0.16, -0.20, 0.60, 0.80, 0.16,
+ -0.20, -0.60, -0.80, 0.00, -1.00, 0.12, 0.20, 0.16,
+ -0.20, 0.68, 0.70, 0.59, -0.80, -0.99, -0.56, -0.60,
+ 0.36, -0.40, -0.68, -0.70, -0.68, -0.70, -0.36, -0.50,
+ -0.44, 0.60, 0.64, 0.70, -0.12, 0.10, -0.52, 0.60,
+ 0.36, 0.40, 0.00, 0.00, 0.95, -0.84, 0.00, 0.44,
+ 0.56, 0.60, 0.32, -0.30, 0.00, 0.00, 0.60, 0.70,
+ 0.00, 0.00, 0.60, 0.70, -0.12, -0.20, 0.52, -0.70,
+ 0.00, 0.00, 0.56, 0.70, -0.12, 0.10, -0.52, -0.70,
+ 0.00, 0.00, 0.88, -0.76, 0.00, -0.44, 0.00, 0.00,
+ -0.52, -0.70, 0.52, -0.70, 0.36, -0.40, -0.44, -0.50,
+ 0.00, 0.00, 0.60, 0.60, 0.84, 0.00, 0.12, -0.24,
+ 0.00, 0.80, -0.56, 0.60, -0.32, -0.30, 0.48, -0.50,
+ 0.28, -0.30, -0.48, -0.50, 0.12, 0.20, 0.48, -0.60,
+ 0.48, 0.60, -0.12, 0.20, 0.24, 0.00, 0.76, -0.52,
+
+ /* 3668-3795 */
+ -0.60, -0.52, 0.60, 0.48, -0.50, -0.24, -0.30, 0.12,
+ -0.10, 0.48, 0.60, 0.52, -0.20, 0.36, 0.40, -0.44,
+ 0.50, -0.24, -0.30, -0.48, -0.60, -0.44, -0.60, -0.12,
+ 0.10, 0.76, 0.76, 0.20, -0.20, 0.48, 0.50, 0.40,
+ -0.50, -0.24, -0.30, 0.44, -0.60, 0.44, -0.60, 0.36,
+ 0.00, -0.64, 0.72, 0.00, -0.12, 0.00, -0.10, -0.40,
+ -0.60, -0.20, -0.20, -0.44, 0.50, -0.44, 0.50, 0.20,
+ 0.20, -0.44, -0.50, 0.20, -0.20, -0.20, 0.20, -0.44,
+ -0.50, 0.64, 0.00, 0.32, -0.36, 0.50, -0.20, -0.30,
+ 0.12, -0.10, 0.48, 0.50, -0.12, 0.30, -0.36, -0.50,
+ 0.00, 0.00, 0.48, 0.50, -0.48, 0.50, 0.68, 0.00,
+ -0.12, 0.56, -0.40, 0.44, -0.50, -0.12, -0.10, 0.24,
+ 0.30, -0.40, 0.40, 0.64, 0.00, -0.24, 0.64, 0.00,
+ -0.20, 0.00, 0.00, 0.44, -0.50, 0.44, 0.50, -0.12,
+ 0.20, -0.36, -0.50, 0.12, 0.00, 0.64, -0.40, 0.50,
+ 0.00, 0.10, 0.00, 0.00, -0.40, 0.50, 0.00, 0.00,
+
+ /* 3796-3923 */
+ -0.40, -0.50, 0.56, 0.00, 0.28, 0.00, 0.10, 0.36,
+ 0.50, 0.00, -0.10, 0.36, -0.50, 0.36, 0.50, 0.00,
+ -0.10, 0.24, -0.20, -0.36, -0.40, 0.16, 0.20, 0.40,
+ -0.40, 0.00, 0.00, -0.36, -0.50, -0.36, -0.50, -0.32,
+ -0.50, -0.12, 0.10, 0.20, 0.20, -0.36, 0.40, -0.60,
+ 0.60, 0.28, 0.00, 0.52, 0.12, -0.10, 0.40, 0.40,
+ 0.00, -0.50, 0.20, -0.20, -0.32, 0.40, 0.16, 0.20,
+ -0.16, 0.20, 0.32, 0.40, 0.56, 0.00, -0.12, 0.32,
+ -0.40, -0.16, -0.20, 0.00, 0.00, 0.40, 0.40, -0.40,
+ -0.40, -0.40, 0.40, -0.36, 0.40, 0.12, 0.10, 0.00,
+ 0.10, 0.36, 0.40, 0.00, -0.10, 0.36, 0.40, -0.36,
+ 0.40, 0.00, 0.10, 0.32, 0.00, 0.44, 0.12, 0.20,
+ 0.28, -0.40, 0.00, 0.00, 0.36, 0.40, 0.32, -0.40,
+ -0.16, 0.12, 0.10, 0.32, -0.40, 0.20, 0.30, -0.24,
+ 0.30, 0.00, 0.10, 0.32, 0.40, 0.00, -0.10, -0.32,
+ -0.40, -0.32, 0.40, 0.00, 0.10, -0.52, -0.52, 0.52,
+
+ /* 3924-4051 */
+ 0.32, -0.40, 0.00, 0.00, 0.32, 0.40, 0.32, -0.40,
+ 0.00, 0.00, -0.32, -0.40, -0.32, 0.40, 0.32, 0.40,
+ 0.00, 0.00, 0.32, 0.40, 0.00, 0.00, -0.32, -0.40,
+ 0.00, 0.00, 0.32, 0.40, 0.16, 0.20, 0.32, -0.30,
+ -0.16, 0.00, -0.48, -0.20, 0.20, -0.28, -0.30, 0.28,
+ -0.40, 0.00, 0.00, 0.28, -0.40, 0.00, 0.00, 0.28,
+ -0.40, 0.00, 0.00, -0.28, -0.40, 0.28, 0.40, -0.28,
+ -0.40, -0.48, -0.20, 0.20, 0.24, 0.30, 0.44, 0.00,
+ 0.16, 0.24, 0.30, 0.16, -0.20, 0.24, 0.30, -0.12,
+ 0.20, 0.20, 0.30, -0.16, 0.20, 0.00, 0.00, 0.44,
+ -0.32, 0.30, 0.24, 0.00, -0.36, 0.36, 0.00, 0.24,
+ 0.12, -0.20, 0.20, 0.30, -0.12, 0.00, -0.28, 0.30,
+ -0.24, 0.30, 0.12, 0.10, -0.28, -0.30, -0.28, 0.30,
+ 0.00, 0.00, -0.28, -0.30, 0.00, 0.00, -0.28, -0.30,
+ 0.00, 0.00, 0.28, 0.30, 0.00, 0.00, -0.28, -0.30,
+ -0.28, 0.30, 0.00, 0.00, -0.28, -0.30, 0.00, 0.00,
+
+ /* 4052-4179 */
+ 0.28, 0.30, 0.00, 0.00, -0.28, 0.30, 0.28, -0.30,
+ -0.28, 0.30, 0.40, 0.40, -0.24, 0.30, 0.00, -0.10,
+ 0.16, 0.00, 0.36, -0.20, 0.30, -0.12, -0.10, -0.24,
+ -0.30, 0.00, 0.00, -0.24, 0.30, -0.24, 0.30, 0.00,
+ 0.00, -0.24, 0.30, -0.24, 0.30, 0.24, -0.30, 0.00,
+ 0.00, 0.24, -0.30, 0.00, 0.00, 0.24, 0.30, 0.24,
+ -0.30, 0.24, 0.30, -0.24, 0.30, -0.24, 0.30, -0.20,
+ 0.20, -0.16, -0.20, 0.00, 0.00, -0.32, 0.20, 0.00,
+ 0.10, 0.20, -0.30, 0.20, -0.20, 0.12, 0.20, -0.16,
+ 0.20, 0.16, 0.20, 0.20, 0.30, 0.20, 0.30, 0.00,
+ 0.00, -0.20, 0.30, 0.00, 0.00, 0.20, 0.30, -0.20,
+ -0.30, -0.20, -0.30, 0.20, -0.30, 0.00, 0.00, 0.20,
+ 0.30, 0.00, 0.00, 0.20, 0.30, 0.00, 0.00, 0.20,
+ 0.30, 0.00, 0.00, 0.20, 0.30, 0.00, 0.00, 0.20,
+ -0.30, 0.00, 0.00, -0.20, -0.30, 0.00, 0.00, -0.20,
+ 0.30, 0.00, 0.00, -0.20, 0.30, 0.00, 0.00, 0.36,
+
+ /* 4180-4307 */
+ 0.00, 0.00, 0.36, 0.12, 0.10, -0.24, 0.20, 0.12,
+ -0.20, -0.16, -0.20, -0.13, 0.10, 0.22, 0.21, 0.20,
+ 0.00, -0.28, 0.32, 0.00, -0.12, -0.20, -0.20, 0.12,
+ -0.10, 0.12, 0.10, -0.20, 0.20, 0.00, 0.00, -0.32,
+ 0.32, 0.00, 0.00, 0.32, 0.32, 0.00, 0.00, -0.24,
+ -0.20, 0.24, 0.20, 0.20, 0.00, -0.24, 0.00, 0.00,
+ -0.24, -0.20, 0.00, 0.00, 0.24, 0.20, -0.24, -0.20,
+ 0.00, 0.00, -0.24, 0.20, 0.16, -0.20, 0.12, 0.10,
+ 0.20, 0.20, 0.00, -0.10, -0.12, 0.10, -0.16, -0.20,
+ -0.12, -0.10, -0.16, 0.20, 0.20, 0.20, 0.00, 0.00,
+ -0.20, 0.20, -0.20, 0.20, -0.20, 0.20, -0.20, 0.20,
+ 0.20, -0.20, -0.20, -0.20, 0.00, 0.00, -0.20, 0.20,
+ 0.20, 0.00, -0.20, 0.00, 0.00, -0.20, 0.20, -0.20,
+ 0.20, -0.20, -0.20, -0.20, -0.20, 0.00, 0.00, 0.20,
+ 0.20, 0.20, 0.20, 0.12, -0.20, -0.12, -0.10, 0.28,
+ -0.28, 0.16, -0.20, 0.00, -0.10, 0.00, 0.10, -0.16,
+
+ /* 4308-4435 */
+ 0.20, 0.00, -0.10, -0.16, -0.20, 0.00, -0.10, 0.16,
+ -0.20, 0.16, -0.20, 0.00, 0.00, 0.16, 0.20, -0.16,
+ 0.20, 0.00, 0.00, 0.16, 0.20, 0.16, -0.20, 0.16,
+ -0.20, -0.16, 0.20, 0.16, -0.20, 0.00, 0.00, 0.16,
+ 0.20, 0.00, 0.00, 0.16, 0.20, 0.00, 0.00, -0.16,
+ -0.20, 0.16, -0.20, -0.16, -0.20, 0.00, 0.00, -0.16,
+ -0.20, 0.00, 0.00, -0.16, 0.20, 0.00, 0.00, 0.16,
+ -0.20, 0.16, 0.20, 0.16, 0.20, 0.00, 0.00, -0.16,
+ -0.20, 0.00, 0.00, -0.16, -0.20, 0.00, 0.00, 0.16,
+ 0.20, 0.16, 0.20, 0.00, 0.00, 0.16, 0.20, 0.16,
+ -0.20, 0.16, 0.20, 0.00, 0.00, -0.16, 0.20, 0.00,
+ 0.10, 0.12, -0.20, 0.12, -0.20, 0.00, -0.10, 0.00,
+ -0.10, 0.12, 0.20, 0.00, -0.10, -0.12, 0.20, -0.15,
+ 0.20, -0.24, 0.24, 0.00, 0.00, 0.24, 0.24, 0.12,
+ -0.20, -0.12, -0.20, 0.00, 0.00, 0.12, 0.20, 0.12,
+ -0.20, 0.12, 0.20, 0.12, 0.20, 0.12, 0.20, 0.12,
+
+ /* 4436-4563 */
+ -0.20, -0.12, 0.20, 0.00, 0.00, 0.12, 0.20, 0.12,
+ 0.00, -0.20, 0.00, 0.00, -0.12, -0.20, 0.12, -0.20,
+ 0.00, 0.00, 0.12, 0.20, -0.12, 0.20, -0.12, 0.20,
+ 0.12, -0.20, 0.00, 0.00, 0.12, 0.20, 0.20, 0.00,
+ 0.12, 0.00, 0.00, -0.12, 0.20, 0.00, 0.00, -0.12,
+ -0.20, 0.00, 0.00, -0.12, -0.20, -0.12, -0.20, 0.00,
+ 0.00, 0.12, -0.20, 0.12, -0.20, 0.12, 0.20, -0.12,
+ -0.20, 0.00, 0.00, 0.12, -0.20, 0.12, -0.20, 0.12,
+ 0.20, 0.12, 0.00, 0.20, -0.12, -0.20, 0.00, 0.00,
+ 0.12, 0.20, -0.16, 0.00, 0.16, -0.20, 0.20, 0.00,
+ 0.00, -0.20, 0.00, 0.00, -0.20, 0.20, 0.00, 0.00,
+ 0.20, 0.20, -0.20, 0.00, 0.00, -0.20, 0.12, 0.00,
+ -0.16, 0.20, 0.00, 0.00, 0.20, 0.12, -0.10, 0.00,
+ 0.10, 0.16, -0.16, -0.16, -0.16, -0.16, -0.16, 0.00,
+ 0.00, -0.16, 0.00, 0.00, -0.16, -0.16, -0.16, 0.00,
+ 0.00, -0.16, 0.00, 0.00, 0.16, 0.00, 0.00, 0.16,
+
+ /* 4564-4691 */
+ 0.00, 0.00, 0.16, 0.16, 0.00, 0.00, -0.16, 0.00,
+ 0.00, -0.16, -0.16, 0.00, 0.00, 0.16, 0.00, 0.00,
+ -0.16, -0.16, 0.00, 0.00, -0.16, -0.16, 0.12, 0.10,
+ 0.12, -0.10, 0.12, 0.10, 0.00, 0.00, 0.12, 0.10,
+ -0.12, 0.10, 0.00, 0.00, 0.12, 0.10, 0.12, -0.10,
+ 0.00, 0.00, -0.12, -0.10, 0.00, 0.00, 0.12, 0.10,
+ 0.12, 0.00, 0.00, 0.12, 0.00, 0.00, -0.12, 0.00,
+ 0.00, 0.12, 0.12, 0.12, 0.12, 0.12, 0.00, 0.00,
+ 0.12, 0.00, 0.00, 0.12, 0.12, 0.00, 0.00, 0.12,
+ 0.00, 0.00, 0.12, -0.12, -0.12, 0.12, 0.12, -0.12,
+ -0.12, 0.00, 0.00, 0.12, -0.12, 0.12, 0.12, -0.12,
+ -0.12, 0.00, 0.00, -0.12, -0.12, 0.00, 0.00, -0.12,
+ 0.12, 0.00, 0.00, 0.12, 0.00, 0.00, 0.12, 0.00,
+ 0.00, 0.12, -0.12, 0.00, 0.00, -0.12, 0.12, -0.12,
+ -0.12, 0.12, 0.00, 0.00, 0.12, 0.12, 0.12, -0.12,
+ 0.00, 0.00, -0.12, -0.12, -0.12, 0.00, 0.00, -0.12,
+
+ /* 4692-NA */
+ -0.12, 0.00, 0.00, 0.12, 0.12, 0.00, 0.00, -0.12,
+ -0.12, -0.12, -0.12, 0.12, 0.00, 0.00, 0.12, -0.12,
+ 0.00, 0.00, -0.12, -0.12, 0.00, 0.00, 0.12, -0.12,
+ -0.12, -0.12, -0.12, 0.12, 0.12, -0.12, -0.12, 0.00,
+ 0.00, -0.12, 0.00, 0.00, -0.12, 0.12, 0.00, 0.00,
+ 0.12, 0.00, 0.00, -0.12, -0.12, 0.00, 0.00, -0.12,
+ -0.12, 0.12, 0.00, 0.00, 0.12, 0.12, 0.00, 0.00,
+ 0.12, 0.00, 0.00, 0.12, 0.12, 0.08, 0.00, 0.04
+ };
+
+/* Number of amplitude coefficients */
+ static const int NA = (int) (sizeof a / sizeof (double));
+
+/* Amplitude usage: X or Y, sin or cos, power of T. */
+ static const int jaxy[] = {0,1,0,1,0,1,0,1,0,1,0,1,0,1,0,1,0,1,0,1};
+ static const int jasc[] = {0,1,1,0,1,0,0,1,0,1,1,0,1,0,0,1,0,1,1,0};
+ static const int japt[] = {0,0,0,0,1,1,1,1,2,2,2,2,3,3,3,3,4,4,4,4};
+
+/* Miscellaneous */
+ double t, w, pt[MAXPT+1], fa[14], xypr[2], xypl[2], xyls[2], arg,
+ sc[2];
+ int jpt, i, j, jxy, ialast, ifreq, m, ia, jsc;
+
+/*--------------------------------------------------------------------*/
+
+/* Interval between fundamental date J2000.0 and given date (JC). */
+ t = ((date1 - DJ00) + date2) / DJC;
+
+/* Powers of T. */
+ w = 1.0;
+ for (jpt = 0; jpt <= MAXPT; jpt++) {
+ pt[jpt] = w;
+ w *= t;
+ }
+
+/* Initialize totals in X and Y: polynomial, luni-solar, planetary. */
+ for (jxy = 0; jxy < 2; jxy++) {
+ xypr[jxy] = 0.0;
+ xyls[jxy] = 0.0;
+ xypl[jxy] = 0.0;
+ }
+
+/* --------------------------------- */
+/* Fundamental arguments (IERS 2003) */
+/* --------------------------------- */
+
+/* Mean anomaly of the Moon. */
+ fa[0] = iauFal03(t);
+
+/* Mean anomaly of the Sun. */
+ fa[1] = iauFalp03(t);
+
+/* Mean argument of the latitude of the Moon. */
+ fa[2] = iauFaf03(t);
+
+/* Mean elongation of the Moon from the Sun. */
+ fa[3] = iauFad03(t);
+
+/* Mean longitude of the ascending node of the Moon. */
+ fa[4] = iauFaom03(t);
+
+/* Planetary longitudes, Mercury through Neptune. */
+ fa[5] = iauFame03(t);
+ fa[6] = iauFave03(t);
+ fa[7] = iauFae03(t);
+ fa[8] = iauFama03(t);
+ fa[9] = iauFaju03(t);
+ fa[10] = iauFasa03(t);
+ fa[11] = iauFaur03(t);
+ fa[12] = iauFane03(t);
+
+/* General accumulated precession in longitude. */
+ fa[13] = iauFapa03(t);
+
+/* -------------------------------------- */
+/* Polynomial part of precession-nutation */
+/* -------------------------------------- */
+
+ for (jxy = 0; jxy < 2; jxy++) {
+ for (j = MAXPT; j >= 0; j--) {
+ xypr[jxy] += xyp[jxy][j] * pt[j];
+ }
+ }
+
+/* ---------------------------------- */
+/* Nutation periodic terms, planetary */
+/* ---------------------------------- */
+
+/* Work backwards through the coefficients per frequency list. */
+ ialast = NA;
+ for (ifreq = NFPL-1; ifreq >= 0; ifreq--) {
+
+ /* Obtain the argument functions. */
+ arg = 0.0;
+ for (i = 0; i < 14; i++) {
+ m = mfapl[ifreq][i];
+ if (m != 0) arg += (double)m * fa[i];
+ }
+ sc[0] = sin(arg);
+ sc[1] = cos(arg);
+
+ /* Work backwards through the amplitudes at this frequency. */
+ ia = nc[ifreq+NFLS];
+ for (i = ialast; i >= ia; i--) {
+
+ /* Coefficient number (0 = 1st). */
+ j = i-ia;
+
+ /* X or Y. */
+ jxy = jaxy[j];
+
+ /* Sin or cos. */
+ jsc = jasc[j];
+
+ /* Power of T. */
+ jpt = japt[j];
+
+ /* Accumulate the component. */
+ xypl[jxy] += a[i-1] * sc[jsc] * pt[jpt];
+ }
+ ialast = ia-1;
+ }
+
+/* ----------------------------------- */
+/* Nutation periodic terms, luni-solar */
+/* ----------------------------------- */
+
+/* Continue working backwards through the number of coefficients list. */
+ for (ifreq = NFLS-1; ifreq >= 0; ifreq--) {
+
+ /* Obtain the argument functions. */
+ arg = 0.0;
+ for (i = 0; i < 5; i++) {
+ m = mfals[ifreq][i];
+ if (m != 0) arg += (double)m * fa[i];
+ }
+ sc[0] = sin(arg);
+ sc[1] = cos(arg);
+
+ /* Work backwards through the amplitudes at this frequency. */
+ ia = nc[ifreq];
+ for (i = ialast; i >= ia; i--) {
+
+ /* Coefficient number (0 = 1st). */
+ j = i-ia;
+
+ /* X or Y. */
+ jxy = jaxy[j];
+
+ /* Sin or cos. */
+ jsc = jasc[j];
+
+ /* Power of T. */
+ jpt = japt[j];
+
+ /* Accumulate the component. */
+ xyls[jxy] += a[i-1] * sc[jsc] * pt[jpt];
+ }
+ ialast = ia-1;
+ }
+
+/* ------------------------------------ */
+/* Results: CIP unit vector components */
+/* ------------------------------------ */
+
+ *x = DAS2R * (xypr[0] + (xyls[0] + xypl[0]) / 1e6);
+ *y = DAS2R * (xypr[1] + (xyls[1] + xypl[1]) / 1e6);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/xys00a.c b/sofa/xys00a.c
new file mode 100644
index 0000000..57f8607
--- /dev/null
+++ b/sofa/xys00a.c
@@ -0,0 +1,183 @@
+#include "sofam.h"
+
+void iauXys00a(double date1, double date2,
+ double *x, double *y, double *s)
+/*
+** - - - - - - - - - -
+** i a u X y s 0 0 a
+** - - - - - - - - - -
+**
+** For a given TT date, compute the X,Y coordinates of the Celestial
+** Intermediate Pole and the CIO locator s, using the IAU 2000A
+** precession-nutation model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** x,y double Celestial Intermediate Pole (Note 2)
+** s double the CIO locator s (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The Celestial Intermediate Pole coordinates are the x,y
+** components of the unit vector in the Geocentric Celestial
+** Reference System.
+**
+** 3) The CIO locator s (in radians) positions the Celestial
+** Intermediate Origin on the equator of the CIP.
+**
+** 4) A faster, but slightly less accurate result (about 1 mas for
+** X,Y), can be obtained by using instead the iauXys00b function.
+**
+** Called:
+** iauPnm00a classical NPB matrix, IAU 2000A
+** iauBpn2xy extract CIP X,Y coordinates from NPB matrix
+** iauS00 the CIO locator s, given X,Y, IAU 2000A
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2008 May 12
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rbpn[3][3];
+
+
+/* Form the bias-precession-nutation matrix, IAU 2000A. */
+ iauPnm00a(date1, date2, rbpn);
+
+/* Extract X,Y. */
+ iauBpn2xy(rbpn, x, y);
+
+/* Obtain s. */
+ *s = iauS00(date1, date2, *x, *y);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/xys00b.c b/sofa/xys00b.c
new file mode 100644
index 0000000..1f4f2b0
--- /dev/null
+++ b/sofa/xys00b.c
@@ -0,0 +1,183 @@
+#include "sofam.h"
+
+void iauXys00b(double date1, double date2,
+ double *x, double *y, double *s)
+/*
+** - - - - - - - - - -
+** i a u X y s 0 0 b
+** - - - - - - - - - -
+**
+** For a given TT date, compute the X,Y coordinates of the Celestial
+** Intermediate Pole and the CIO locator s, using the IAU 2000B
+** precession-nutation model.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** x,y double Celestial Intermediate Pole (Note 2)
+** s double the CIO locator s (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The Celestial Intermediate Pole coordinates are the x,y
+** components of the unit vector in the Geocentric Celestial
+** Reference System.
+**
+** 3) The CIO locator s (in radians) positions the Celestial
+** Intermediate Origin on the equator of the CIP.
+**
+** 4) The present function is faster, but slightly less accurate (about
+** 1 mas in X,Y), than the iauXys00a function.
+**
+** Called:
+** iauPnm00b classical NPB matrix, IAU 2000B
+** iauBpn2xy extract CIP X,Y coordinates from NPB matrix
+** iauS00 the CIO locator s, given X,Y, IAU 2000A
+**
+** Reference:
+**
+** McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
+** IERS Technical Note No. 32, BKG (2004)
+**
+** This revision: 2008 May 12
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rbpn[3][3];
+
+
+/* Form the bias-precession-nutation matrix, IAU 2000A. */
+ iauPnm00b(date1, date2, rbpn);
+
+/* Extract X,Y. */
+ iauBpn2xy(rbpn, x, y);
+
+/* Obtain s. */
+ *s = iauS00(date1, date2, *x, *y);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/xys06a.c b/sofa/xys06a.c
new file mode 100644
index 0000000..f892054
--- /dev/null
+++ b/sofa/xys06a.c
@@ -0,0 +1,183 @@
+#include "sofam.h"
+
+void iauXys06a(double date1, double date2,
+ double *x, double *y, double *s)
+/*
+** - - - - - - - - - -
+** i a u X y s 0 6 a
+** - - - - - - - - - -
+**
+** For a given TT date, compute the X,Y coordinates of the Celestial
+** Intermediate Pole and the CIO locator s, using the IAU 2006
+** precession and IAU 2000A nutation models.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: support function.
+**
+** Given:
+** date1,date2 double TT as a 2-part Julian Date (Note 1)
+**
+** Returned:
+** x,y double Celestial Intermediate Pole (Note 2)
+** s double the CIO locator s (Note 2)
+**
+** Notes:
+**
+** 1) The TT date date1+date2 is a Julian Date, apportioned in any
+** convenient way between the two arguments. For example,
+** JD(TT)=2450123.7 could be expressed in any of these ways,
+** among others:
+**
+** date1 date2
+**
+** 2450123.7 0.0 (JD method)
+** 2451545.0 -1421.3 (J2000 method)
+** 2400000.5 50123.2 (MJD method)
+** 2450123.5 0.2 (date & time method)
+**
+** The JD method is the most natural and convenient to use in
+** cases where the loss of several decimal digits of resolution
+** is acceptable. The J2000 method is best matched to the way
+** the argument is handled internally and will deliver the
+** optimum resolution. The MJD method and the date & time methods
+** are both good compromises between resolution and convenience.
+**
+** 2) The Celestial Intermediate Pole coordinates are the x,y components
+** of the unit vector in the Geocentric Celestial Reference System.
+**
+** 3) The CIO locator s (in radians) positions the Celestial
+** Intermediate Origin on the equator of the CIP.
+**
+** 4) Series-based solutions for generating X and Y are also available:
+** see Capitaine & Wallace (2006) and iauXy06.
+**
+** Called:
+** iauPnm06a classical NPB matrix, IAU 2006/2000A
+** iauBpn2xy extract CIP X,Y coordinates from NPB matrix
+** iauS06 the CIO locator s, given X,Y, IAU 2006
+**
+** References:
+**
+** Capitaine, N. & Wallace, P.T., 2006, Astron.Astrophys. 450, 855
+**
+** Wallace, P.T. & Capitaine, N., 2006, Astron.Astrophys. 459, 981
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ double rbpn[3][3];
+
+
+/* Form the bias-precession-nutation matrix, IAU 2000A. */
+ iauPnm06a(date1, date2, rbpn);
+
+/* Extract X,Y. */
+ iauBpn2xy(rbpn, x, y);
+
+/* Obtain s. */
+ *s = iauS06(date1, date2, *x, *y);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/zp.c b/sofa/zp.c
new file mode 100644
index 0000000..a07504f
--- /dev/null
+++ b/sofa/zp.c
@@ -0,0 +1,127 @@
+#include "sofam.h"
+
+void iauZp(double p[3])
+/*
+** - - - - - -
+** i a u Z p
+** - - - - - -
+**
+** Zero a p-vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Returned:
+** p double[3] p-vector
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ p[0] = 0.0;
+ p[1] = 0.0;
+ p[2] = 0.0;
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/zpv.c b/sofa/zpv.c
new file mode 100644
index 0000000..c725fb4
--- /dev/null
+++ b/sofa/zpv.c
@@ -0,0 +1,129 @@
+#include "sofam.h"
+
+void iauZpv(double pv[2][3])
+/*
+** - - - - - - -
+** i a u Z p v
+** - - - - - - -
+**
+** Zero a pv-vector.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Returned:
+** pv double[2][3] pv-vector
+**
+** Called:
+** iauZp zero p-vector
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ iauZp(pv[0]);
+ iauZp(pv[1]);
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa/zr.c b/sofa/zr.c
new file mode 100644
index 0000000..7af1b6f
--- /dev/null
+++ b/sofa/zr.c
@@ -0,0 +1,132 @@
+#include "sofam.h"
+
+void iauZr(double r[3][3])
+/*
+** - - - - - -
+** i a u Z r
+** - - - - - -
+**
+** Initialize an r-matrix to the null matrix.
+**
+** This function is part of the International Astronomical Union's
+** SOFA (Standards Of Fundamental Astronomy) software collection.
+**
+** Status: vector/matrix support function.
+**
+** Returned:
+** r double[3][3] r-matrix
+**
+** This revision: 2008 May 11
+**
+** SOFA release 2012-03-01
+**
+** Copyright (C) 2012 IAU SOFA Board. See notes at end.
+*/
+{
+ int i, j;
+
+
+ for (i = 0; i < 3; i++) {
+ for (j = 0; j < 3; j++) {
+ r[i][j] = 0.0;
+ }
+ }
+
+ return;
+
+/*----------------------------------------------------------------------
+**
+** Copyright (C) 2012
+** Standards Of Fundamental Astronomy Board
+** of the International Astronomical Union.
+**
+** =====================
+** SOFA Software License
+** =====================
+**
+** NOTICE TO USER:
+**
+** BY USING THIS SOFTWARE YOU ACCEPT THE FOLLOWING SIX TERMS AND
+** CONDITIONS WHICH APPLY TO ITS USE.
+**
+** 1. The Software is owned by the IAU SOFA Board ("SOFA").
+**
+** 2. Permission is granted to anyone to use the SOFA software for any
+** purpose, including commercial applications, free of charge and
+** without payment of royalties, subject to the conditions and
+** restrictions listed below.
+**
+** 3. You (the user) may copy and distribute SOFA source code to others,
+** and use and adapt its code and algorithms in your own software,
+** on a world-wide, royalty-free basis. That portion of your
+** distribution that does not consist of intact and unchanged copies
+** of SOFA source code files is a "derived work" that must comply
+** with the following requirements:
+**
+** a) Your work shall be marked or carry a statement that it
+** (i) uses routines and computations derived by you from
+** software provided by SOFA under license to you; and
+** (ii) does not itself constitute software provided by and/or
+** endorsed by SOFA.
+**
+** b) The source code of your derived work must contain descriptions
+** of how the derived work is based upon, contains and/or differs
+** from the original SOFA software.
+**
+** c) The names of all routines in your derived work shall not
+** include the prefix "iau" or "sofa" or trivial modifications
+** thereof such as changes of case.
+**
+** d) The origin of the SOFA components of your derived work must
+** not be misrepresented; you must not claim that you wrote the
+** original software, nor file a patent application for SOFA
+** software or algorithms embedded in the SOFA software.
+**
+** e) These requirements must be reproduced intact in any source
+** distribution and shall apply to anyone to whom you have
+** granted a further right to modify the source code of your
+** derived work.
+**
+** Note that, as originally distributed, the SOFA software is
+** intended to be a definitive implementation of the IAU standards,
+** and consequently third-party modifications are discouraged. All
+** variations, no matter how minor, must be explicitly marked as
+** such, as explained above.
+**
+** 4. You shall not cause the SOFA software to be brought into
+** disrepute, either by misuse, or use for inappropriate tasks, or
+** by inappropriate modification.
+**
+** 5. The SOFA software is provided "as is" and SOFA makes no warranty
+** as to its use or performance. SOFA does not and cannot warrant
+** the performance or results which the user may obtain by using the
+** SOFA software. SOFA makes no warranties, express or implied, as
+** to non-infringement of third party rights, merchantability, or
+** fitness for any particular purpose. In no event will SOFA be
+** liable to the user for any consequential, incidental, or special
+** damages, including any lost profits or lost savings, even if a
+** SOFA representative has been advised of such damages, or for any
+** claim by any third party.
+**
+** 6. The provision of any version of the SOFA software under the terms
+** and conditions specified herein does not imply that future
+** versions will also be made available under the same terms and
+** conditions.
+*
+** In any published work or commercial product which uses the SOFA
+** software directly, acknowledgement (see www.iausofa.org) is
+** appreciated.
+**
+** Correspondence concerning SOFA software should be addressed as
+** follows:
+**
+** By email: sofa at ukho.gov.uk
+** By post: IAU SOFA Center
+** HM Nautical Almanac Office
+** UK Hydrographic Office
+** Admiralty Way, Taunton
+** Somerset, TA1 2DN
+** United Kingdom
+**
+**--------------------------------------------------------------------*/
+}
diff --git a/sofa2ast.h b/sofa2ast.h
new file mode 100644
index 0000000..f1aa9a0
--- /dev/null
+++ b/sofa2ast.h
@@ -0,0 +1,247 @@
+#if !defined( SOFA2AST_INCLUDED ) /* Include this file only once */
+#define SOFA2AST_INCLUDED
+/*
+* Name:
+* sofa2ast.h
+
+* Type:
+* C include file.
+
+* Purpose:
+* Defines new names for symbols exported by the IAU SOFA library.
+
+* Invocation:
+* #include "sofa2ast.h"
+
+* Description:
+* This include file defines a new name for each public function
+* defined by the SOFA library. The names defined by SOFA itself are
+* of the form "iauXxx" (e.g. iauPmp) - this include file defines
+* a macro that translates each such name to the form "astIauXxx"
+* (e.g. astIauPmp). This is done so that the names do not clash
+* with any external SOFA library with which the application is linked.
+*
+* It should be included at the start of any AST source file that refers
+* to SOFA functions using the standard names (e.g. iauPmp).
+
+* Copyright:
+* Copyright (C) 2012 Science & Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public Licence as
+* published by the Free Software Foundation; either version 2 of
+* the Licence, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful,but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public Licence for more details.
+*
+* You should have received a copy of the GNU General Public Licence
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street,Fifth Floor, Boston, MA
+* 02110-1301, USA
+
+* Authors:
+* DSB: D.S. Berry (Starlink)
+
+* History:
+* 16-FEB-2012 (DSB):
+* Original version.
+*/
+
+/* Rename all SOFA functions called directlty from PAL. */
+#define iauAf2a astIauAf2a
+#define iauAnp astIauAnp
+#define iauAnpm astIauAnpm
+#define iauC2s astIauC2s
+#define iauCal2jd astIauCal2jd
+#define iauD2tf astIauD2tf
+#define iauDat astIauDat
+#define iauEe06a astIauEe06a
+#define iauEpb astIauEpb
+#define iauEpb2jd astIauEpb2jd
+#define iauEpj astIauEpj
+#define iauEpj2jd astIauEpj2jd
+#define iauEpv00 astIauEpv00
+#define iauFk5hz astIauFk5hz
+#define iauGd2gc astIauGd2gc
+#define iauGmst06 astIauGmst06
+#define iauHfk5z astIauHfk5z
+#define iauIr astIauIr
+#define iauJd2cal astIauJd2cal
+#define iauObl06 astIauObl06
+#define iauP06e astIauP06e
+#define iauPap astIauPap
+#define iauPas astIauPas
+#define iauPdp astIauPdp
+#define iauPmat06 astIauPmat06
+#define iauPn astIauPn
+#define iauPnm06a astIauPnm06a
+#define iauPxp astIauPxp
+#define iauRm2v astIauRm2v
+#define iauRv2m astIauRv2m
+#define iauRx astIauRx
+#define iauRxp astIauRxp
+#define iauRxpv astIauRxpv
+#define iauRxr astIauRxr
+#define iauRy astIauRy
+#define iauRz astIauRz
+#define iauS2c astIauS2c
+#define iauSepp astIauSepp
+#define iauSeps astIauSeps
+#define iauTf2a astIauTf2a
+#define iauTf2d astIauTf2d
+#define iauTr astIauTr
+#define iauTrxp astIauTrxp
+
+
+/* Rename all SOFA functions called internally within the above SOFA
+ functions. */
+#define iauA2af astIauA2af
+#define iauA2tf astIauA2tf
+#define iauBi00 astIauBi00
+#define iauBp00 astIauBp00
+#define iauBp06 astIauBp06
+#define iauBpn2xy astIauBpn2xy
+#define iauC2i00a astIauC2i00a
+#define iauC2i00b astIauC2i00b
+#define iauC2i06a astIauC2i06a
+#define iauC2ibpn astIauC2ibpn
+#define iauC2ixy astIauC2ixy
+#define iauC2ixys astIauC2ixys
+#define iauC2t00a astIauC2t00a
+#define iauC2t00b astIauC2t00b
+#define iauC2t06a astIauC2t06a
+#define iauC2tcio astIauC2tcio
+#define iauC2teqx astIauC2teqx
+#define iauC2tpe astIauC2tpe
+#define iauC2txy astIauC2txy
+#define iauCp astIauCp
+#define iauCpv astIauCpv
+#define iauCr astIauCr
+#define iauD2dtf astIauD2dtf
+#define iauDtdb astIauDtdb
+#define iauDtf2d astIauDtf2d
+#define iauEe00 astIauEe00
+#define iauEe00a astIauEe00a
+#define iauEe00b astIauEe00b
+#define iauEect00 astIauEect00
+#define iauEform astIauEform
+#define iauEo06a astIauEo06a
+#define iauEors astIauEors
+#define iauEqeq94 astIauEqeq94
+#define iauEra00 astIauEra00
+#define iauFad03 astIauFad03
+#define iauFae03 astIauFae03
+#define iauFaf03 astIauFaf03
+#define iauFaju03 astIauFaju03
+#define iauFal03 astIauFal03
+#define iauFalp03 astIauFalp03
+#define iauFama03 astIauFama03
+#define iauFame03 astIauFame03
+#define iauFane03 astIauFane03
+#define iauFaom03 astIauFaom03
+#define iauFapa03 astIauFapa03
+#define iauFasa03 astIauFasa03
+#define iauFaur03 astIauFaur03
+#define iauFave03 astIauFave03
+#define iauFk52h astIauFk52h
+#define iauFk5hip astIauFk5hip
+#define iauFw2m astIauFw2m
+#define iauFw2xy astIauFw2xy
+#define iauGc2gd astIauGc2gd
+#define iauGc2gde astIauGc2gde
+#define iauGd2gce astIauGd2gce
+#define iauGmst00 astIauGmst00
+#define iauGmst82 astIauGmst82
+#define iauGst00a astIauGst00a
+#define iauGst00b astIauGst00b
+#define iauGst06 astIauGst06
+#define iauGst06a astIauGst06a
+#define iauGst94 astIauGst94
+#define iauH2fk5 astIauH2fk5
+#define iauJdcalf astIauJdcalf
+#define iauNum00a astIauNum00a
+#define iauNum00b astIauNum00b
+#define iauNum06a astIauNum06a
+#define iauNumat astIauNumat
+#define iauNut00a astIauNut00a
+#define iauNut00b astIauNut00b
+#define iauNut06a astIauNut06a
+#define iauNut80 astIauNut80
+#define iauNutm80 astIauNutm80
+#define iauObl80 astIauObl80
+#define iauP2pv astIauP2pv
+#define iauP2s astIauP2s
+#define iauPb06 astIauPb06
+#define iauPfw06 astIauPfw06
+#define iauPlan94 astIauPlan94
+#define iauPm astIauPm
+#define iauPmat00 astIauPmat00
+#define iauPmat76 astIauPmat76
+#define iauPmp astIauPmp
+#define iauPn00 astIauPn00
+#define iauPn00a astIauPn00a
+#define iauPn00b astIauPn00b
+#define iauPn06 astIauPn06
+#define iauPn06a astIauPn06a
+#define iauPnm00a astIauPnm00a
+#define iauPnm00b astIauPnm00b
+#define iauPnm80 astIauPnm80
+#define iauPom00 astIauPom00
+#define iauPpp astIauPpp
+#define iauPpsp astIauPpsp
+#define iauPr00 astIauPr00
+#define iauPrec76 astIauPrec76
+#define iauPv2p astIauPv2p
+#define iauPv2s astIauPv2s
+#define iauPvdpv astIauPvdpv
+#define iauPvm astIauPvm
+#define iauPvmpv astIauPvmpv
+#define iauPvppv astIauPvppv
+#define iauPvstar astIauPvstar
+#define iauPvu astIauPvu
+#define iauPvup astIauPvup
+#define iauPvxpv astIauPvxpv
+#define iauS00 astIauS00
+#define iauS00a astIauS00a
+#define iauS00b astIauS00b
+#define iauS06 astIauS06
+#define iauS06a astIauS06a
+#define iauS2p astIauS2p
+#define iauS2pv astIauS2pv
+#define iauS2xpv astIauS2xpv
+#define iauSp00 astIauSp00
+#define iauStarpm astIauStarpm
+#define iauStarpv astIauStarpv
+#define iauSxp astIauSxp
+#define iauSxpv astIauSxpv
+#define iauTaitt astIauTaitt
+#define iauTaiut1 astIauTaiut1
+#define iauTaiutc astIauTaiutc
+#define iauTcbtdb astIauTcbtdb
+#define iauTcgtt astIauTcgtt
+#define iauTdbtcb astIauTdbtcb
+#define iauTdbtt astIauTdbtt
+#define iauTrxpv astIauTrxpv
+#define iauTttai astIauTttai
+#define iauTttcg astIauTttcg
+#define iauTttdb astIauTttdb
+#define iauTtut1 astIauTtut1
+#define iauUt1tai astIauUt1tai
+#define iauUt1tt astIauUt1tt
+#define iauUt1utc astIauUt1utc
+#define iauUtctai astIauUtctai
+#define iauUtcut1 astIauUtcut1
+#define iauXy06 astIauXy06
+#define iauXys00a astIauXys00a
+#define iauXys00b astIauXys00b
+#define iauXys06a astIauXys06a
+#define iauZp astIauZp
+#define iauZpv astIauZpv
+#define iauZr astIaunZr
+
+#endif
diff --git a/sofam.h b/sofam.h
new file mode 100644
index 0000000..d848e74
--- /dev/null
+++ b/sofam.h
@@ -0,0 +1,61 @@
+#if !defined( SOFAM_INCLUDED ) /* Include this file only once */
+#define SOFAM_INCLUDED
+/*
+*+
+* Name:
+* sofam.h
+
+* Purpose:
+* Macros defined by the SOFA library.
+
+* Language:
+* Starlink ANSI C
+
+* Type of Module:
+* Include file
+
+* Description:
+* Macros defined by the SOFA library. This is needed by the pal.c
+* file, which includes source files that include "sofam.h" from the
+* current directory (i.e. the main AST source directory), not the
+* sofa subdirectory.
+
+* Authors:
+* DSBJ: David S Berry (JAC, Hawaii)
+* {enter_new_authors_here}
+
+* History:
+* 23-FEB-2012 (DSB):
+* Initial version.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 2012 Science and Technology Facilities Council.
+* All Rights Reserved.
+
+* Licence:
+* This program is free software; you can redistribute it and/or
+* modify it under the terms of the GNU General Public License as
+* published by the Free Software Foundation; either version 3 of
+* the License, or (at your option) any later version.
+*
+* This program is distributed in the hope that it will be
+* useful, but WITHOUT ANY WARRANTY; without even the implied
+* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR
+* PURPOSE. See the GNU General Public License for more details.
+*
+* You should have received a copy of the GNU General Public License
+* along with this program; if not, write to the Free Software
+* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301
+* USA.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+/* Include the macros defined in the corresponding header file in the
+ sofa subdirectory. */
+#include "sofa/sofam.h"
+
+#endif
diff --git a/specmap.c b/specmap.c
index 39878da..81808d9 100644
--- a/specmap.c
+++ b/specmap.c
@@ -749,13 +749,13 @@ static double BaryVel( double ra, double dec, FrameDef *def, int *status ) {
/* Get the Cartesian vector towards the source, in the Cartesian FK5
J2000 system. */
- palSlaDcs2c( ra, dec, v );
+ palDcs2c( ra, dec, v );
/* If not already done so, get the Earth/Sun velocity and position vectors in
the same system. Speed is returned in units of AU/s. Store in the supplied
frame definition structure. */
if( def->dvb[ 0 ] == AST__BAD ) {
- palSlaEvp( def->epoch, 2000.0, def->dvb, dpb, dvh, dph );
+ palEvp( def->epoch, 2000.0, def->dvb, dpb, dvh, dph );
/* Change the barycentric velocity of the earth into the heliocentric
velocity of the barycentre. */
@@ -766,7 +766,7 @@ static double BaryVel( double ra, double dec, FrameDef *def, int *status ) {
/* Return the component away from the source, of the velocity of the
barycentre relative to the sun (in m/s). */
- return -palSlaDvdv( v, def->dvb )*149.597870E9;
+ return -palDvdv( v, def->dvb )*149.597870E9;
}
@@ -1754,11 +1754,11 @@ static double GalVel( double ra, double dec, FrameDef *def, int *status ) {
/* Get the component away from the source, of the velocity of the sun
relative to the dynamic LSR (in km/s). */
- s1 = (double) palSlaRvlsrd( (float) ra, (float) dec );
+ s1 = (double) palRvlsrd( (float) ra, (float) dec );
/* Get the component away from the source, of the velocity of the
dynamic LSR relative to the galactic centre (in km/s). */
- s2 = (double) palSlaRvgalc( (float) ra, (float) dec );
+ s2 = (double) palRvgalc( (float) ra, (float) dec );
/* Return the total velocity of the galactic centre away from the source,
relative to the sun, in m/s. */
@@ -1817,17 +1817,17 @@ static double GeoVel( double ra, double dec, FrameDef *def, int *status ) {
/* Get the Cartesian vector towards the source, in the Cartesian FK5
J2000 system. */
- palSlaDcs2c( ra, dec, v );
+ palDcs2c( ra, dec, v );
/* If not already done so, get the Earth/Sun velocity and position vectors in
the same system. Speed is returned in units of AU/s. Store in the supplied
frame definition structure. */
- if( def->dvh[ 0 ] == AST__BAD ) palSlaEvp( def->epoch, 2000.0, dvb, dpb,
+ if( def->dvh[ 0 ] == AST__BAD ) palEvp( def->epoch, 2000.0, dvb, dpb,
def->dvh, dph );
/* Return the component away from the source, of the velocity of the earths
centre relative to the sun (in m/s). */
- return -palSlaDvdv( v, def->dvh )*149.597870E9;
+ return -palDvdv( v, def->dvh )*149.597870E9;
}
void astInitSpecMapVtab_( AstSpecMapVtab *vtab, const char *name, int *status ) {
@@ -1970,7 +1970,7 @@ static double LgVel( double ra, double dec, FrameDef *def, int *status ) {
/* Return the component away from the source, of the velocity of the
local group relative to the sun (in m/s). */
- return -1000.0*palSlaRvlg( (float) ra, (float) dec );
+ return -1000.0*palRvlg( (float) ra, (float) dec );
}
static double LsrdVel( double ra, double dec, FrameDef *def, int *status ) {
@@ -2020,7 +2020,7 @@ static double LsrdVel( double ra, double dec, FrameDef *def, int *status ) {
relative to the dynamical LSR (in m/s). This can also be thought of as the
velocity of the LSR towards the source relative to the sun. Return the
negated value (i.e. velocity of lsrd *away from* the source. */
- return -1000.0*palSlaRvlsrd( (float) ra, (float) dec );
+ return -1000.0*palRvlsrd( (float) ra, (float) dec );
}
static double LsrkVel( double ra, double dec, FrameDef *def, int *status ) {
@@ -2070,7 +2070,7 @@ static double LsrkVel( double ra, double dec, FrameDef *def, int *status ) {
relative to the kinematic LSR (in m/s). This can also be thought of as the
velocity of the LSR towards the source relative to the sun. Return the
negated value (i.e. velocity of lsrk *away from* the source. */
- return -1000.0*palSlaRvlsrk( (float) ra, (float) dec );
+ return -1000.0*palRvlsrk( (float) ra, (float) dec );
}
static int MapMerge( AstMapping *this, int where, int series, int *nmap,
@@ -2822,14 +2822,14 @@ static double Rverot( double phi, double h, double ra, double da,
/* Get the Cartesian coordinates of the unit vector pointing towards the
given sky position. */
- palSlaDcs2c( ra, da, v );
+ palDcs2c( ra, da, v );
/* Get velocity and position of the observer. */
- palSlaPvobs( phi, h, st, pv );
+ palPvobs( phi, h, st, pv );
/* Return the component of the observer's velocity away from the sky
position, and convert from AU/s to km/s. */
- return -palSlaDvdv( v, pv + 3 )*149.597870E6;
+ return -palDvdv( v, pv + 3 )*149.597870E6;
}
static void SpecAdd( AstSpecMap *this, const char *cvt, const double args[], int *status ) {
@@ -3545,16 +3545,16 @@ static double TopoVel( double ra, double dec, FrameDef *def, int *status ) {
/* If not already done so, get the parameters defining the transformation
of mean ra and dec to apparent ra and dec, and store in the supplied frame
definition structure. */
- if( def->amprms[ 0 ] == AST__BAD ) palSlaMappa( 2000.0, def->epoch,
+ if( def->amprms[ 0 ] == AST__BAD ) palMappa( 2000.0, def->epoch,
def->amprms );
/* Convert the source position from mean ra and dec to apparent ra and dec. */
- palSlaMapqkz( ra, dec, def->amprms, &raa, &deca );
+ palMapqkz( ra, dec, def->amprms, &raa, &deca );
/* If not already done so, get the local apparent siderial time (in radians)
and store in the supplied frame definition structure. */
- if( def->last == AST__BAD ) def->last = palSlaGmst( def->epoch ) +
- palSlaEqeqx( def->epoch ) +
+ if( def->last == AST__BAD ) def->last = palGmst( def->epoch ) +
+ palEqeqx( def->epoch ) +
def->obslon;
/* Get the component away from the source, of the velocity of the observer
@@ -3798,12 +3798,12 @@ static double UserVel( double ra, double dec, FrameDef *def, int *status ) {
}
/* Convert given J2000 RA,Dec to x,y,z. */
- palSlaDcs2c( ra, dec, vb );
+ palDcs2c( ra, dec, vb );
/* Return the dot product with the user velocity. Invert it to get the
velocity towards the observer (the def->veluser value is supposed to be
positive if the source is moving away from the observer). */
- return -palSlaDvdv( def->vuser, vb );
+ return -palDvdv( def->vuser, vb );
}
/* Copy constructor. */
diff --git a/sphmap.c b/sphmap.c
index 8707f05..915d278 100644
--- a/sphmap.c
+++ b/sphmap.c
@@ -1079,7 +1079,7 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
/* Otherwise use a SLALIB function to do the conversion (SLALIB always
returns zero at either pole which is why we make the above check). */
} else {
- palSlaDcc2s( v, q0++, q1++ );
+ palDcc2s( v, q0++, q1++ );
}
} else {
@@ -1106,7 +1106,7 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
/* Apply the mapping to every point. */
for( point = 0; point < npoint; point++ ){
if( *q0 != AST__BAD && *q1 != AST__BAD ){
- palSlaDcs2c( *q0, *q1, v );
+ palDcs2c( *q0, *q1, v );
*(p0++) = v[ 0 ];
*(p1++) = v[ 1 ];
*(p2++) = v[ 2 ];
diff --git a/sun210.htx_tar b/sun210.htx_tar
index bf23c91..1fb8c5d 100644
Binary files a/sun210.htx_tar and b/sun210.htx_tar differ
diff --git a/sun210.ps b/sun210.ps
index 44c15ac..386fb89 100644
--- a/sun210.ps
+++ b/sun210.ps
@@ -1,19 +1,19 @@
%!PS-Adobe-2.0
-%%Creator: dvips(k) 5.98 Copyright 2009 Radical Eye Software
+%%Creator: dvips(k) 5.96.1 Copyright 2007 Radical Eye Software
%%Title: sun210.dvi
-%%CreationDate: Wed Jan 11 22:22:15 2012
+%%CreationDate: Tue Mar 13 09:57:22 2012
%%Pages: 615
%%PageOrder: Ascend
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+%%BoundingBox: 0 0 595 842
%%DocumentFonts: CMR10 CMCSC10 CMBX10 CMR12 CMBX12 CMSL10 CMTT10 CMTI10
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-%%+ CMTI9 CMTT9 CMMI12 CMBXTI10
+%%+ CMR8 CMSY10 CMR6 CMR9 CMTT9 CMSY8 CMMI10 CMMI9 CMSY9 CMMI7 CMMI8
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%%DocumentPaperSizes: a4
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%DVIPSWebPage: (www.radicaleye.com)
%DVIPSCommandLine: dvips -f sun210
%DVIPSParameters: dpi=600
-%DVIPSSource: TeX output 2012.01.11:2222
+%DVIPSSource: TeX output 2012.03.13:0957
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-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMBXTI10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
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+%!PS-AdobeFont-1.1: CMBXTI10 1.0
+%%CreationDate: 1991 Aug 18 17:46:30
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
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+/FontInfo 7 dict dup begin
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%%EndFont
%%BeginFont: CMMI12
-%!PS-AdobeFont-1.0: CMMI12 003.002
-%%Title: CMMI12
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMMI12.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMMI12 known{/CMMI12 findfont dup/UniqueID known{dup
-/UniqueID get 5087386 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMMI12 1.100
+%%CreationDate: 1996 Jul 27 08:57:55
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMMI12 def
-/FontBBox {-31 -250 1026 750 }readonly def
-/UniqueID 5087386 def
-/PaintType 0 def
-/FontInfo 10 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMMI12.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.100) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMMI12) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
-/ascent 750 def
end readonly def
+/FontName /CMMI12 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 60 /less put
dup 62 /greater put
readonly def
+/FontBBox{-30 -250 1026 750}readonly def
currentdict end
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@@ -614,46 +277,31 @@ A4CAE9E8E42F3F281F31B1A00D435069E6A1FCDE911D9F83331EECB3F32EEC66
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMBX10
-%!PS-AdobeFont-1.0: CMBX10 003.002
-%%Title: CMBX10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMBX10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMBX10 known{/CMBX10 findfont dup/UniqueID known{dup
-/UniqueID get 5000768 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMBX10 1.00B
+%%CreationDate: 1992 Feb 19 19:54:06
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMBX10 def
-/FontBBox {-56 -250 1164 750 }readonly def
-/UniqueID 5000768 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMBX10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.00B) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMBX10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Bold) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMBX10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
dup 12 /fi put
dup 34 /quotedblright put
+dup 38 /ampersand put
dup 40 /parenleft put
dup 41 /parenright put
dup 43 /plus put
@@ -730,689 +378,461 @@ dup 120 /x put
dup 121 /y put
dup 124 /emdash put
readonly def
+/FontBBox{-301 -250 1164 946}readonly def
currentdict end
currentfile eexec
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@@ -1422,41 +842,25 @@ E8C7E39722AC35627607E47625B0EB98FE4C0D7DBE5F4B32977370FE23071B4F
0000000000000000000000000000000000000000000000000000000000000000
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMR12
-%!PS-AdobeFont-1.0: CMR12 003.002
-%%Title: CMR12
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMR12.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMR12 known{/CMR12 findfont dup/UniqueID known{dup
-/UniqueID get 5000794 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMR12 1.0
+%%CreationDate: 1991 Aug 20 16:38:05
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMR12 def
-/FontBBox {-34 -251 988 750 }readonly def
-/UniqueID 5000794 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMR12.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMR12) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMR12 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -1477,7 +881,7 @@ dup 50 /two put
dup 51 /three put
dup 52 /four put
dup 53 /five put
-dup 54 /six put
+dup 55 /seven put
dup 57 /nine put
dup 63 /question put
dup 65 /A put
@@ -1530,612 +934,399 @@ dup 120 /x put
dup 121 /y put
dup 122 /z put
readonly def
+/FontBBox{-34 -251 988 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMTI9
-%!PS-AdobeFont-1.0: CMTI9 003.002
-%%Title: CMTI9
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMTI9.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMTI9 known{/CMTI9 findfont dup/UniqueID known{dup
-/UniqueID get 5000827 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMTI9 1.0
+%%CreationDate: 1991 Aug 18 21:08:07
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMTI9 def
-/FontBBox {-35 -250 1148 750 }readonly def
-/UniqueID 5000827 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMTI9.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMTI9) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMTI9 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 46 /period put
@@ -2521,229 +1432,72 @@ dup 105 /i put
dup 116 /t put
dup 118 /v put
readonly def
+/FontBBox{-35 -250 1148 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMMI8
-%!PS-AdobeFont-1.0: CMMI8 003.002
-%%Title: CMMI8
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMMI8.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMMI8 known{/CMMI8 findfont dup/UniqueID known{dup
-/UniqueID get 5087383 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMMI8 1.100
+%%CreationDate: 1996 Jul 23 07:53:54
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMMI8 def
-/FontBBox {-24 -250 1110 750 }readonly def
-/UniqueID 5087383 def
-/PaintType 0 def
-/FontInfo 10 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMMI8.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.100) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMMI8) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
-/ascent 750 def
end readonly def
+/FontName /CMMI8 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 58 /period put
@@ -2807,274 +1544,121 @@ dup 115 /s put
dup 116 /t put
dup 117 /u put
readonly def
+/FontBBox{-24 -250 1110 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMSY10
-%!PS-AdobeFont-1.0: CMSY10 003.002
-%%Title: CMSY10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMSY10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMSY10 known{/CMSY10 findfont dup/UniqueID known{dup
-/UniqueID get 5096651 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMSY10 1.0
+%%CreationDate: 1991 Aug 15 07:20:57
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMSY10 def
-/FontBBox {-29 -960 1116 775 }readonly def
-/UniqueID 5096651 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMSY10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMSY10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
-/ItalicAngle -14.04 def
+/ItalicAngle -14.035 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMSY10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 0 /minus put
@@ -3133,238 +1701,69 @@ dup 110 /backslash put
dup 112 /radical put
dup 120 /section put
readonly def
+/FontBBox{-29 -960 1116 775}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMR10
-%!PS-AdobeFont-1.0: CMR10 003.002
-%%Title: CMR10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMR10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMR10 known{/CMR10 findfont dup/UniqueID known{dup
-/UniqueID get 5000793 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMR10 1.00B
+%%CreationDate: 1992 Feb 19 19:54:52
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMR10 def
-/FontBBox {-40 -250 1009 750 }readonly def
-/UniqueID 5000793 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMR10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.00B) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMR10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMR10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -3505,805 +1888,549 @@ dup 122 /z put
dup 123 /endash put
dup 124 /emdash put
readonly def
+/FontBBox{-251 -250 1009 969}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMMI7
-%!PS-AdobeFont-1.0: CMMI7 003.002
-%%Title: CMMI7
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMMI7.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMMI7 known{/CMMI7 findfont dup/UniqueID known{dup
-/UniqueID get 5087382 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMMI7 1.100
+%%CreationDate: 1996 Jul 23 07:53:53
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMMI7 def
-/FontBBox {-1 -250 1171 750 }readonly def
-/UniqueID 5087382 def
-/PaintType 0 def
-/FontInfo 10 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMMI7.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.100) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMMI7) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
-/ascent 750 def
end readonly def
+/FontName /CMMI7 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 76 /L put
@@ -4366,274 +2476,119 @@ dup 115 /s put
dup 116 /t put
dup 117 /u put
readonly def
+/FontBBox{0 -250 1171 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMMI10
-%!PS-AdobeFont-1.0: CMMI10 003.002
-%%Title: CMMI10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMMI10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMMI10 known{/CMMI10 findfont dup/UniqueID known{dup
-/UniqueID get 5087385 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMMI10 1.100
+%%CreationDate: 1996 Jul 23 07:53:57
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMMI10 def
-/FontBBox {-32 -250 1048 750 }readonly def
-/UniqueID 5087385 def
-/PaintType 0 def
-/FontInfo 10 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMMI10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.100) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMMI10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
-/ascent 750 def
end readonly def
+/FontName /CMMI10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 22 /mu put
@@ -4714,389 +2652,231 @@ dup 120 /x put
dup 121 /y put
dup 122 /z put
readonly def
+/FontBBox{-32 -250 1048 750}readonly def
currentdict end
currentfile eexec
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%%EndFont
%%BeginFont: CMSY9
-%!PS-AdobeFont-1.0: CMSY9 003.002
-%%Title: CMSY9
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMSY9.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMSY9 known{/CMSY9 findfont dup/UniqueID known{dup
-/UniqueID get 5096650 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMSY9 1.0
+%%CreationDate: 1991 Aug 15 07:22:27
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMSY9 def
-/FontBBox {-29 -958 1146 777 }readonly def
-/UniqueID 5096650 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMSY9.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMSY9) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
-/ItalicAngle -14.04 def
+/ItalicAngle -14.035 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMSY9 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 0 /minus put
dup 3 /asteriskmath put
readonly def
+/FontBBox{-30 -958 1146 777}readonly def
currentdict end
currentfile eexec
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-{restore}if
%%EndFont
%%BeginFont: CMMI9
-%!PS-AdobeFont-1.0: CMMI9 003.002
-%%Title: CMMI9
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMMI9.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMMI9 known{/CMMI9 findfont dup/UniqueID known{dup
-/UniqueID get 5087384 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMMI9 1.100
+%%CreationDate: 1996 Jul 23 07:53:55
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMMI9 def
-/FontBBox {-29 -250 1075 750 }readonly def
-/UniqueID 5087384 def
-/PaintType 0 def
-/FontInfo 10 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMMI9.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.100) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMMI9) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
-/ascent 750 def
end readonly def
+/FontName /CMMI9 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 58 /period put
readonly def
+/FontBBox{-29 -250 1075 750}readonly def
currentdict end
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMSY8
-%!PS-AdobeFont-1.0: CMSY8 003.002
-%%Title: CMSY8
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMSY8.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMSY8 known{/CMSY8 findfont dup/UniqueID known{dup
-/UniqueID get 5096649 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMSY8 1.0
+%%CreationDate: 1991 Aug 15 07:22:10
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMSY8 def
-/FontBBox {-30 -955 1185 779 }readonly def
-/UniqueID 5096649 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMSY8.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMSY8) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
-/ItalicAngle -14.04 def
+/ItalicAngle -14.035 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMSY8 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 0 /minus put
dup 14 /openbullet put
readonly def
+/FontBBox{-30 -955 1185 779}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
-%%BeginFont: CMR9
-%!PS-AdobeFont-1.0: CMR9 003.002
-%%Title: CMR9
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMR9.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMR9 known{/CMR9 findfont dup/UniqueID known{dup
-/UniqueID get 5000792 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%%BeginFont: CMTT9
+%!PS-AdobeFont-1.1: CMTT9 1.0
+%%CreationDate: 1991 Aug 20 16:46:24
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMR9 def
-/FontBBox {-39 -250 1036 750 }readonly def
-/UniqueID 5000792 def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
+/FullName (CMTT9) readonly def
+/FamilyName (Computer Modern) readonly def
+/Weight (Medium) readonly def
+/ItalicAngle 0 def
+/isFixedPitch true def
+end readonly def
+/FontName /CMTT9 def
/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMR9.) readonly def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
+/Encoding 256 array
+0 1 255 {1 index exch /.notdef put} for
+dup 45 /hyphen put
+dup 95 /underscore put
+dup 97 /a put
+dup 101 /e put
+dup 104 /h put
+dup 105 /i put
+dup 108 /l put
+dup 110 /n put
+dup 112 /p put
+dup 114 /r put
+dup 116 /t put
+dup 119 /w put
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+readonly def
+/FontBBox{-6 -233 542 698}readonly def
+currentdict end
+currentfile eexec
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+cleartomark
+%%EndFont
+%%BeginFont: CMR9
+%!PS-AdobeFont-1.1: CMR9 1.0
+%%CreationDate: 1991 Aug 20 16:39:59
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
+11 dict begin
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMR9) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMR9 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -5882,7 +3237,6 @@ dup 49 /one put
dup 50 /two put
dup 51 /three put
dup 53 /five put
-dup 54 /six put
dup 55 /seven put
dup 56 /eight put
dup 58 /colon put
@@ -5938,632 +3292,387 @@ dup 120 /x put
dup 121 /y put
dup 122 /z put
readonly def
+/FontBBox{-39 -250 1036 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMR6
-%!PS-AdobeFont-1.0: CMR6 003.002
-%%Title: CMR6
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMR6.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMR6 known{/CMR6 findfont dup/UniqueID known{dup
-/UniqueID get 5000789 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMR6 1.0
+%%CreationDate: 1991 Aug 20 16:39:02
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMR6 def
-/FontBBox {-20 -250 1193 750 }readonly def
-/UniqueID 5000789 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMR6.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMR6) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMR6 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 48 /zero put
@@ -6621,243 +3714,91 @@ dup 55 /seven put
dup 56 /eight put
dup 57 /nine put
readonly def
+/FontBBox{-20 -250 1193 750}readonly def
currentdict end
currentfile eexec
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%%EndFont
%%BeginFont: CMTT10
-%!PS-AdobeFont-1.0: CMTT10 003.002
-%%Title: CMTT10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMTT10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
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-/UniqueID get 5000832 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMTT10 1.00B
+%%CreationDate: 1992 Apr 26 10:42:42
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMTT10 def
-/FontBBox {-4 -233 537 696 }readonly def
-/UniqueID 5000832 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMTT10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.00B) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMTT10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch true def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMTT10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 33 /exclam put
@@ -6995,651 +3920,466 @@ dup 122 /z put
dup 123 /braceleft put
dup 125 /braceright put
readonly def
+/FontBBox{-4 -235 731 800}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMR8
-%!PS-AdobeFont-1.0: CMR8 003.002
-%%Title: CMR8
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMR8.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMR8 known{/CMR8 findfont dup/UniqueID known{dup
-/UniqueID get 5000791 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMR8 1.0
+%%CreationDate: 1991 Aug 20 16:39:40
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMR8 def
-/FontBBox {-36 -250 1070 750 }readonly def
-/UniqueID 5000791 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMR8.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMR8) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMR8 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 48 /zero put
@@ -7697,243 +4421,91 @@ dup 55 /seven put
dup 56 /eight put
dup 57 /nine put
readonly def
+/FontBBox{-36 -250 1070 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMBX12
-%!PS-AdobeFont-1.0: CMBX12 003.002
-%%Title: CMBX12
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMBX12.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMBX12 known{/CMBX12 findfont dup/UniqueID known{dup
-/UniqueID get 5000769 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMBX12 1.0
+%%CreationDate: 1991 Aug 20 16:34:54
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMBX12 def
-/FontBBox {-53 -251 1139 750 }readonly def
-/UniqueID 5000769 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMBX12.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMBX12) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Bold) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMBX12 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -8055,598 +4611,386 @@ dup 121 /y put
dup 122 /z put
dup 124 /emdash put
readonly def
+/FontBBox{-53 -251 1139 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMTI10
-%!PS-AdobeFont-1.0: CMTI10 003.002
-%%Title: CMTI10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMTI10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMTI10 known{/CMTI10 findfont dup/UniqueID known{dup
-/UniqueID get 5000828 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMTI10 1.00B
+%%CreationDate: 1992 Feb 19 19:56:16
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMTI10 def
-/FontBBox {-35 -250 1124 750 }readonly def
-/UniqueID 5000828 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMTI10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.00B) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMTI10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMTI10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -8740,520 +5068,335 @@ dup 119 /w put
dup 120 /x put
dup 121 /y put
readonly def
+/FontBBox{-163 -250 1146 969}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMSL10
-%!PS-AdobeFont-1.0: CMSL10 003.002
-%%Title: CMSL10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMSL10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMSL10 known{/CMSL10 findfont dup/UniqueID known{dup
-/UniqueID get 5000798 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMSL10 1.0
+%%CreationDate: 1991 Aug 20 16:40:20
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMSL10 def
-/FontBBox {-62 -250 1123 750 }readonly def
-/UniqueID 5000798 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMSL10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMSL10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -9.46 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMSL10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -9368,631 +5495,421 @@ dup 120 /x put
dup 121 /y put
dup 124 /emdash put
readonly def
+/FontBBox{-62 -250 1123 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMCSC10
-%!PS-AdobeFont-1.0: CMCSC10 003.002
-%%Title: CMCSC10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMCSC10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMCSC10 known{/CMCSC10 findfont dup/UniqueID known{dup
-/UniqueID get 5087402 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMCSC10 1.0
+%%CreationDate: 1991 Aug 18 17:46:49
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMCSC10 def
-/FontBBox {14 -250 1077 750 }readonly def
-/UniqueID 5087402 def
-/PaintType 0 def
-/FontInfo 10 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMCSC10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMCSC10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
-/ascent 750 def
end readonly def
+/FontName /CMCSC10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 65 /A put
@@ -10058,296 +5958,122 @@ dup 116 /t put
dup 117 /u put
dup 121 /y put
readonly def
+/FontBBox{14 -250 1077 750}readonly def
currentdict end
currentfile eexec
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-(precision)h(of)g(\\)p Fo(:)p Fn(\003)p Fr(",)h(then)d(Digits)i(will)g
+(precision)h(of)g(\\)p Fn(:)p Fm(\003)p Fr(",)h(then)d(Digits)i(will)g
(b)r(e)f(used)f(to)0 5602 y(determine)i(the)f(actual)h(precision)h
(used.)73 5661 y Fs(12)138 5693 y Fr(This)g(is)f(a)g(consequence)f(of)i
(implemen)n(ting)f(the)f(AST)g(library)h(in)g(C.)p eop
@@ -90812,10 +86533,10 @@ b(this)g(case,)j(the)d(axes)h(of)g(a)f(2-dimensional)h(F)-8
b(rame)23 b(could)e(b)s(e)g(in)m(terc)m(hanged)h(b)m(y)f(passing)g
(this)g(p)s(erm)m(utation)0 2640 y(arra)m(y)45 b(to)f(the)h(AST)p
Fy(_)p FG(PERMAXES)e(function.)81 b(That)44 b(is,)k(an)c(\()p
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+Fo(x)2380 2654 y Fv(1)2420 2640 y Fo(;)15 b(x)2512 2654
y Fv(2)2552 2640 y FG(\))44 b(co)s(ordinate)h(system)f(w)m(ould)g(b)s
-(e)0 2753 y(c)m(hanged)31 b(in)m(to)g(an)g(\()p Fp(x)749
-2767 y Fv(2)788 2753 y Fp(;)15 b(x)880 2767 y Fv(1)920
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+2767 y Fv(2)788 2753 y Fo(;)15 b(x)880 2767 y Fv(1)920
2753 y FG(\))31 b(co)s(ordinate)g(system)g(b)m(y:)262
2992 y Ft(CALL)41 b(AST_PERMAXES\()e(FRAME,)i(PERM,)g(STATUS)g(\))0
3244 y FG(If)36 b(the)h(axes)g(are)g(p)s(erm)m(uted)e(more)i(than)f
@@ -91039,7 +86760,7 @@ b(with)g(a)h(2-dimensional)h(F)-8 b(rame)33 b(the)g(returned)f(angle)h
(taking)h(the)f(\\shortest)h(route")f(from)g(the)g(\014rst)f(p)s(oin)m
(t)h(to)h(the)f(second.)0 1866 y(If)29 b(the)h(F)-8 b(rame)31
b(has)e(more)h(than)f(2)h(axes,)h(the)f(result)f(is)h(un-signed)f(and)g
-(is)h(alw)m(a)m(ys)h(in)e(the)h(range)g(zero)h(to)f Fp(\031)s
+(is)h(alw)m(a)m(ys)h(in)e(the)h(range)g(zero)h(to)f Fo(\031)s
FG(.)0 2026 y(The)22 b(AST)p Fy(_)p FG(AXANGLE)h(routine)g(is)f
(similar)h(to)h(AST)p Fy(_)p FG(AXANGLE,)f(but)f(the)h(\\reference)g
(direction",)j(from)0 2138 y(whic)m(h)k(angles)h(are)g(measured,)f(is)h
@@ -91070,7 +86791,7 @@ h(for)f(the)g(Domain)i(attribute,)g(consider)e(using)g(di\013eren)m(t)h
(di\013eren)m(t)g(co)s(ordinate)g(systems)g(asso)s(ciated)h(with)e(a)g
(CCD)h(image:)111 4165 y(1.)46 b(A)31 b(co)s(ordinate)g(system)f(based)
h(on)f(pixel)g(n)m(um)m(b)s(ers.)111 4350 y(2.)46 b(P)m(ositions)32
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+b(on)e(the)h(CCD)f(c)m(hip,)g(measured)g(in)g Fo(\026)p
FG(m.)111 4534 y(3.)46 b(P)m(ositions)32 b(in)e(the)h(fo)s(cal)g(plane)
f(of)h(the)f(telescop)s(e,)i(measured)e(in)g(mm.)111
4719 y(4.)46 b(A)31 b(celestial)i(co)s(ordinate)e(system,)g(measured)e
@@ -91089,7 +86810,7 @@ h(di\013eren)m(t)e(results.)39 b(F)-8 b(or)28 b(example,)h(w)m(e)f
(legitimate,)k(ho)m(w)m(ev)m(er,)e(to)g(directly)f(compare)g(p)s
(ositions)g(in)f(one)h(image)h(mea-)0 5693 y(sured)e(in)g(pixels)h
(with)g(p)s(ositions)f(in)h(the)g(other)g(measured)f(in)h(mm,)f(nor)h
-(to)g(equate)h(c)m(hip)f(p)s(ositions)g(in)f Fp(\026)p
+(to)g(equate)h(c)m(hip)f(p)s(ositions)g(in)f Fo(\026)p
FG(m)p eop end
%%Page: 72 82
TeXDict begin 72 81 bop 0 52 a FG(72)1200 b Fz(7)92 b(REPRESENTING)29
@@ -91206,9 +86927,9 @@ y FG(When)31 b(c)m(ho)s(osing)g(a)h(v)-5 b(alue)31 b(for)g(the)g
m(an)m(t)i(to)0 1808 y(iden)m(tify)25 b(an)f(instrumen)m(tal)h(co)s
(ordinate)g(system,)h(then)e(it)h(is)g(sensible)f(to)h(add)f(a)h
(distinguishing)f(pre\014x.)38 b(F)-8 b(or)0 1920 y(instance,)25
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-Fp(>)f FG(\()p Fx(e.g.)g FG(an)h(acron)m(ym\))h(iden)m(ti\014es)0
+b(y)m(ou)f(migh)m(t)f(use)g Fo(<)p FG(INST)p Fo(>)p Fy(_)p
+FG(F)m(OCAL)p Fy(_)p FG(PLANE,)e(where)i Fo(<)p FG(INST)p
+Fo(>)f FG(\()p Fx(e.g.)g FG(an)h(acron)m(ym\))h(iden)m(ti\014es)0
2033 y(y)m(our)30 b(instrumen)m(t.)0 2193 y(F)-8 b(or)37
b(some)g(purp)s(oses,)g(ho)m(w)m(ev)m(er,)j(a)d(standard)e(c)m(hoice)k
(of)e(Domain)g(name)g(is)f(desirable)h(so)g(that)g(di\013eren)m(t)0
@@ -91388,9 +87109,9 @@ b(CVT)262 3110 y(...)262 3209 y(CVT)i(=)h(AST_CONVERT\()c(FRAME1,)h
(tained)g(within)f(the)g(F)-8 b(rameSet)22 b(returned)d(b)m(y)h(AST)p
Fy(_)p FG(CONVER)-8 b(T)19 b(will)i(b)s(e)e(a)i(one-dimensional)0
3594 y(Zo)s(omMap)33 b(whic)m(h)g(simply)f(scales)j(its)e(input)f(\(a)i
-(v)m(elo)s(cit)m(y)i(in)d Fp(k)s(m=h)p FG(\))h(b)m(y)f(a)g(factor)h(of)
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g(0.278)h(to)e(create)i(its)0 3706 y(output)30 b(\(a)h(v)m(elo)s(cit)m
-(y)i(in)d Fp(m=s)p FG(\).)0 3872 y(In)43 b(fact)i(w)m(e)g(need)f(not)g
+(y)i(in)d Fo(m=s)p FG(\).)0 3872 y(In)43 b(fact)i(w)m(e)g(need)f(not)g
(ha)m(v)m(e)h(set)g(the)f(Unit)g(attribute)h(activ)m(e)h(in)e(FRAME1)h
(since)f(the)h(b)s(eha)m(viour)e(of)0 3985 y(AST)p Fy(_)p
FG(CONVER)-8 b(T)29 b(is)h(determined)g(b)m(y)h(its)f(TO)g(F)-8
@@ -91616,33 +87337,33 @@ b(for)d(m)m(ultiples)i(&)f(sub-m)m(ultiples)p 3161 984
V 617 987 2546 4 v 615 1100 4 113 v 667 1066 a FG(Sub-m)m(ultiple)99
b(Name)i(Pre\014x)p 1888 1100 V 1888 1100 V 99 w(Sub-m)m(ultiple)e
(Name)h(Pre\014x)p 3161 1100 V 617 1103 2546 4 v 615
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1183 y FG(deci)174 b(d)p 1888 1216 V 285 w(10)517 b(deca)153
b(da)p 3161 1216 V 615 1329 V 667 1295 a(10)757 1262
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1329 V 296 w(10)2030 1262 y Fv(2)2547 1295 y FG(hecto)118
b(h)p 3161 1329 V 615 1442 V 667 1408 a(10)757 1375 y
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V 260 w(10)2030 1375 y Fv(3)2547 1408 y FG(kilo)186 b(k)p
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Fv(6)1274 1521 y FG(micro)108 b(u)p 1888 1555 V 285 w(10)2030
1488 y Fv(6)2547 1521 y FG(mega)123 b(M)p 3161 1555 V
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1634 y FG(nano)138 b(n)p 1888 1668 V 285 w(10)2030 1601
y Fv(9)2547 1634 y FG(giga)169 b(G)p 3161 1668 V 615
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1747 y FG(pico)g(p)p 1888 1781 V 285 w(10)2030 1714 y
Fv(12)2547 1747 y FG(tera)k(T)p 3161 1781 V 615 1894
-V 667 1860 a(10)757 1827 y Fq(\000)p Fv(15)1274 1860
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y FG(fem)m(to)109 b(f)p 1888 1894 V 308 w(10)2030 1827
y Fv(15)2547 1860 y FG(p)s(eta)155 b(P)p 3161 1894 V
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1973 y FG(atto)170 b(a)p 1888 2007 V 291 w(10)2030 1940
y Fv(18)2547 1973 y FG(exa)196 b(E)p 3161 2007 V 615
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2086 y FG(zepto)119 b(z)p 1888 2120 V 296 w(10)2030 2053
y Fv(21)2547 2086 y FG(zetta)134 b(Z)p 3161 2120 V 615
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2199 y FG(y)m(o)s(cto)117 b(y)p 1888 2233 V 288 w(10)2030
2166 y Fv(24)2547 2199 y FG(y)m(otta)124 b(Y)p 3161 2233
V 617 2236 2546 4 v 590 3621 2601 4 v 588 3734 4 113
@@ -91657,10 +87378,10 @@ V 101 w(m)m(ultiplication)h(\(an)f(asterisk\))p 3188
121 w(m)m(ultiplication)h(\(a)f(dot\))p 3188 4192 V 588
4305 V 639 4271 a(sym1/sym2)p 1143 4305 V 101 w(division)p
3188 4305 V 588 4418 V 639 4384 a(sym1**y)p 1143 4418
-V 213 w(exp)s(onen)m(tiation)g(\()p Fp(y)j FG(m)m(ust)c(b)s(e)g(a)g(n)m
+V 213 w(exp)s(onen)m(tiation)g(\()p Fo(y)j FG(m)m(ust)c(b)s(e)g(a)g(n)m
(umerical)h(constan)m(t\))p 3188 4418 V 588 4531 V 639
4497 a(sym1)p Fy(^)p FG(y)p 1143 4531 V 255 w(exp)s(onen)m(tiation)g
-(\()p Fp(y)j FG(m)m(ust)c(b)s(e)g(a)g(n)m(umerical)h(constan)m(t\))p
+(\()p Fo(y)j FG(m)m(ust)c(b)s(e)g(a)g(n)m(umerical)h(constan)m(t\))p
3188 4531 V 588 4644 V 639 4610 a(log\(sym1\))p 1143
4644 V 166 w(common)f(logarithm)p 3188 4644 V 588 4756
V 639 4723 a(ln\(sym1\))p 1143 4756 V 205 w(natural)g(logarithm)p
@@ -92516,7 +88237,7 @@ b(alue)26 b(of)f(\\V)-8 b(opt",)28 b(but)d(if)g(a)g(di\013eren)m(t)h
(System)f(v)-5 b(alue)0 5197 y(w)m(ere)32 b(set,)g(the)g(defaults)f(w)m
(ould)g(b)s(e)g(corresp)s(ondingly)f(di\013eren)m(t.)44
b(F)-8 b(or)32 b(example,)h(b)m(y)e(default)h(frequency)e(is)0
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FG(,)h(so)f(setting)g(\\System=freq")g(w)m(ould)g(c)m(hange)h(the)e
(appropriate)0 5423 y(line)e(ab)s(o)m(v)m(e)g(from:)227
5693 y Fy(#)143 b(Uni1)47 b(=)g("km/s")333 b(#)47 b(Units)g(for)f(axis)
@@ -92633,22 +88354,22 @@ b(\(a)i(Sp)s(ecCub)s(eF)-8 b(rame\))30 b(will)h(b)s(e)f(added)g(to)i
1524 y(v)-5 b(ariation)32 b(in)e(Doppler)g(shift.)0 1680
y(The)40 b(maxim)m(um)g(v)m(elo)s(cit)m(y)j(error)d(in)m(tro)s(duced)f
(b)m(y)i(this)f(problem)f(is)i(of)f(the)h(order)f(of)g
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b FG(is)33 b(the)g(relativ)m(e)i(v)m(elo)s(cit)m(y)h(of)d(the)h(t)m(w)m
(o)g(standards)e(of)0 1906 y(rest.)56 b(As)35 b(an)g(example,)i(when)e
(correcting)h(from)f(the)h(observ)m(ers)f(rest)h(frame)f(\(i.e.)56
b(the)36 b(top)s(o)s(cen)m(tric)g(rest)0 2019 y(frame\))f(to)h(the)f
(kinematic)h(lo)s(cal)h(standard)d(of)h(rest)g(the)g(maxim)m(um)g(v)-5
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h(view)f(the)h(maxim)m(um)f(v)m(elo)s(cit)m(y)j(error)d(in)m(tro)s
(duced)g(b)m(y)g(the)h(correction)g(will)g(b)s(e)0 2245
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(the)f(maxim)m(um)f(error)g(when)g(correcting)i(from)e(the)h(observ)m
(ers)0 2357 y(rest)h(frame)f(to)h(the)g(lo)s(cal)g(group)f(is)g(ab)s
-(out)g(5)h Fp(k)s(m=s)g FG(o)m(v)m(er)g(a)g(1)g(degree)g(\014eld)f(of)g
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(view.)0 2641 y Fw(9.7)112 b(Handling)39 b(Dual-Sideband)h(Sp)s(ectra)0
2856 y FG(Dual)32 b(sideband)d(sup)s(er-hetero)s(dyne)h(receiv)m(ers)i
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@@ -92658,10 +88379,10 @@ y(ab)s(out)c(0.03)j Fp(k)s(m=s)p FG(.)40 b(As)30 b(another)g(example,)h
(frequency".)40 b(In)26 b(the)i(rest)f(frame)h(of)f(the)h(observ)m(er)f
(\(top)s(o)s(cen)m(tric\),)j(these)e(are)g(related)g(to)0
3195 y(eac)m(h)k(other)e(as)h(follo)m(ws:)1544 3518 y
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+3530 y Fk(LO)2007 3518 y Fi(\000)18 b Fl(f)2131 3530
+y Fk(usb)3446 3518 y Fj(\(1\))0 3754 y FG(where)34 b
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m(wn)f(as)h(the)f(\\lo)s(cal)j(oscillator)g(frequency".)53
b(In)34 b(other)h(w)m(ords,)g(the)0 3867 y(lo)s(cal)30
b(oscillator)g(frequency)e(is)g(alw)m(a)m(ys)i(mid-w)m(a)m(y)f(b)s(et)m
@@ -92671,8 +88392,8 @@ y Fv(15)897 3980 y FG(.)63 b(If)38 b(y)m(ou)g(w)m(an)m(t)h(to)f
(describ)s(e)g(the)g(sp)s(ectral)g(axis)h(of)f(suc)m(h)f(a)i(sp)s
(ectrum)e(using)g(a)0 4093 y(Sp)s(ecF)-8 b(rame)31 b(y)m(ou)h(m)m(ust)f
(c)m(ho)s(ose)h(whether)f(y)m(ou)g(w)m(an)m(t)h(the)g(Sp)s(ecF)-8
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4206 y(Sp)s(ecF)-8 b(rame)42 b(cannot)g(describ)s(e)f(b)s(oth)f
(sidebands)g(sim)m(ultaneously)-8 b(.)76 b(Ho)m(w)m(ev)m(er,)46
b(there)c(is)f(a)h(sub-class)f(of)0 4319 y(Sp)s(ecF)-8
@@ -92746,15 +88467,15 @@ b(The)20 b(in)m(termediate)i(frequency)d(is)i(the)f(di\013erence)h(b)s
(et)m(w)m(een)g(the)f(top)s(o)s(cen)m(tric)i(frequency)0
2732 y(at)31 b(the)g(cen)m(tral)g(sp)s(ectral)g(p)s(osition)g(and)e
(the)i(top)s(o)s(cen)m(tric)g(frequency)f(of)h(the)f(lo)s(cal)i
-(oscillator.)43 b(So:)1528 3081 y Fm(f)1569 3093 y Fl(LO)1693
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%%Page: 201 211
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%%Page: 202 212
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(fail)h(for)f(an)n(y)g(reason.)p 0 3411 3780 12 v 0 3542
@@ -116687,7 +112408,7 @@ a FA(AST)p Fe(_)p FA(COLUMNNAME)1538 3543 y Fd(Get)39
b(the)f(name)1537 3642 y(of)g(the)h(column)1636 3742
y(at)f(a)h(giv)m(en)1569 3857 y(index)g(within)1648 3956
y(the)f(T)-10 b(able)2411 3542 y FA(AST)p Fe(_)p FA(COLUMNNAME)0
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4331 y(This)29 b(function)h(is)f(in)n(tended)g(primarily)f(as)g(a)h
@@ -116706,21 +112427,21 @@ b(Column)g(in)h(the)f(T)-7 b(able)25 b(will)g(ha)n(v)n(e)f(index)h
4994 y Fc(In)m(v)m(o)s(cation:)123 b Ft(RESULT)41 b(=)i
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5137 y Fc(Argumen)m(ts:)259 5267 y(THIS)32 b(=)g(INTEGER)g(\(Giv)m
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b(The)31 b(\014rst)g(column)h(has)e(index)i(one,)g(and)f(the)h(last)f
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eop end
%%Page: 206 216
TeXDict begin 206 215 bop 0 52 a FG(206)2115 b Fz(B)92
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1671 y FA(AST)p Fe(_)p FA(COLUMNNULL)0 2134 y Fc(Description:)44
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b(The)37 b(supplied)g(n)n(ull)g(v)-5 b(alue)37 b(is)g(assigned)f(to)h
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b(an)n(y)h(v)-5 b(alue)26 b(set)h(b)n(y)f(a)g(previous)f(call)h(to)g
@@ -116783,7 +112504,7 @@ b(an)n(y)h(v)-5 b(alue)26 b(set)h(b)n(y)f(a)g(previous)f(call)h(to)g
b(alue)26 b(supplied)h(for)427 4847 y(argumen)n(t)g(NEWV)-9
b(AL)28 b(is)f(ignored)g(and)g(the)h(curren)n(t)f(n)n(ull)h(v)-5
b(alue)27 b(is)h(left)g(unc)n(hanged.)259 4971 y Fc(NEWV)-11
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b(if)i(SET)f(is)g(.F)-9 b(ALSE.)22 b(An)g(error)e(will)i(b)r(e)h(rep)r
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@@ -116791,7 +112512,7 @@ b(is)g(outside)g(the)h(range)d(of)i(v)-5 b(alues)34 b(that)h(can)e(b)r
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b(.F)-9 b(ALSE.)30 b(is)g(returned)g(otherwise.)44 b(If)31
@@ -116801,7 +112522,7 @@ b(ALSE.)27 b(is)h(returned.)p eop end
%%Page: 207 217
TeXDict begin 207 216 bop 3643 52 a FG(207)259 351 y
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b(alue)34 b(on)g(exit)g(\(i.e.)58 b(NEWV)-9 b(AL)35 b(if)f(SET)g(is)h
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y(previous)f(in)n(v)n(o)r(cation)g(of)i(this)f(function,)i(it)f(will)f
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f(system)i(to)f(the)h(one)f(y)n(ou)g(requested.)p eop
end
%%Page: 226 236
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b(rames.)64 b(F)-7 b(rame)36 b(n)n(um)n(b)r(er)g(1)h(\(its)g(base)f(F)
@@ -118381,17 +114102,17 @@ b(ran2\),)27 b(then)i(it)g(pro)n(vides)e(a)h(means)g(of)g(con)n(v)n
end
%%Page: 227 237
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@@ -118958,7 +114679,7 @@ TeXDict begin 233 242 bop 3643 52 a FG(233)p 0 351 3780
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%%Page: 234 244
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@@ -119301,54 +115022,54 @@ b(T)g(A)1759 3984 y Fd(Retriev)m(e)1828 4084 y(all)1808
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eop end
%%Page: 238 248
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%%Page: 239 249
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%%Page: 243 253
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%%Page: 245 255
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@@ -119826,18 +115547,18 @@ FA(GETREGIONPOINTS)p eop end
%%Page: 246 256
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%%Page: 247 257
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(an)n(y)227 3890 y(leading)h(or)g(trailing)g(spaces.)36
b(It)28 b(requires)e(the)i(follo)n(wing)e(in)n(terface:)227
4009 y(INTEGER)h(FUNCTION)i(TXEXT\()e(GRF)n(CON,)h(TEXT,)g(X,)g(Y,)g
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(of)h(the)427 5637 y(b)r(ounding)28 b(b)r(o)n(x.)p eop
end
@@ -120570,7 +116291,7 @@ b(AST)29 b(R)m(OUTINE)i(DESCRIPTIONS)p 0 351 3780 12
v 0 482 a FA(AST)p Fe(_)p FA(GRID)913 483 y Fd(Dra)m(w)38
b(a)g(set)h(of)f(lab)s(elled)g(co)s(ordinate)e(axes)3089
482 y FA(AST)p Fe(_)p FA(GRID)0 651 y Fc(Description:)44
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751 y(a)31 b(co)r(ordinate)f(grid)g(sup)r(erimp)r(osed.)47
b(Details)31 b(of)g(the)g(axes)f(and)h(grid)f(can)h(b)r(e)g(con)n
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y Fc(ST)-8 b(A)g(TUS)34 b(=)e(INTEGER)f(\(Giv)m(en)h(and)g(Returned\))
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(graphics)f(v)n(olume)h(sp)r(eci\014ed)g(when)h(the)g(Plot3D)e(w)n(as)g
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b(error)e(results)h(if)i(either)e(the)h(curren)n(t)f(F)-7
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2778 y(not)k(de\014ned)g(in)g(either)g(direction)g(\(i.e.)37
@@ -120604,7 +116325,7 @@ b(ranIn)n(v)n(erse)25 b(attribute)i(is)f(zero\).)p 0
2966 V 0 3096 a FA(AST)p Fe(_)p FA(GRIDLINE)1237 3104
y Fd(Dra)m(w)37 b(a)i(grid)f(line)g(\(or)f(axis\))1643
3225 y(for)h(a)h(Plot)2765 3096 y FA(AST)p Fe(_)p FA(GRIDLINE)0
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227 3578 y(co)r(ordinate)38 b(grids,)j(and)d(tic)n(k)h(marks)e(on)i
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b(curv)n(e)e(is)i(transformed)e(in)n(to)h(graphical)f(co)r(ordinate)h
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3899 y(ph)n(ysical)24 b(co)r(ordinates)f(ma)n(y)g(result)h(in)h(a)f
@@ -120621,66 +116342,66 @@ b(curv)n(e)e(is)i(transformed)e(in)n(to)h(graphical)f(co)r(ordinate)h
f(in)h(the)f(Mapping)h(b)r(et)n(w)n(een)f(ph)n(ysical)g(and)g
(graphical)f(co)r(ordinates)g(are)g(catered)h(for,)g(as)227
4098 y(is)i(an)n(y)f(clipping)g(established)g(using)h(AST)p
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b Ft(CALL)42 b(AST_GRIDLINE\()c(THIS,)j(AXIS,)h(START,)f(LENGTH,)g
(STATUS)g(\))0 4385 y Fc(Argumen)m(ts:)259 4515 y(THIS)32
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%%Page: 265 275
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@@ -121779,112 +117500,112 @@ b(alue)29 b(is)g(an)g(AST)g(Ob)5 b(ject)29 b(p)r(oin)n(ter,)g(the)h(Ob)
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end
%%Page: 272 282
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eop end
%%Page: 273 283
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@@ -122379,7 +118100,7 @@ TeXDict begin 281 290 bop 3643 52 a FG(281)p 0 351 3780
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@@ -122494,7 +118215,7 @@ TeXDict begin 283 292 bop 3643 52 a FG(283)p 0 351 3780
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@@ -123257,8 +118978,8 @@ b(in)n(teger)f(v)-5 b(alue)32 b(of)g(X2)g(is)g(tak)n(en)f(\(rounding)g
eop end
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3893 y(to)n(w)n(ards)20 b(the)i(second)f(p)r(oin)n(t.)35
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%%Page: 300 310
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eop end
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%%Page: 333 343
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b(\015ag)f(\(see)h(b)r(elo)n(w\).)p eop end
%%Page: 336 346
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end
%%Page: 338 348
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@@ -127163,15 +122884,15 @@ TeXDict begin 339 348 bop 3643 52 a FG(339)0 351 y Fc(In)m(v)m(o)s
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%%Page: 354 364
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y FA(AST)p Fe(_)p FA(SETFITSU)0 2436 y Fc(Description:)44
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b(The)31 b(new)h(unde\014ned)g(v)-5 b(alue)31 b(can)g(either)h(o)n(v)n
@@ -128795,17 +124516,17 @@ b(The)31 b(new)h(unde\014ned)g(v)-5 b(alue)31 b(can)g(either)h(o)n(v)n
(in)n(to)g(the)h(FitsChan.)0 2780 y Fc(In)m(v)m(o)s(cation:)123
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-b(=)g(INTEGER)g(\(Giv)m(en\))427 3157 y Fk(P)n(oin)n(ter)26
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b(to)i(the)g(FitsChan.)259 3286 y Fc(NAME)j(=)h(CHARA)m(CTER)g
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-3386 y Fk(A)25 b(c)n(haracter)d(string)i(con)n(taining)g(the)g(FITS)h
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(FITS)f(header)427 3485 y(card,)k(in)g(whic)n(h)g(case)f(the)h(k)n(eyw)
n(ord)e(to)i(use)g(is)g(extracted)f(from)g(it.)39 b(No)28
b(more)f(than)h(80)f(c)n(haracters)f(are)427 3585 y(read)h(from)g(this)
h(string.)259 3713 y Fc(COMMENT)j(=)h(CHARA)m(CTER)f
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-3813 y Fk(A)i(string)e(holding)h(a)f(commen)n(t)h(to)g(asso)r(ciated)f
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@@ -128814,25 +124535,25 @@ f(an)n(y)f(existing)h(commen)n(t)g(in)h(the)f(card)f(b)r(eing)i(o)n(v)n
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b(no)i(commen)n(t)f(is)h(stored)e(with)j(the)f(card.)259
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%%Page: 358 368
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697 y(celestial)f(co)s(ordinate)1715 797 y(system)2651
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b(al-)227 1091 y(ues)19 b(\(in)h(radians\))e(supplied)i(within)g(the)f
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(supplied)g(SkyF)-7 b(rame.)0 1242 y Fc(In)m(v)m(o)s(cation:)123
b Ft(CALL)42 b(AST_SETREFPOS\()37 b(THIS,)42 b(FRM,)g(LON,)g(LAT,)g
(STATUS)f(\))0 1392 y Fc(Argumen)m(ts:)259 1530 y(THIS)32
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b(to)i(the)g(Sp)r(ecF)-7 b(rame.)259 1763 y Fc(FRM)31
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3161 V 0 3291 a FA(AST)p Fe(_)p FA(SETUNC)1061 3292 y
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3406 y(a)j(Region)2886 3291 y FA(AST)p Fe(_)p FA(SETUNC)0
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@@ -128905,68 +124626,68 @@ b(or)27 b(b)r(e)g(a)g(Prism)g(con)n(taining)g(cen)n(tro-symetric)427
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b(A)g(TUS)34 b(=)e(INTEGER)f(\(Giv)m(en)h(and)g(Returned\))427
-5626 y Fk(The)c(global)e(status.)p eop end
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%%Page: 359 369
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1615 y(p)r(erformed)18 b(b)n(y)g(carrying)f(out)h(eac)n(h)g(of)g(the)h
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end
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%%Page: 393 403
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%%Page: 409 419
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TeXDict begin 410 419 bop 0 52 a FG(410)1994 b Fz(C)91
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b(of)g(the)g(SideBand)g(attribute)g(in)g(eac)n(h)227
@@ -133093,7 +128814,7 @@ b(of)g(the)g(SideBand)g(attribute)g(in)g(eac)n(h)227
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@@ -133115,8 +128836,8 @@ b(The)28 b(default)g(v)-5 b(alue)27 b(for)g(AlignSideBand)h(is)f(zero.)
p eop end
%%Page: 411 421
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%%Page: 417 427
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@@ -133664,30 +129385,30 @@ b(T)31 b(and)h(CD)f(k)n(eyw)n(ords)f(are)g(in)i(units)g(of)f(degrees)f
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%%Page: 418 428
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227 1311 y(cess)i(the)g(con)n(ten)n(ts)f(of)h(the)g(FitsChan,)h(suc)n
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eop end
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%%Page: 451 461
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eop end
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end
%%Page: 496 506
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eop end
%%Page: 497 507
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%%Page: 516 526
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end
%%Page: 517 527
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@@ -141390,27 +137111,27 @@ g(a)f(new)i(Ob)5 b(ject)25 b(from)g(its)g(FITS)g(header)227
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y(When)21 b(y)n(ou)f(create)f(a)h(FitsChan,)i(y)n(ou)d(ha)n(v)n(e)g
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@@ -141436,11 +137157,11 @@ h(function)g(or)e(a)i(v)-5 b(alue)30 b(for)g(SinkFile,)i(an)n(y)d
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@@ -141453,7 +137174,7 @@ b(of)g(enco)r(dings)g(include)h(the)h(DSS)f(enco)r(ding)p
eop end
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%%Page: 528 538
@@ -142150,11 +137871,11 @@ TeXDict begin 528 537 bop 0 52 a FG(528)2251 b Fz(D)91
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end
%%Page: 529 539
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-Fc(F)-8 b(unctions)n(:)227 5504 y Fk(The)30 b(SelectorMap)e(class)g(do)
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f(whic)n(h)i(are)e(applicable)h(to)g(all)227 5603 y(Mappings.)p
eop end
@@ -143207,32 +138928,32 @@ TeXDict begin 542 551 bop 0 52 a FG(542)2251 b Fz(D)91
b(AST)30 b(CLASS)f(DESCRIPTIONS)p 0 351 3780 12 v 0 483
a FA(ShiftMap)306 b Fd(Add)39 b(a)f(constan)m(t)f(v)-7
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b(rame)34 b(whic)n(h)g(describ)r(es)g(celestial)g(longitude/latitude)
227 3826 y(co)r(ordinate)f(systems.)56 b(The)34 b(particular)f
@@ -143255,53 +138976,53 @@ b(See)27 b(attributes)h(SkyRef,)g(SkyRefIs,)f(SkyRefP)h(and)f
b(alues)33 b(used)g(b)n(y)g(a)g(SkyF)-7 b(rame)32 b(are)h(in)g
(radians.)52 b(These)33 b(ma)n(y)g(b)r(e)g(formatted)g(in)g(more)227
4669 y(con)n(v)n(en)n(tional)26 b(w)n(a)n(ys)g(for)h(displa)n(y)g(b)n
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+y Fj(The)28 b(SkyF)-7 b(rame)27 b(class)f(inherits)i(from)f(the)h(F)-7
b(rame)27 b(class.)-2 5350 y Fc(A)m(ttributes)n(:)227
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(all)g(F)-7 b(rames,)42 b(ev)n(ery)c(SkyF)-7 b(rame)39
b(also)g(has)g(the)h(follo)n(wing)227 5596 y(attributes:)p
eop end
%%Page: 543 553
TeXDict begin 543 552 bop 3643 52 a FG(543)340 351 y
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-y Fj(\017)45 b Fk(AST)p Ft(_)p Fk(SKYOFFSETMAP:)27 b(Obtain)h(a)f
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b(of)g(celestial)e(co)s(ordinate)f(con)m(v)m(ersions)326
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(sp)r(ecialised)f(form)h(of)g(Mapping)f(whic)n(h)h(can)g(b)r(e)g(used)g
(to)g(represen)n(t)f(a)g(sequence)227 3208 y(of)e(con)n(v)n(ersions)d
(b)r(et)n(w)n(een)i(standard)g(celestial)g(\(longitude,)h(latitude\))g
(co)r(ordinate)f(systems.)227 3338 y(When)d(an)e(SlaMap)h(is)g(\014rst)
f(created,)h(it)h(simply)f(p)r(erforms)f(a)g(unit)i(\(n)n(ull\))f
(Mapping)g(on)f(a)h(pair)f(of)h(co)r(ordinates.)227 3438
-y(Using)39 b(the)g(AST)p Ft(_)p Fk(SLAADD)h(routine,)h(a)e(series)f(of)
+y(Using)39 b(the)g(AST)p Ft(_)p Fj(SLAADD)h(routine,)h(a)e(series)f(of)
g(co)r(ordinate)g(con)n(v)n(ersion)e(steps)j(ma)n(y)f(then)h(b)r(e)h
(added,)227 3538 y(selected)34 b(from)f(those)h(pro)n(vided)e(b)n(y)i
(the)g(SLALIB)g(P)n(ositional)e(Astronom)n(y)g(Library)h(\(Starlink)g
@@ -143312,18 +139033,18 @@ b(ariet)n(y)29 b(of)h(celestial)g(co)r(ordinate)e(systems)i(to)227
f(pro)n(vided)f(b)n(y)i(SLALIB.)227 3867 y(F)-7 b(or)18
b(details)g(of)g(the)h(individual)g(co)r(ordinate)e(con)n(v)n(ersions)f
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-(class.)-2 4693 y Fc(A)m(ttributes)n(:)227 4839 y Fk(The)37
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b(SlaMap)f(class)g(do)r(es)g(not)h(de\014ne)g(an)n(y)f(new)h
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(all)227 4939 y(Mappings.)-2 5099 y Fc(F)-8 b(unctions)n(:)227
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(all)f(Mappings,)g(the)h(follo)n(wing)f(routine)g(ma)n(y)f(also)h(b)r
(e)h(applied)227 5345 y(to)i(all)f(SlaMaps:)340 5622
-y Fj(\017)45 b Fk(AST)p Ft(_)p Fk(SLAADD:)29 b(Add)g(a)e(celestial)g
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(co)r(ordinate)f(con)n(v)n(ersion)f(to)j(an)f(SlaMap)p
eop end
%%Page: 544 554
@@ -143332,7 +139053,7 @@ b(AST)30 b(CLASS)f(DESCRIPTIONS)p 0 351 3780 12 v 0 483
a FA(Sp)t(ecFluxF)-11 b(rame)1228 490 y Fd(Comp)s(ound)37
b(sp)s(ectrum/\015ux)1730 609 y(F)-10 b(rame)2871 483
y FA(Sp)t(ecFluxF)f(rame)0 773 y Fc(Description:)44 b
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b(rame)34 b(and)g(a)g(FluxF)-7 b(rame)35 b(in)n(to)f(a)g(single)g
(2-dimensional)227 872 y(comp)r(ound)24 b(F)-7 b(rame.)34
b(Suc)n(h)24 b(a)f(F)-7 b(rame)22 b(can)h(for)g(instance)g(b)r(e)h
@@ -143340,30 +139061,30 @@ b(Suc)n(h)24 b(a)f(F)-7 b(rame)22 b(can)h(for)g(instance)g(b)r(e)h
n(h)227 972 y(the)k(\014rst)g(axis)e(represen)n(ts)h(sp)r(ectral)g(p)r
(osition)g(and)g(the)h(second)f(axis)g(represen)n(ts)f(\015ux.)0
1120 y Fc(Constructor)32 b(F)-8 b(unction:)227 1220 y
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b(Ho)n(w)n(ev)n(er,)24 b(the)j(attributes)g(of)f(the)h(comp)r(onen)n(t)
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227 2008 y(attributes)d(of)f(the)h(Sp)r(ecFluxF)-7 b(rame.)36
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(an)n(y)f(attribute)i(name,)f(in)h(whic)n(h)f(case)f(the)i(request)e
(to)h(access)f(the)h(attribute)227 2307 y(will)d(b)r(e)g(forw)n(arded)e
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(de\014ne)g(an)n(y)f(new)g(routines)g(b)r(ey)n(ond)g(those)h(whic)n(h)f
(are)g(applicable)g(to)227 2701 y(all)f(CmpF)-7 b(rames.)p
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b(co)s(ordinate)g(system)h(description)3138 3029 y FA(Sp)t(ecF)-11
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b(rame)38 b(is)g(a)f(sp)r(ecialised)g(form)h(of)f(one-dimensional)g(F)
-7 b(rame)37 b(whic)n(h)h(represen)n(ts)e(v)-5 b(arious)227
3316 y(co)r(ordinate)22 b(systems)h(used)h(to)f(describ)r(e)g(p)r
@@ -143381,30 +139102,30 @@ r(o)r(c)n(h)f(of)h(observ)-5 b(ation,)23 b(units,)i(etc)f(\(see)f(the)h
(represen)n(t)e(o\013sets)i(from)227 3839 y(a)j(giv)n(en)g(sp)r(ectral)
g(p)r(osition,)h(rather)e(than)i(absolute)f(sp)r(ectral)g(v)-5
b(alues.)0 3987 y Fc(Constructor)32 b(F)-8 b(unction:)227
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%%Page: 546 556
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%%Page: 552 562
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%%Page: 553 563
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(the)h(mean)g(of)g(the)g(input)f(pixels)i(in)e(a)i(b)s(o)m(x)f(cen)m
@@ -146065,15 +141779,15 @@ s(d)f(called)j(AST)p Fy(_)p FG(AXDIST)-8 b(ANCE)32 b(whic)m(h)h
(o)g(supplied)e(axis)h(v)-5 b(alues.)59 b(F)-8 b(or)36
b(axes)h(b)s(elonging)f(to)h(SkyF)-8 b(rames,)38 b(the)f(returned)227
3570 y(v)-5 b(alue)31 b(is)g(normalized)f(in)m(to)i(the)e(range)h
-Fu(\006)p Fp(\031)s FG(.)111 3751 y(4.)46 b(The)31 b(F)-8
+Fu(\006)p Fo(\031)s FG(.)111 3751 y(4.)46 b(The)31 b(F)-8
b(rame)31 b(class)h(has)f(a)g(new)f(metho)s(d)h(called)h(AST)p
Fy(_)p FG(AX)m(OFFSET)e(whic)m(h)g(returns)g(an)h(axis)g(v)-5
b(alue)227 3863 y(a)40 b(giv)m(en)g(incremen)m(t)g(a)m(w)m(a)m(y)i
(from)d(a)g(sp)s(eci\014ed)g(axis)h(v)-5 b(alue.)68 b(F)-8
b(or)40 b(axes)g(b)s(elonging)g(to)g(SkyF)-8 b(rames,)227
3976 y(the)34 b(returned)f(v)-5 b(alue)34 b(is)f(normalized)i(in)m(to)f
-(the)g(range)g Fu(\006)p Fp(\031)j FG(\(for)c(latitude)i(axes\))g(or)e
-(zero)i(to)f(2)p Fp(\031)j FG(\(for)227 4089 y(longitude)31
+(the)g(range)g Fu(\006)p Fo(\031)j FG(\(for)c(latitude)i(axes\))g(or)e
+(zero)i(to)f(2)p Fo(\031)j FG(\(for)227 4089 y(longitude)31
b(axes\).)111 4270 y(5.)46 b(The)27 b(Plot)i(class)f(has)g(a)g(new)f
(metho)s(d)g(called)i(AST)p Fy(_)p FG(GENCUR)-10 b(VE)27
b(whic)m(h)g(allo)m(ws)i(generalised)g(user-)227 4383
@@ -146135,8 +141849,8 @@ b(v)m(ersions)g(V1.7)g(and)f(V1.8-2:)111 2986 y(1.)46
b(The)33 b(SkyF)-8 b(rame)34 b(class)h(has)e(a)h(new)f(attribute)h
(called)h(NegLon)f(whic)m(h)g(allo)m(ws)h(longitude)f(v)-5
b(alues)34 b(to)227 3099 y(b)s(e)c(displa)m(y)m(ed)h(in)f(the)h(range)f
-Fu(\000)p Fp(\031)j FG(to)f(+)p Fp(\031)s FG(,)e(instead)h(of)f(the)h
-(usual)f(range)g(zero)h(to)h(2)p Fp(:\031)s FG(.)111
+Fu(\000)p Fo(\031)j FG(to)f(+)p Fo(\031)s FG(,)e(instead)h(of)f(the)h
+(usual)f(range)g(zero)h(to)h(2)p Fo(:\031)s FG(.)111
3327 y(2.)46 b(Some)29 b(new)f(routines)g(\(AST)p Fy(_)p
FG(ANGLE,)h(AST)p Fy(_)p FG(AXANGLE,)g(AST)p Fy(_)p FG(RESOL)-10
b(VE,)26 b(AST)p Fy(_)p FG(OFFSET2,)227 3440 y(AST)p
@@ -147153,9 +142867,9 @@ Fy(__)p FG(SOMB)f(and)f(AST)p Fy(__)p FG(SOMBCOS)f(ha)m(v)m(e)k(b)s
(een)e(added)f(to)j(AST)p Fy(_)p FG(P)-8 b(AR.)21 b(These)227
1877 y(sp)s(ecify)j(k)m(ernels)h(for)g(AST)p Fy(_)p FG(RESAMPLE)e(and)h
(AST)p Fy(_)p FG(REBIN)f(based)h(on)h(the)g(\\Som)m(brero")g(function)
-227 1990 y(\()31 b(2)21 b Fu(\003)f Fp(J)9 b FG(1\()p
-Fp(x)p FG(\))p Fp(=x)32 b FG(where)e Fp(J)9 b FG(1\()p
-Fp(x)p FG(\))32 b(is)e(the)h(\014rst)e(order)h(Bessel)i(function)e(of)g
+227 1990 y(\()31 b(2)21 b Fu(\003)f Fo(J)9 b FG(1\()p
+Fo(x)p FG(\))p Fo(=x)32 b FG(where)e Fo(J)9 b FG(1\()p
+Fo(x)p FG(\))32 b(is)e(the)h(\014rst)e(order)h(Bessel)i(function)e(of)g
(the)h(\014rst)e(kind\).)111 2177 y(3.)46 b(The)f(SkyF)-8
b(rame)45 b(class)g(no)m(w)g(supp)s(orts)e(a)i(System)g(v)-5
b(alue)45 b(of)g(AZEL)f(corresp)s(onding)g(to)h(horizon)227
@@ -148044,25 +143758,43 @@ eop end
TeXDict begin 605 614 bop 0 52 a Fz(G.45)92 b(Changes)31
b(In)m(tro)s(duced)e(in)h(V6.0-1)2174 b FG(605)0 351
y Fw(G.45)112 b(Changes)39 b(In)m(tro)s(duced)f(in)f(V6.0-1)0
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-2037 y(new)30 b(facilities.)p eop end
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+Fu(\000)g Fo(<)g(r)s(el)r(ease)g(>)p FG(")227 1662 y(to)31
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+eop end
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userdict /end-hook known{end-hook}if
diff --git a/sun210.tex b/sun210.tex
index 9ed1a14..e4dd5b3 100644
--- a/sun210.tex
+++ b/sun210.tex
@@ -17,17 +17,17 @@
\newcommand{\stardocsource} {sun\stardocnumber}
% Variable part - replace [xxx] as appropriate.
-\newcommand{\stardocnumber} {210.26}
+\newcommand{\stardocnumber} {210.27}
\newcommand{\stardocauthors} {R.F. Warren-Smith \& D.S. Berry}
-\newcommand{\stardocdate} {4th October 2011}
+\newcommand{\stardocdate} {16th February 2012}
\newcommand{\stardoctitle} {AST\\
A Library for Handling\\
World Coordinate Systems\\
in Astronomy}
-\newcommand{\stardoccopyright} {Copyright (C) 2009 Science \& Technology Facilities Council}
+\newcommand{\stardoccopyright} {Copyright (C) 2012 Science \& Technology Facilities Council}
\newcommand{\stardoctitlehtml} {AST - A Library for Handling World Coordinate
Systems in Astronomy}
-\newcommand{\stardocversion} {V6.0}
+\newcommand{\stardocversion} {V7.0}
\newcommand{\stardocmanual} {Programmer's Guide\\(Fortran Version)}
\newcommand{\stardocmanualhtml}{Programmer's Guide (Fortran Version)}
\newcommand{\stardocabstract} {
@@ -777,10 +777,11 @@ are described here:
\begin{enumerate}
\item {\bf{Minimum Software Dependencies.}}
-The AST library depends on no other other software\footnote{It now comes with a
-minimal cut-down version of the widely-available SLALIB positional astronomy
-library (\xref{SUN/67}{sun67}{}), including just those functions needed
-by AST, and the previous dependency on SLALIB is no longer present}.
+The AST library depends on no other other software\footnote{It comes with
+bundled copies of the IAU SOFA and Starlink PAL libraries which are built
+at the same time as the other AST internal libraries. Alternatively, external
+PAL and SOFA libraries may be used by specifying the ``{\tt
+--with-external\_pal}'' option when configuring AST}.
\item {\bf{Environment Independence.}}
AST is designed so that it can operate in a variety of ``programming
@@ -47000,20 +47001,16 @@ in a non-standard location.} is on your PATH.
}
}
\sstdiytopic{
- SLALIB
+ SOFA \& PAL
}{
- The AST distribution includes a cut down subset of the C version of
- the SLALIB library written by Pat Wallace. This subset contains only
- the functions needed by the AST library. It is built as part of the
- process of building AST and is distributed under GPL (and is thus
- compatible with the AST license). Previous version of this script
- allowed AST applications to be linked against external SLALIB
- libraries (either Fortran or C) rather than the internal version.
- The current version of this script does not provide this option,
- and always uses the internal SLALIB library. However, for backward
- compatibility, this script still allows the {\tt{"}}-fsla{\tt{"}} and {\tt{"}}-csla{\tt{"}} flags
- (previously used for selecting which version of SLALIB to use) to be
- specified, but they will be ignored.
+ The AST distribution includes bundled copies of the IAU SOFA and
+ Starlink PAL libraries. These will be used for fundamental
+ positional astronomy calculations unless the {\tt{"}}--with-external\_pal{\tt{"}}
+ option was used when AST was configured. If {\tt{"}}--with-external\_pal{\tt{"}}
+ is used, this script will include {\tt{"}}-lpal{\tt{"}} in the returned list of
+ linking options, and the user should then ensure that extrnal copies
+ of the PAL and SOFA libraries are available (SOFA functions are used
+ within PAL).
}
}
\sstroutine{
@@ -49974,12 +49971,10 @@ routine \htmlref{AST\_TUNEC}{AST_TUNEC}.
\end{enumerate}
-\subsection{\xlabel{changes}\xlabel{list_of_most_recent_changes}Changes
-Introduced in V6.0-1}
+\subsection{Changes Introduced in V6.0-1}
-The following describes the most significant changes which have
-occurred in the AST library between versions V6.0 and V6.0-1 (the
-current version):
+The following describes the most significant changes which
+occurred in the AST library between versions V6.0 and V6.0-1:
\begin{enumerate}
@@ -49995,6 +49990,25 @@ be used when aligning SkyFrames if the \htmlref{AlignSystem}{AlignSystem} attrib
\end{enumerate}
+\subsection{\xlabel{changes}\xlabel{list_of_most_recent_changes}Changes
+Introduced in V7.0.0}
+
+The following describes the most significant changes which have
+occurred in the AST library between versions V6.0-1 and V7.0.0 (the
+current version):
+
+\begin{enumerate}
+
+\item Fundamental positional astronomy calculations are now performed
+using the IAU SOFA library where possible, and the Starlink PAL library
+otherwise (the PAL library contains a subset of the Fortran Starlink SLALIB
+library re-written in C). Copies of these libraries are bundled with AST
+and so do not need to be obtained or built separately, although external
+copies of SOFA and PAL can be used if necessary by including the
+``{\tt --with-external\_pal}'' option when configuring AST.
+
+\end{enumerate}
+
Programs which are statically linked will need to be re-linked in
order to take advantage of these new facilities.
diff --git a/sun211.htx_tar b/sun211.htx_tar
index 087eefe..cde1ee0 100644
Binary files a/sun211.htx_tar and b/sun211.htx_tar differ
diff --git a/sun211.ps b/sun211.ps
index d4cc7a9..189f40b 100644
--- a/sun211.ps
+++ b/sun211.ps
@@ -1,19 +1,19 @@
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+%%Creator: dvips(k) 5.96.1 Copyright 2007 Radical Eye Software
%%Title: sun211.dvi
-%%CreationDate: Wed Jan 11 22:22:16 2012
-%%Pages: 635
+%%CreationDate: Tue Mar 13 09:57:22 2012
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%DVIPSWebPage: (www.radicaleye.com)
%DVIPSCommandLine: dvips -f sun211
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+%DVIPSSource: TeX output 2012.03.13:0957
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMBX10
-%!PS-AdobeFont-1.0: CMBX10 003.002
-%%Title: CMBX10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMBX10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMBX10 known{/CMBX10 findfont dup/UniqueID known{dup
-/UniqueID get 5000768 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMBX10 1.00B
+%%CreationDate: 1992 Feb 19 19:54:06
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMBX10 def
-/FontBBox {-56 -250 1164 750 }readonly def
-/UniqueID 5000768 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMBX10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.00B) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMBX10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Bold) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMBX10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -747,6 +370,7 @@ dup 12 /fi put
dup 13 /fl put
dup 15 /ffl put
dup 34 /quotedblright put
+dup 38 /ampersand put
dup 40 /parenleft put
dup 41 /parenright put
dup 43 /plus put
@@ -822,702 +446,472 @@ dup 121 /y put
dup 122 /z put
dup 124 /emdash put
readonly def
+/FontBBox{-301 -250 1164 946}readonly def
currentdict end
currentfile eexec
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@@ -1527,41 +921,25 @@ EF2020AB74B2907D6A95B63E2494C702836AEDD492960C9B1B45657246
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMR12
-%!PS-AdobeFont-1.0: CMR12 003.002
-%%Title: CMR12
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMR12.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMR12 known{/CMR12 findfont dup/UniqueID known{dup
-/UniqueID get 5000794 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMR12 1.0
+%%CreationDate: 1991 Aug 20 16:38:05
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMR12 def
-/FontBBox {-34 -251 988 750 }readonly def
-/UniqueID 5000794 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMR12.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMR12) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMR12 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -1582,7 +960,7 @@ dup 50 /two put
dup 51 /three put
dup 52 /four put
dup 53 /five put
-dup 54 /six put
+dup 55 /seven put
dup 57 /nine put
dup 63 /question put
dup 65 /A put
@@ -1635,612 +1013,399 @@ dup 120 /x put
dup 121 /y put
dup 122 /z put
readonly def
+/FontBBox{-34 -251 988 750}readonly def
currentdict end
currentfile eexec
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-%%EndFont
-%%BeginFont: CMTT9
-%!PS-AdobeFont-1.0: CMTT9 003.002
-%%Title: CMTT9
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMTT9.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMTT9 known{/CMTT9 findfont dup/UniqueID known{dup
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%%EndFont
%%BeginFont: CMTI9
-%!PS-AdobeFont-1.0: CMTI9 003.002
-%%Title: CMTI9
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMTI9.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMTI9 known{/CMTI9 findfont dup/UniqueID known{dup
-/UniqueID get 5000827 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMTI9 1.0
+%%CreationDate: 1991 Aug 18 21:08:07
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMTI9 def
-/FontBBox {-35 -250 1148 750 }readonly def
-/UniqueID 5000827 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMTI9.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMTI9) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMTI9 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 46 /period put
@@ -2535,229 +1444,72 @@ dup 105 /i put
dup 116 /t put
dup 118 /v put
readonly def
+/FontBBox{-35 -250 1148 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMMI8
-%!PS-AdobeFont-1.0: CMMI8 003.002
-%%Title: CMMI8
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMMI8.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMMI8 known{/CMMI8 findfont dup/UniqueID known{dup
-/UniqueID get 5087383 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMMI8 1.100
+%%CreationDate: 1996 Jul 23 07:53:54
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMMI8 def
-/FontBBox {-24 -250 1110 750 }readonly def
-/UniqueID 5087383 def
-/PaintType 0 def
-/FontInfo 10 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMMI8.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.100) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMMI8) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
-/ascent 750 def
end readonly def
+/FontName /CMMI8 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 58 /period put
@@ -2821,274 +1556,121 @@ dup 115 /s put
dup 116 /t put
dup 117 /u put
readonly def
+/FontBBox{-24 -250 1110 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMSY10
-%!PS-AdobeFont-1.0: CMSY10 003.002
-%%Title: CMSY10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMSY10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMSY10 known{/CMSY10 findfont dup/UniqueID known{dup
-/UniqueID get 5096651 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMSY10 1.0
+%%CreationDate: 1991 Aug 15 07:20:57
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMSY10 def
-/FontBBox {-29 -960 1116 775 }readonly def
-/UniqueID 5096651 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMSY10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMSY10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
-/ItalicAngle -14.04 def
+/ItalicAngle -14.035 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMSY10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 0 /minus put
@@ -3149,250 +1715,81 @@ dup 110 /backslash put
dup 112 /radical put
dup 120 /section put
readonly def
+/FontBBox{-29 -960 1116 775}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMR10
-%!PS-AdobeFont-1.0: CMR10 003.002
-%%Title: CMR10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMR10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMR10 known{/CMR10 findfont dup/UniqueID known{dup
-/UniqueID get 5000793 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMR10 1.00B
+%%CreationDate: 1992 Feb 19 19:54:52
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMR10 def
-/FontBBox {-40 -250 1009 750 }readonly def
-/UniqueID 5000793 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMR10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.00B) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMR10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMR10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -3533,805 +1914,549 @@ dup 122 /z put
dup 123 /endash put
dup 124 /emdash put
readonly def
+/FontBBox{-251 -250 1009 969}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMMI7
-%!PS-AdobeFont-1.0: CMMI7 003.002
-%%Title: CMMI7
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMMI7.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMMI7 known{/CMMI7 findfont dup/UniqueID known{dup
-/UniqueID get 5087382 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMMI7 1.100
+%%CreationDate: 1996 Jul 23 07:53:53
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMMI7 def
-/FontBBox {-1 -250 1171 750 }readonly def
-/UniqueID 5087382 def
-/PaintType 0 def
-/FontInfo 10 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMMI7.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.100) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMMI7) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
-/ascent 750 def
end readonly def
+/FontName /CMMI7 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 76 /L put
@@ -4394,274 +2502,119 @@ dup 115 /s put
dup 116 /t put
dup 117 /u put
readonly def
+/FontBBox{0 -250 1171 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMMI10
-%!PS-AdobeFont-1.0: CMMI10 003.002
-%%Title: CMMI10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMMI10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMMI10 known{/CMMI10 findfont dup/UniqueID known{dup
-/UniqueID get 5087385 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMMI10 1.100
+%%CreationDate: 1996 Jul 23 07:53:57
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMMI10 def
-/FontBBox {-32 -250 1048 750 }readonly def
-/UniqueID 5087385 def
-/PaintType 0 def
-/FontInfo 10 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMMI10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.100) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMMI10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
-/ascent 750 def
end readonly def
+/FontName /CMMI10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 22 /mu put
@@ -4742,389 +2678,231 @@ dup 120 /x put
dup 121 /y put
dup 122 /z put
readonly def
+/FontBBox{-32 -250 1048 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMSY9
-%!PS-AdobeFont-1.0: CMSY9 003.002
-%%Title: CMSY9
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMSY9.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMSY9 known{/CMSY9 findfont dup/UniqueID known{dup
-/UniqueID get 5096650 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMSY9 1.0
+%%CreationDate: 1991 Aug 15 07:22:27
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMSY9 def
-/FontBBox {-29 -958 1146 777 }readonly def
-/UniqueID 5096650 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMSY9.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMSY9) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
-/ItalicAngle -14.04 def
+/ItalicAngle -14.035 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMSY9 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 0 /minus put
dup 3 /asteriskmath put
readonly def
+/FontBBox{-30 -958 1146 777}readonly def
currentdict end
currentfile eexec
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%%EndFont
%%BeginFont: CMMI9
-%!PS-AdobeFont-1.0: CMMI9 003.002
-%%Title: CMMI9
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMMI9.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMMI9 known{/CMMI9 findfont dup/UniqueID known{dup
-/UniqueID get 5087384 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMMI9 1.100
+%%CreationDate: 1996 Jul 23 07:53:55
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMMI9 def
-/FontBBox {-29 -250 1075 750 }readonly def
-/UniqueID 5087384 def
-/PaintType 0 def
-/FontInfo 10 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMMI9.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.100) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMMI9) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
-/ascent 750 def
end readonly def
+/FontName /CMMI9 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 58 /period put
readonly def
+/FontBBox{-29 -250 1075 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMSY8
-%!PS-AdobeFont-1.0: CMSY8 003.002
-%%Title: CMSY8
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMSY8.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMSY8 known{/CMSY8 findfont dup/UniqueID known{dup
-/UniqueID get 5096649 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMSY8 1.0
+%%CreationDate: 1991 Aug 15 07:22:10
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMSY8 def
-/FontBBox {-30 -955 1185 779 }readonly def
-/UniqueID 5096649 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMSY8.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMSY8) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
-/ItalicAngle -14.04 def
+/ItalicAngle -14.035 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMSY8 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 0 /minus put
dup 14 /openbullet put
readonly def
+/FontBBox{-30 -955 1185 779}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMTT10
-%!PS-AdobeFont-1.0: CMTT10 003.002
-%%Title: CMTT10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMTT10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMTT10 known{/CMTT10 findfont dup/UniqueID known{dup
-/UniqueID get 5000832 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMTT10 1.00B
+%%CreationDate: 1992 Apr 26 10:42:42
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMTT10 def
-/FontBBox {-4 -233 537 696 }readonly def
-/UniqueID 5000832 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMTT10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.00B) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMTT10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch true def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMTT10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 33 /exclam put
@@ -5986,653 +3210,468 @@ dup 123 /braceleft put
dup 124 /bar put
dup 125 /braceright put
readonly def
+/FontBBox{-4 -235 731 800}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
-%%BeginFont: CMR9
-%!PS-AdobeFont-1.0: CMR9 003.002
-%%Title: CMR9
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMR9.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMR9 known{/CMR9 findfont dup/UniqueID known{dup
-/UniqueID get 5000792 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%%BeginFont: CMTT9
+%!PS-AdobeFont-1.1: CMTT9 1.0
+%%CreationDate: 1991 Aug 20 16:46:24
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMR9 def
-/FontBBox {-39 -250 1036 750 }readonly def
-/UniqueID 5000792 def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
+/FullName (CMTT9) readonly def
+/FamilyName (Computer Modern) readonly def
+/Weight (Medium) readonly def
+/ItalicAngle 0 def
+/isFixedPitch true def
+end readonly def
+/FontName /CMTT9 def
/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMR9.) readonly def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
+/Encoding 256 array
+0 1 255 {1 index exch /.notdef put} for
+dup 45 /hyphen put
+dup 95 /underscore put
+dup 97 /a put
+dup 101 /e put
+dup 104 /h put
+dup 105 /i put
+dup 108 /l put
+dup 110 /n put
+dup 112 /p put
+dup 114 /r put
+dup 116 /t put
+dup 119 /w put
+dup 120 /x put
+readonly def
+/FontBBox{-6 -233 542 698}readonly def
+currentdict end
+currentfile eexec
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+cleartomark
+%%EndFont
+%%BeginFont: CMR9
+%!PS-AdobeFont-1.1: CMR9 1.0
+%%CreationDate: 1991 Aug 20 16:39:59
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
+11 dict begin
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMR9) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMR9 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -6696,7 +3848,6 @@ dup 49 /one put
dup 50 /two put
dup 51 /three put
dup 53 /five put
-dup 54 /six put
dup 55 /seven put
dup 56 /eight put
dup 58 /colon put
@@ -6752,635 +3903,390 @@ dup 120 /x put
dup 121 /y put
dup 122 /z put
readonly def
+/FontBBox{-39 -250 1036 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMR6
-%!PS-AdobeFont-1.0: CMR6 003.002
-%%Title: CMR6
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMR6.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMR6 known{/CMR6 findfont dup/UniqueID known{dup
-/UniqueID get 5000789 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMR6 1.0
+%%CreationDate: 1991 Aug 20 16:39:02
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMR6 def
-/FontBBox {-20 -250 1193 750 }readonly def
-/UniqueID 5000789 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMR6.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMR6) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMR6 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 48 /zero put
@@ -7438,243 +4328,91 @@ dup 55 /seven put
dup 56 /eight put
dup 57 /nine put
readonly def
+/FontBBox{-20 -250 1193 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMR8
-%!PS-AdobeFont-1.0: CMR8 003.002
-%%Title: CMR8
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMR8.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMR8 known{/CMR8 findfont dup/UniqueID known{dup
-/UniqueID get 5000791 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMR8 1.0
+%%CreationDate: 1991 Aug 20 16:39:40
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMR8 def
-/FontBBox {-36 -250 1070 750 }readonly def
-/UniqueID 5000791 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMR8.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMR8) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMR8 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 48 /zero put
@@ -7732,243 +4454,91 @@ dup 55 /seven put
dup 56 /eight put
dup 57 /nine put
readonly def
+/FontBBox{-36 -250 1070 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMBX12
-%!PS-AdobeFont-1.0: CMBX12 003.002
-%%Title: CMBX12
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMBX12.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMBX12 known{/CMBX12 findfont dup/UniqueID known{dup
-/UniqueID get 5000769 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMBX12 1.0
+%%CreationDate: 1991 Aug 20 16:34:54
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMBX12 def
-/FontBBox {-53 -251 1139 750 }readonly def
-/UniqueID 5000769 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMBX12.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMBX12) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Bold) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMBX12 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -8090,598 +4644,386 @@ dup 121 /y put
dup 122 /z put
dup 124 /emdash put
readonly def
+/FontBBox{-53 -251 1139 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMTI10
-%!PS-AdobeFont-1.0: CMTI10 003.002
-%%Title: CMTI10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMTI10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMTI10 known{/CMTI10 findfont dup/UniqueID known{dup
-/UniqueID get 5000828 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMTI10 1.00B
+%%CreationDate: 1992 Feb 19 19:56:16
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMTI10 def
-/FontBBox {-35 -250 1124 750 }readonly def
-/UniqueID 5000828 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMTI10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.00B) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMTI10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -14.04 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMTI10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -8781,556 +5107,371 @@ dup 119 /w put
dup 120 /x put
dup 121 /y put
readonly def
+/FontBBox{-163 -250 1146 969}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMSL10
-%!PS-AdobeFont-1.0: CMSL10 003.002
-%%Title: CMSL10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMSL10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMSL10 known{/CMSL10 findfont dup/UniqueID known{dup
-/UniqueID get 5000798 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMSL10 1.0
+%%CreationDate: 1991 Aug 20 16:40:20
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMSL10 def
-/FontBBox {-62 -250 1123 750 }readonly def
-/UniqueID 5000798 def
-/PaintType 0 def
-/FontInfo 9 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMSL10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMSL10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle -9.46 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
end readonly def
+/FontName /CMSL10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 11 /ff put
@@ -9445,631 +5570,421 @@ dup 120 /x put
dup 121 /y put
dup 124 /emdash put
readonly def
+/FontBBox{-62 -250 1123 750}readonly def
currentdict end
currentfile eexec
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cleartomark
-{restore}if
%%EndFont
%%BeginFont: CMCSC10
-%!PS-AdobeFont-1.0: CMCSC10 003.002
-%%Title: CMCSC10
-%Version: 003.002
-%%CreationDate: Mon Jul 13 16:17:00 2009
-%%Creator: David M. Jones
-%Copyright: Copyright (c) 1997, 2009 American Mathematical Society
-%Copyright: (<http://www.ams.org>), with Reserved Font Name CMCSC10.
-% This Font Software is licensed under the SIL Open Font License, Version 1.1.
-% This license is in the accompanying file OFL.txt, and is also
-% available with a FAQ at: http://scripts.sil.org/OFL.
-%%EndComments
-FontDirectory/CMCSC10 known{/CMCSC10 findfont dup/UniqueID known{dup
-/UniqueID get 5087402 eq exch/FontType get 1 eq and}{pop false}ifelse
-{save true}{false}ifelse}{false}ifelse
+%!PS-AdobeFont-1.1: CMCSC10 1.0
+%%CreationDate: 1991 Aug 18 17:46:49
+% Copyright (C) 1997 American Mathematical Society. All Rights Reserved.
11 dict begin
-/FontType 1 def
-/FontMatrix [0.001 0 0 0.001 0 0 ]readonly def
-/FontName /CMCSC10 def
-/FontBBox {14 -250 1077 750 }readonly def
-/UniqueID 5087402 def
-/PaintType 0 def
-/FontInfo 10 dict dup begin
-/version (003.002) readonly def
-/Notice (Copyright \050c\051 1997, 2009 American Mathematical Society \050<http://www.ams.org>\051, with Reserved Font Name CMCSC10.) readonly def
+/FontInfo 7 dict dup begin
+/version (1.0) readonly def
+/Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def
/FullName (CMCSC10) readonly def
/FamilyName (Computer Modern) readonly def
/Weight (Medium) readonly def
/ItalicAngle 0 def
/isFixedPitch false def
-/UnderlinePosition -100 def
-/UnderlineThickness 50 def
-/ascent 750 def
end readonly def
+/FontName /CMCSC10 def
+/PaintType 0 def
+/FontType 1 def
+/FontMatrix [0.001 0 0 0.001 0 0] readonly def
/Encoding 256 array
0 1 255 {1 index exch /.notdef put} for
dup 65 /A put
@@ -10135,296 +6033,122 @@ dup 116 /t put
dup 117 /u put
dup 121 /y put
readonly def
+/FontBBox{14 -250 1077 750}readonly def
currentdict end
currentfile eexec
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%%Page: 68 78
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1148 y(y)m(our)30 b(instrumen)m(t.)0 1317 y(F)-8 b(or)37
b(some)g(purp)s(oses,)g(ho)m(w)m(ev)m(er,)j(a)d(standard)e(c)m(hoice)k
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1329 V 296 w(10)2030 1262 y Fv(2)2547 1295 y FF(hecto)118
b(h)p 3161 1329 V 615 1442 V 667 1408 a(10)757 1375 y
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V 260 w(10)2030 1375 y Fv(3)2547 1408 y FF(kilo)186 b(k)p
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1488 y Fv(6)2547 1521 y FF(mega)123 b(M)p 3161 1555 V
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Fv(12)2547 1747 y FF(tera)k(T)p 3161 1781 V 615 1894
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y FF(fem)m(to)109 b(f)p 1888 1894 V 308 w(10)2030 1827
y Fv(15)2547 1860 y FF(p)s(eta)155 b(P)p 3161 1894 V
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2086 y FF(zepto)119 b(z)p 1888 2120 V 296 w(10)2030 2053
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2166 y Fv(24)2547 2199 y FF(y)m(otta)124 b(Y)p 3161 2233
V 617 2236 2546 4 v 590 3621 2601 4 v 588 3734 4 113
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121 w(m)m(ultiplication)h(\(a)f(dot\))p 3188 4192 V 588
4305 V 639 4271 a(sym1/sym2)p 1143 4305 V 101 w(division)p
3188 4305 V 588 4418 V 639 4384 a(sym1**y)p 1143 4418
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3188 4531 V 588 4644 V 639 4610 a(log\(sym1\))p 1143
4644 V 166 w(common)f(logarithm)p 3188 4644 V 588 4756
V 639 4723 a(ln\(sym1\))p 1143 4756 V 205 w(natural)g(logarithm)p
@@ -92193,7 +87914,7 @@ b(of)g(these)g(attributes)g(explicitly)h(unless)e(y)m(ou)h(ha)m(v)m(e)h
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@@ -92204,7 +87925,7 @@ eop end
%%Page: 86 96
TeXDict begin 86 95 bop 0 52 a FF(86)1229 b Fy(8)91 b(CELESTIAL)29
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b(=)g("Declination")379 b(#)47 b(Label)f(for)h(axis)g(2)418
@@ -92225,7 +87946,7 @@ b(Coordinate)e(system)h(description)227 2158 y(#)143
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(all)h(set)f(to)g(v)-5 b(alues)32 b(appropriate)0 2728
@@ -92291,7 +88012,7 @@ b(A)32 b(range)h(of)f(\014eld)g(separators)h(is)g(also)0
a FD(F)-9 b(ormat)35 b(Sp)s(eci\014er)p 1667 1334 V 100
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V 811 1337 2158 4 v 811 1354 V 809 1467 4 113 v 861 1433
-a Fq(d)p 1667 1467 V 809 w(219)p 2967 1467 V 809 1579
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V 861 1546 a(d.3)p 1667 1579 V 713 w(219.123)p 2967 1579
V 809 1692 V 861 1659 a(dm)p 1667 1692 V 761 w(219:05)p
2967 1692 V 809 1805 V 861 1771 a(dm.2)p 1667 1805 V
@@ -92318,7 +88039,7 @@ b(to)f(whether)e(the)i(v)-5 b(alue)35 b(is)f(to)h(b)s(e)f(formatted)h
b(b)m(y)f(including)g(\\t")h(to)h(request)e(time.)136
3938 y Fu(\017)46 b FF(The)35 b(n)m(um)m(b)s(er)g(of)g(decimal)i
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4051 y(in)m(teger.)k(An)23 b(asterisk)i(can)e(b)s(e)g(used)g(in)g
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b(lo)m(w)m(er)h(or)f(upp)s(er)e(case)j(ma)m(y)g(b)s(e)e(used.)75
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FF(")h(or)e(\\22h14m11.2s"\).)p eop end
%%Page: 89 99
TeXDict begin 89 98 bop 0 52 a Fy(8.7)92 b(Reading)31
@@ -92436,11 +88157,11 @@ b FF(89)136 351 y Fu(\017)46 b FF(The)30 b(presence)h(of)f(certain)i
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FF({)e(angle)477 1018 y(h)f({)h(time)227 1233 y(Incompatible)36
b(angle/time)i(iden)m(ti\014cation)f(c)m(haracters)g(ma)m(y)f(not)g(b)s
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FF({)100 b(arc-min)m(utes)31 b(and)f(arc-seconds)477
3182 y(9h13s)161 b({)100 b(hours)29 b(and)h(seconds)g(of)g(time)477
3295 y(:45:33)153 b({)100 b(min)m(utes)30 b(and)g(seconds)g(\(of)h(arc)
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@@ -92518,9 +88239,9 @@ b(and)f(seconds)277 804 y(12)244 b({)100 b(min)m(utes)277
917 y(:13)219 b({)100 b(seconds)277 1030 y Fu(\000)p
FF(18:)148 b({)100 b(min)m(utes)277 1142 y(12.8)174 b({)100
b(min)m(utes)277 1255 y(1)31 b(2)g(3)137 b({)100 b(hours,)30
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FF({)g(arc-min)m(utes)277 1820 y Fu(\000)p FF(33h)122
b({)100 b(hours)0 2070 y(\(in)36 b(the)h(last)g(four)f(cases,)i
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378 b(#)47 b(Standard)f(of)h(rest)418 4115 y(RstFrq)f(=)i(250000000000)
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(set)f(to)h(v)-5 b(alues)30 b(appropriate)g(for)0 4701
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(System)f(v)-5 b(alue)0 4973 y(w)m(ere)32 b(set,)g(the)g(defaults)f(w)m
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@@ -103590,7 +99311,7 @@ b(means)g(they)227 4463 y(will)d(b)s(e)f(aligned)h(so)f(that)h(the)g
(\014rst)f(elemen)m(t)h(their)g(data)g(arra)m(ys)g(corresp)s(ond.)111
4640 y(4.)46 b(If)27 b(all)i(of)e(the)h(ab)s(o)m(v)m(e)g(fail,)h
(astCon)m(v)m(ert)g(will)f(return)f(the)g(v)-5 b(alue)28
-b(AST)p Fq(__)p FF(NULL.)e(Otherwise)i(a)f(p)s(oin)m(ter)227
+b(AST)p Fp(__)p FF(NULL.)e(Otherwise)i(a)f(p)s(oin)m(ter)227
4753 y(to)k(a)g(F)-8 b(rameSet)32 b(will)e(b)s(e)g(returned.)0
4976 y(The)35 b(resulting)g(\\cvt")i(F)-8 b(rameSet)36
b(ma)m(y)g(then)f(b)s(e)g(used)f(directly)i(\()p Fu(x)p
@@ -103685,7 +99406,7 @@ b(rame)33 b(w)m(e)g(w)m(an)m(t)h(to)0 5442 y(alter)d(and)f(all)h(the)g
b(\(Figure)f(14\).)p 0 5516 1512 4 v 73 5570 a Fs(22)138
5602 y Fr(This)d(is)g(b)r(ecause)f(an)n(y)g(transformation)i(to)e(or)h
(from)g(this)f(new)g(F)-6 b(rame)28 b(m)n(ust)f(go)h
-Fg(via)f Fr(the)f(base)i(F)-6 b(rame)27 b(represen)n(ting)h(the)0
+Ff(via)f Fr(the)f(base)i(F)-6 b(rame)27 b(represen)n(ting)h(the)0
5693 y(original)f(data)f(grid)g(co)r(ordinate)h(system,)f(whic)n(h)g(w)
n(e)g(assume)g(w)n(as)h(correctly)f(related)h(to)e(all)i(the)e(other)h
(F)-6 b(rames)26 b(presen)n(t.)p eop end
@@ -111884,7 +107605,7 @@ b(ject's)29 b(textual)h(description.)40 b(If)29 b(y)m(ou)g(then)f(p)s
(rep)s(eated)0 1396 y(to)k(read)g(eac)m(h)h(Ob)5 b(ject)33
b(in)f(turn.)47 b(When)33 b(there)f(are)i(no)e(more)h(Ob)5
b(jects)33 b(to)g(b)s(e)f(read,)i(astRead)f(will)h(return)0
-1509 y(the)d(v)-5 b(alue)30 b(AST)p Fq(__)p FF(NULL)g(to)h(indicate)g
+1509 y(the)d(v)-5 b(alue)30 b(AST)p Fp(__)p FF(NULL)g(to)h(indicate)g
(an)f Fx(end-of-\014le.)0 1790 y Fw(15.6)112 b(V)-9 b(alidating)39
b(Input)0 2003 y FF(The)29 b(p)s(oin)m(ter)h(returned)f(b)m(y)h
(astRead)h(\()p Fu(x)p FF(15.4\))h(could)e(iden)m(tify)h(an)m(y)f
@@ -111893,8 +107614,8 @@ b(Input)0 2003 y FF(The)29 b(p)s(oin)m(ter)h(returned)f(b)m(y)h
(read.)52 b(If)34 b(it)h(is)f(necessary)g(to)h(test)h(for)e(a)g
(particular)h(class)g(\(sa)m(y)g(a)0 2229 y(F)-8 b(rame\),)28
b(this)e(ma)m(y)h(b)s(e)e(done)h(as)g(follo)m(ws)i(using)d(the)h
-(appropriate)g(mem)m(b)s(er)g(of)g(the)g(astIsA)p Fo(<)p
-FF(Class)p Fo(>)g FF(family)0 2342 y(of)31 b(functions:)227
+(appropriate)g(mem)m(b)s(er)g(of)g(the)g(astIsA)p Fn(<)p
+FF(Class)p Fn(>)g FF(family)0 2342 y(of)31 b(functions:)227
2558 y Ft(int)43 b(ok;)227 2757 y(...)227 2956 y(ok)g(=)g
(astIsAFrame\()c(object)i(\);)0 3185 y FF(Note,)33 b(ho)m(w)m(ev)m(er,)
f(that)g(this)f(will)g(accept)h(an)m(y)g(F)-8 b(rame,)32
@@ -112003,7 +107724,7 @@ b(alen)m(t)39 b(to)f(the)0 690 y(follo)m(wing)32 b(use)e(of)g(a)h
("")i(\);)227 988 y(\(void\))e(astWrite\()f(channel,)h(object)g(\);)227
1088 y(channel)g(=)i(astAnnul\()d(channel)h(\);)0 1300
y FF(Some)34 b(lines)f(of)h(the)g(output)f(start)h(with)f(a)h(\\)p
-Fq(#)p FF(")g(commen)m(t)h(c)m(haracter,)h(whic)m(h)d(turns)f(the)i
+Fp(#)p FF(")g(commen)m(t)h(c)m(haracter,)h(whic)m(h)d(turns)f(the)i
(rest)g(of)f(the)h(line)0 1413 y(in)m(to)40 b(a)f(commen)m(t.)66
b(These)39 b(lines)g(will)g(b)s(e)f(ignored)g(when)g(read)h(bac)m(k)g
(in)f(b)m(y)h(astRead.)66 b(They)39 b(t)m(ypically)0
@@ -112759,11 +108480,11 @@ Fx(e.g.)g FF(a)g(F)-8 b(rame)28 b(title)i(can)e(b)s(e)f(of)h(arbitrary)
f(length\).)41 b(If)27 b(this)h(o)s(ccurs,)g(the)0 3878
y(long)j(string)g(will)f(b)s(e)g(split)h(o)m(v)m(er)h(t)m(w)m(o)g(or)e
(more)h(header)f(cards.)41 b(Eac)m(h)31 b(\\con)m(tin)m(uation")i(card)
-e(will)g(ha)m(v)m(e)g(the)0 3991 y(k)m(eyw)m(ord)d Fq(CONTINUE)e
+e(will)g(ha)m(v)m(e)g(the)0 3991 y(k)m(eyw)m(ord)d Fp(CONTINUE)e
FF(in)i(columns)f(1)h(to)h(8,)g(and)e(will)i(con)m(tain)g(a)f(space)h
(in)e(column)h(9)g(\(instead)h(of)f(the)g(usual)0 4104
y(equals)h(sign\).)40 b(An)29 b(amp)s(ersand)e(\(\\)p
-Fq(&)p FF("\))i(is)g(app)s(ended)e(to)i(the)g(end)f(of)g(eac)m(h)i(of)f
+Fp(&)p FF("\))i(is)g(app)s(ended)e(to)i(the)g(end)f(of)g(eac)m(h)i(of)f
(the)g(strings)f(\(except)i(the)f(last)0 4217 y(one\))i(to)g(indicate)h
(that)f(the)f(string)g(is)h(con)m(tin)m(ued)g(on)f(the)h(next)f(card.)0
4375 y(Note,)42 b(this)d(splitting)h(of)f(long)g(strings)g(o)m(v)m(er)h
@@ -112880,7 +108601,7 @@ b(Ho)m(w)m(ev)m(er,)27 b(if)d(y)m(ou)g(c)m(hange)227
(duced)g(in)227 1210 y(detail.)111 1392 y(3.)46 b(The)32
b(FITS)g(k)m(eyw)m(ords)g(whic)m(h)h(app)s(ear)e(to)i(the)g(left)g(of)f
(the)h(\\=")g(signs)f(ha)m(v)m(e)i(additional)f(c)m(haracters)227
-1505 y(\(\\)p Fq(_)p FF(A",)27 b(\\)p Fq(_)p FF(B",)f
+1505 y(\(\\)p Fp(_)p FF(A",)27 b(\\)p Fp(_)p FF(B",)f
Fx(etc.)p FF(\))38 b(app)s(ended)24 b(to)h(them.)39 b(This)24
b(is)h(done)g(in)g(order)f(to)i(mak)m(e)g(eac)m(h)g(k)m(eyw)m(ord)f
(unique.)0 1743 y(This)d(last)i(p)s(oin)m(t)f(is)h(w)m(orth)f(further)e
@@ -112962,7 +108683,7 @@ b(Concatenated)h(Cards)f(to)f(a)h(FitsChan)0 1238 y FF(If)f(y)m(ou)h
Fu(x)p FF(16.8)h(should)d(b)s(e)h(read.)0 1961 y(F)-8
b(or)39 b(instance,)j(if)d(y)m(ou)g(are)g(using)f(the)h(CFITSIO)e
(library)h(for)h(access)h(to)f(FITS)f(\014les,)j(y)m(ou)e(can)g(use)f
-(the)0 2074 y(CFITSIO)29 b(\014ts)p Fq(_)p FF(hdr2str)f(function)j(to)g
+(the)0 2074 y(CFITSIO)29 b(\014ts)p Fp(_)p FF(hdr2str)f(function)j(to)g
(obtain)f(a)h(string)g(suitable)f(for)h(passing)f(to)h(astPutCards:)227
2504 y Ft(if\()43 b(!fits_hdr2str\()37 b(fptr,)42 b(0,)h(NULL,)e(0,)i
(&header,)d(&nkeys,)h(&status)g(\))i(\))358 2603 y(fitschan)d(=)j
@@ -113235,7 +108956,7 @@ y(The)48 b(con)m(v)m(en)m(tions)i(used)d(are)h(describ)s(ed)f(in)h(a)g
4753 y(M.)g(Calabretta,)48 b Fx(et.)77 b(al.)p FF(,)47
b(often)d(referred)e(to)i(as)g(the)f(\\FITS-W)m(CS)g(pap)s(ers".)79
b(They)427 4866 y(are)30 b(describ)s(ed)f(at)h(h)m
-(ttp://\014ts.gsfc.nasa.go)m(v/\014ts)p Fq(_)p FF(w)m(cs.h)m(tml.)46
+(ttp://\014ts.gsfc.nasa.go)m(v/\014ts)p Fp(_)p FF(w)m(cs.h)m(tml.)46
b(No)m(w)30 b(that)g(the)g(\014rst)f(t)m(w)m(o)427 4979
y(pap)s(ers)j(in)g(this)g(series)h(ha)m(v)m(e)h(b)s(een)e(agreed,)i
(this)f(enco)s(ding)f(should)g(b)s(e)g(understo)s(o)s(d)e(b)m(y)427
@@ -113261,12 +108982,12 @@ Fv(25)1399 351 y FF(It)e(is)g(emplo)m(y)m(ed)h(b)m(y)f(the)g(IRAF)g
577 y(of)k(the)f(curren)m(t)h(FITS-W)m(CS)f(enco)s(ding.)227
731 y FD(FITS-PC)427 844 y FF(This)j(enco)s(ding)g(is)h(based)f(on)g(a)
h(previous)f(v)m(ersion)g(of)h(the)g(prop)s(osed)e(new)h(FITS)f(W)m(CS)
-427 957 y(standard)26 b(whic)m(h)h(used)f Fq(PCjjjjiii)e
-FF(and)i Fq(CDELTj)f FF(k)m(eyw)m(ords)i(to)g(describ)s(e)g(axis)g
+427 957 y(standard)26 b(whic)m(h)h(used)f Fp(PCjjjjiii)e
+FF(and)i Fp(CDELTj)f FF(k)m(eyw)m(ords)i(to)g(describ)s(e)g(axis)g
(rotation)427 1070 y(and)f(scaling.)41 b(V)-8 b(ersions)26
b(of)h(AST)f(prior)f(to)i(V1.5)h(used)e(this)g(sc)m(heme)h(for)f(the)h
(FITS-W)m(CS)427 1183 y(enco)s(ding.)51 b(As)34 b(of)g(V1.5,)i(FITS-W)m
-(CS)e(uses)f Fq(CDi_j)f FF(k)m(eyw)m(ords)i(instead.)2997
+(CS)e(uses)f Fp(CDi_j)f FF(k)m(eyw)m(ords)i(instead.)2997
1150 y Fv(26)3123 1183 y FF(The)g(FITS-)427 1296 y(PC)j(enco)s(ding)g
(is)g(included)f(in)g(AST)h(V1.5)h(only)f(to)h(allo)m(w)g(FITS-W)m(CS)e
(data)i(created)427 1408 y(with)33 b(previous)f(v)m(ersions)h(to)h(b)s
@@ -113280,7 +109001,7 @@ e(\\Non-)427 1901 y(linear)23 b(Co)s(ordinate)e(Systems)h(in)f(AIPS")h
(tly)g(emplo)m(y)m(ed)h(b)m(y)f(the)h(AIPS)e(data)i(analysis)g(facilit)
m(y)-8 b(,)35 b(so)e(its)f(use)427 2127 y(will)26 b(facilitate)i(data)e
(exc)m(hange)h(with)e(AIPS.)f(This)h(enco)s(ding)g(uses)g
-Fq(CROTAi)e FF(and)i Fq(CDELTi)427 2240 y FF(k)m(eyw)m(ords)31
+Fp(CROTAi)e FF(and)i Fp(CDELTi)427 2240 y FF(k)m(eyw)m(ords)31
b(to)g(describ)s(e)f(axis)h(rotation)g(and)f(scaling.)227
2394 y FD(FITS-AIPS++)427 2507 y FF(Enco)s(des)c(co)s(ordinate)g
(system)g(information)g(in)g(FITS)f(header)h(cards)f(using)h(the)g(con)
@@ -113498,7 +109219,7 @@ h(1:)227 2060 y Ft(AstObject)40 b(*wcsinfo;)227 2260
y(...)227 2459 y(astClear\()g(fitschan,)g("Card")h(\);)227
2559 y(wcsinfo)g(=)i(astRead\()d(fitschan)h(\);)0 2822
y FF(If)30 b(the)h(p)s(oin)m(ter)f(returned)f(b)m(y)i(astRead)g(is)f
-(not)h(equal)g(to)g(AST)p Fq(__)p FF(NULL,)f(then)g(an)g(Ob)5
+(not)h(equal)g(to)g(AST)p Fp(__)p FF(NULL,)f(then)g(an)g(Ob)5
b(ject)31 b(has)f(b)s(een)g(read)0 2935 y(successfully)-8
b(.)41 b(Otherwise,)29 b(there)g(w)m(as)g(either)h(no)f(information)g
(to)g(read)g(or)g(the)g(c)m(hoice)i(of)e(FITS)g(enco)s(ding)0
@@ -113765,7 +109486,7 @@ b(\()g(!astWrite\()d(fitschan,)g(wcsinfo)g(\))j(\))h({)227
(encode)i(\);)358 5445 y(if)i(\()g(!astWrite\()c(fitschan,)h(wcsinfo)h
(\))i(\))g({)p 0 5516 1512 4 v 73 5570 a Fs(29)138 5602
y Fr(Storing)34 b(v)l(alues)f(in)g(the)g(FitsChan)h(for)g(FITS)f
-(headers)h(NAXIS1,)g(NAXIS2,)g Fg(etc.)57 b Fr(\(the)33
+(headers)h(NAXIS1,)g(NAXIS2,)g Ff(etc.)57 b Fr(\(the)33
b(grid)h(dimensions)g(in)f(pixels\),)0 5693 y(b)r(efore)27
b(in)n(v)n(oking)e(astW)-6 b(rite)26 b(can)g(sometimes)h(help)e(to)h
(pro)r(duce)f(a)h(successful)h(write.)p eop end
@@ -113885,14 +109606,14 @@ y(<_attribute)e(name="Lbl1")g(quoted="true")f(value="Axis)h(1")925
TeXDict begin 164 173 bop 0 52 a FF(164)1399 b Fy(18)92
b(STORING)29 b(AST)h(OBJECTS)f(AS)h(XML)g(\(XMLCHAN\))111
351 y FF(2.)46 b(AST)39 b(attributes)h(are)g(describ)s(ed)f(b)m(y)g
-(XML)h(elemen)m(ts)h(with)e(the)h(name)f(\\)p Fq(_)p
+(XML)h(elemen)m(ts)h(with)e(the)h(name)f(\\)p Fp(_)p
FF(attribute".)70 b(Unfortu-)227 464 y(nately)-8 b(,)32
b(the)f(w)m(ord)f(\\attribute")i(is)e(also)i(used)d(b)m(y)h(XML)h(to)g
(refer)f(to)h(a)g(\\name=v)-5 b(alue")32 b(pair)e(within)227
577 y(an)36 b(elemen)m(t)h(start)f(tag.)58 b(So)36 b(for)f(instance,)j
(the)e(\\Title")h(attribute)g(of)e(the)h(AST)f(F)-8 b(rame)37
b(ob)5 b(ject)36 b(is)227 690 y(describ)s(ed)g(within)h(an)f(XML)i
-(elemen)m(t)g(with)f(name)g(\\)p Fq(_)p FF(attribute")h(in)f(whic)m(h)f
+(elemen)m(t)g(with)f(name)g(\\)p Fp(_)p FF(attribute")h(in)f(whic)m(h)f
(the)i(XML)f(attribute)227 803 y(\\name")c(has)e(the)g(v)-5
b(alue)32 b(\\Title",)i(and)c(the)i(XML)g(attribute)g(\\v)-5
b(alue")33 b(has)e(the)g(v)-5 b(alue)32 b(\\1-d)g(co)s(ordi-)227
@@ -113910,7 +109631,7 @@ b(elemen)m(ts)i(are)f(ignored)f(when)g(b)s(eing)227 1740
y(read)i(bac)m(k)g(in)m(to)g(an)f(XmlChan.)111 1926 y(5.)46
b(The)20 b(outer-most)h(XML)g(elemen)m(t)h(of)e(an)g(AST)g(ob)5
b(ject)21 b(will)f(set)h(the)g(default)f(namespace)h(to)g
-Fq(http://www.starlink.ac.uk)o(/ast)o(/xm)o(l/)227 2039
+Fp(http://www.starlink.ac.uk)o(/ast)o(/xm)o(l/)227 2039
y FF(whic)m(h)30 b(will)h(b)s(e)f(inherited)g(b)m(y)g(all)h(nested)g
(elemen)m(ts.)0 2295 y(The)j(XmlChan)g(class)h(c)m(hanges)g(the)g
(default)g(v)-5 b(alue)35 b(for)f(the)h(Commen)m(t)f(and)g(F)-8
@@ -114148,8 +109869,8 @@ FF(171)0 351 y(As)31 b(y)m(ou)g(can)h(see,)g(the)f(function)g(comes)h
b(The)28 b(n)m(um)m(b)s(er)f(of)h(p)s(oin)m(ts)f(to)i(b)s(e)e
(transformed)g(\(\\np)s(oin)m(t"\))i(and)f(the)g(n)m(um)m(b)s(ers)0
577 y(of)36 b(input)e(and)h(output)g(co)s(ordinates)h(p)s(er)e(p)s(oin)
-m(t)i(\(\\nco)s(ord)p Fq(_)p FF(in")f(and)g(\\nco)s(ord)p
-Fq(_)p FF(out"|in)g(this)h(case)g(b)s(oth)0 690 y(are)31
+m(t)i(\(\\nco)s(ord)p Fp(_)p FF(in")f(and)g(\\nco)s(ord)p
+Fp(_)p FF(out"|in)g(this)h(case)g(b)s(oth)0 690 y(are)31
b(assumed)g(equal\))h(are)f(passed)g(to)g(the)h(function.)42
b(A)31 b(pair)g(of)g(lo)s(ops)g(then)g(accesses)h(all)g(the)g(co)s
(ordinate)0 803 y(v)-5 b(alues.)55 b(Note)37 b(that)e(it)h(is)f
@@ -114163,12 +109884,12 @@ b(It)32 b(is)f(also)i(p)s(ermissible)d(to)j(require)e(that)0
(arbitrary)i(dimensionalit)m(y)-8 b(,)32 b(as)e(here.)0
1301 y(Before)e(using)f(an)g(incoming)g(co)s(ordinate,)i(the)e
(function)g(m)m(ust)g(\014rst)f(c)m(hec)m(k)j(that)e(it)h(is)f(not)g
-(set)h(to)g(the)f(v)-5 b(alue)0 1414 y(AST)p Fq(__)p
+(set)h(to)g(the)f(v)-5 b(alue)0 1414 y(AST)p Fp(__)p
FF(BAD,)29 b(whic)m(h)f(indicates)i(missing)e(data)i(\()p
Fu(x)p FF(5.8\).)42 b(If)28 b(it)i(is,)f(the)g(same)g(v)-5
b(alue)29 b(is)g(also)h(assigned)f(to)g(an)m(y)0 1527
y(a\013ected)j(output)e(co)s(ordinates.)41 b(The)30 b(v)-5
-b(alue)31 b(AST)p Fq(__)p FF(BAD)f(is)g(also)i(generated)f(if)f(an)m(y)
+b(alue)31 b(AST)p Fp(__)p FF(BAD)f(is)g(also)i(generated)f(if)f(an)m(y)
h(co)s(ordinates)g(cannot)0 1640 y(b)s(e)k(transformed.)55
b(In)35 b(this)h(example,)h(this)f(can)g(happ)s(en)d(with)j(the)f(in)m
(v)m(erse)i(transformation)f(if)f(negativ)m(e)0 1753
@@ -114199,7 +109920,7 @@ y(Mapping.)0 3023 y(If)42 b(an)f(error)h(o)s(ccurs)g(within)f(a)h
(status)h(to)g(an)g(error)f(v)-5 b(alue)38 b(b)s(efore)f(returning.)62
b(This)37 b(will)h(alert)g(AST)f(to)h(the)0 3249 y(error,)33
b(causing)f(it)h(to)g(ab)s(ort)f(the)g(curren)m(t)g(op)s(eration.)47
-b(The)32 b(error)g(v)-5 b(alue)32 b(AST)p Fq(__)p FF(ITFER)f(is)h(a)m
+b(The)32 b(error)g(v)-5 b(alue)32 b(AST)p Fp(__)p FF(ITFER)f(is)h(a)m
(v)-5 b(ailable)35 b(for)0 3362 y(this)e(purp)s(ose,)f(but)g(other)h(v)
-5 b(alues)34 b(ma)m(y)f(also)h(b)s(e)e(used)g(\()p Fx(e.g.)h
FF(if)g(y)m(ou)g(wish)f(to)i(distinguish)e(di\013eren)m(t)h(t)m(yp)s
@@ -114346,10 +110067,10 @@ m(ert,)k(ho)m(w)m(ev)m(er,)h(w)m(e)43 b(ha)m(v)m(e)h(only)f(implemen)m
(Poly3Tran,)c(AST__NOINV,)794 4601 y(purpose,)h(author,)h(contact)g
(\);)0 4849 y FF(Here,)30 b(the)f(\014fth)f(argumen)m(t)h(has)f(b)s
(een)g(set)i(to)f(the)g(\015ag)g(v)-5 b(alue)30 b(AST)p
-Fq(__)p FF(NOINV)d(to)j(indicate)f(the)g(lac)m(k)i(of)e(an)0
+Fp(__)p FF(NOINV)d(to)j(indicate)f(the)g(lac)m(k)i(of)e(an)0
4962 y(in)m(v)m(erse.)42 b(If)29 b(the)h(forw)m(ard)g(transformation)g
(w)m(ere)h(absen)m(t,)g(w)m(e)f(w)m(ould)g(use)g(AST)p
-Fq(__)p FF(NOF)m(OR)f(instead.)41 b(Flag)0 5075 y(v)-5
+Fp(__)p FF(NOF)m(OR)f(instead.)41 b(Flag)0 5075 y(v)-5
b(alues)31 b(for)f(this)g(argumen)m(t)h(ma)m(y)g(b)s(e)f(com)m(bined)g
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5362 y Fw(20.8)112 b(V)-9 b(ariable)38 b(Num)m(b)s(ers)g(of)g(Co)s
@@ -114368,7 +110089,7 @@ b(ariable)27 b(n)m(um)m(b)s(er)e(of)i(co)s(ordinates)h(\(as)f(with)0
b(e)32 b(indicate)f(the)g(acceptabilit)m(y)j(of)d(a)g(v)-5
b(ariable)31 b(n)m(um)m(b)s(er)f(when)f(registering)j(the)0
577 y(transformation)40 b(function)g(b)m(y)f(supplying)g(the)h(v)-5
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+b(alue)40 b(AST)p Fp(__)p FF(ANY)f(for)h(the)g(n)m(um)m(b)s(er)f(of)h
(input)f(and/or)0 690 y(output)30 b(co)s(ordinates,)h(as)g(follo)m(ws:)
227 943 y Ft(astIntraReg\()39 b("SqrTran",)g(AST__ANY,)h(AST__ANY,)g
(SqrTran,)g(0,)794 1043 y(purpose,)g(author,)h(contact)g(\);)0
@@ -114528,13 +110249,13 @@ b(w)m(e)h(migh)m(t)g(use:)227 2421 y Ft(void)42 b(MaxTran\()e
(double)f(*[])h(\);)227 2620 y(...)227 2820 y(astIntraReg\()d
("MaxTran",)g(AST__ANY,)h(1,)j(MaxTran,)d(AST__SIMPIF,)794
2919 y(purpose,)g(author,)h(contact)g(\);)0 3159 y FF(Here,)30
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+b(the)f(\015ag)g(v)-5 b(alue)30 b(AST)p Fp(__)p FF(SIMPIF)d(supplied)g
(for)i(the)g(\014fth)f(argumen)m(t)h(indicates)h(that)g
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b(o)32 b(indicate)g(the)g(complemen)m(tary)g(case,)h(the)e(\015ag)h
-(AST)p Fq(__)p FF(SIMPFI)e(w)m(ould)h(b)s(e)f(used)h(instead.)0
+(AST)p Fp(__)p FF(SIMPFI)e(w)m(ould)h(b)s(e)f(used)h(instead.)0
3498 y(If)h(b)s(oth)g(simpli\014cations)h(are)f(p)s(ossible)g(\(as)h
(with)f(the)h(SqrT)-8 b(ran)31 b(function)h(in)g Fu(x)p
FF(20.4\),)k(then)c(w)m(e)h(w)m(ould)f(use)0 3611 y(the)f(bit)m(wise)g
@@ -114567,9 +110288,9 @@ Fu(x)p FF(15.3\),)47 b(the)0 5443 y(transformation)31
b(function)f(whic)m(h)h(it)g(uses)f(is)h(not)g(stored)g(with)f(it.)43
b(T)-8 b(o)31 b(do)f(so)h(is)g(imp)s(ossible,)g(b)s(ecause)f(the)p
0 5516 1512 4 v 73 5570 a Fs(32)138 5602 y Fr(Remem)n(b)r(er)18
-b(that)h(\\ptr)p Ff(_)p Fr(in")g(iden)n(ti\014es)f(the)g(original)i
+b(that)h(\\ptr)p Fq(_)p Fr(in")g(iden)n(ti\014es)f(the)g(original)i
(\\output")f(co)r(ordinates)h(when)e(applying)g(the)g(in)n(v)n(erse)h
-(transformation)0 5693 y(and)25 b(\\ptr)p Ff(_)p Fr(out")h(iden)n
+(transformation)0 5693 y(and)25 b(\\ptr)p Fq(_)p Fr(out")h(iden)n
(ti\014es)g(the)f(original)j(\\input")d(co)r(ordinates.)p
eop end
%%Page: 177 187
@@ -114739,7 +110460,7 @@ b(This)33 b(is)0 4779 y(p)s(erformed)h(b)m(y)h(astMark,)j(whic)m(h)e
y Fr(Lik)n(e)28 b(an)n(y)g(F)-6 b(rameSet,)29 b(a)g(Plot)g(can)f(b)r(e)
h(used)f(as)g(a)h(Mapping.)43 b(In)28 b(this)g(case)h(it)g(is)f(the)g
(in)n(v)n(erse)h(transformation)h(whic)n(h)e(is)0 5693
-y(used)d(when)h(plotting)g(\()p Fg(i.e.)e Fr(that)i(whic)n(h)f
+y(used)d(when)h(plotting)g(\()p Ff(i.e.)e Fr(that)i(whic)n(h)f
(transforms)j(b)r(et)n(w)n(een)d(the)g(curren)n(t)g(and)h(base)g(F)-6
b(rames\).)p eop end
%%Page: 180 190
@@ -114905,7 +110626,7 @@ b(within)f(the)h(Plot)g(to)g(whic)m(h)f(clipping)h(is)f(to)h(b)s(e)0
b(rame)29 b(\(NAXES)f(is)0 2340 y(the)j(n)m(um)m(b)s(er)e(of)h(axes)h
(in)f(this)g(F)-8 b(rame\).)0 2501 y(Y)g(ou)31 b(can)g(remo)m(v)m(e)g
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+Fp(__)p FF(NOFRAME)g(for)g(\\iframe".)0 2790 y Fw(21.7)112
b(Using)38 b(a)g(Plot)f(as)h(a)g(Mapping)0 3009 y FF(All)e(Plots)g(are)
g(also)h(Mappings)e(\(just)g(lik)m(e)i(the)f(F)-8 b(rameSets)36
b(from)f(whic)m(h)h(they)f(are)h(deriv)m(ed\),)i(so)d(can)h(b)s(e)0
@@ -114939,7 +110660,7 @@ h(b)s(e)f(applied)g(b)m(y)g(a)h(Plot)g(\(if)f(it)h(has)f(b)s(een)g
b(p)s(oin)m(t)f(whic)m(h)g(lies)i(within)d(the)i(clipp)s(ed)f(region)h
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b(co)s(ordinates)g(with)f(the)h(v)-5 b(alue)41 b(AST)p
-Fq(__)p FF(BAD.)f(If)g(y)m(ou)h(wish)f(to)h(a)m(v)m(oid)h(this)e
+Fp(__)p FF(BAD.)f(If)g(y)m(ou)h(wish)f(to)h(a)m(v)m(oid)h(this)e
(clipping,)k(y)m(ou)c(should)0 4845 y(extract)31 b(the)e(relev)-5
b(an)m(t)31 b(Mapping)e(from)g(the)g(Plot)h(\(using)f(astGetMapping\))i
(and)e(use)g(this,)g(instead)h(of)f(the)0 4958 y(Plot,)i(to)h
@@ -114980,7 +110701,7 @@ b(alid)28 b(co)s(ordinates,)i(irresp)s(ectiv)m(e)f(of)g(an)m(y)f
(clipping)h(b)s(eing)f(applied)0 1785 y(\()p Fu(x)p FF(21.6\).)60
b(T)-8 b(o)37 b(indicate)g(this,)g(the)f(resulting)g(co)s(ordinate)h(v)
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+b(alue)37 b(AST)p Fp(__)p FF(BAD)0 1898 y(\()p Fu(x)p
FF(5.8\).)0 2075 y(There)g(are)h(a)g(n)m(um)m(b)s(er)f(of)h(reasons)f
(wh)m(y)h(this)f(ma)m(y)i(o)s(ccur,)g(but)e(t)m(ypically)j(it)e(will)g
(b)s(e)f(b)s(ecause)h(ph)m(ysical)0 2188 y(co)s(ordinates)22
@@ -115113,8 +110834,8 @@ f(to)i(c)m(hange,)h(colour,)g(fon)m(t,)g(size,)f(width,)g(to)0
b(the)g(en)m(try)g(for)f(the)h(Escap)s(e)g(attribute)0
690 y(in)30 b(App)s(endix)f(C)h(for)g(details.)0 855
y(As)j(an)f(example,)i(if)f(the)g(c)m(haracter)h(string)e(\\)p
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-(displa)m(y)m(ed)h(as)0 968 y(\\10)135 935 y Fv(0)p Fh(:)p
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+(displa)m(y)m(ed)h(as)0 968 y(\\10)135 935 y Fv(0)p Fg(:)p
Fv(5)231 968 y FF(")f(-)h(that)f(is,)h(with)f(a)g(sup)s(er-scripted)f
(exp)s(onen)m(t.)46 b(The)32 b(exp)s(onen)m(t)g(text)h(will)g(b)s(e)e
(70\045)i(of)f(the)g(size)h(of)0 1081 y(normal)d(text)g(\(as)g
@@ -115137,7 +110858,7 @@ FF(\).)0 2028 y(Note,)46 b(the)c(facilit)m(y)i(for)e(in)m(terpreting)g
b(if)c(the)h(graphics)g(wrapp)s(er)0 2141 y(functions)24
b(whic)m(h)f(pro)m(vide)h(the)g(in)m(terface)i(to)f(the)f(underlying)f
(graphics)h(system)g(supp)s(ort)e(all)j(the)f(functions)0
-2254 y(included)k(in)h(the)h Fq(grf.h)d FF(\014le)i(as)h(of)f(AST)g
+2254 y(included)k(in)h(the)h Fp(grf.h)d FF(\014le)i(as)h(of)f(AST)g
(V3.2.)41 b(Older)29 b(grf)g(in)m(terfaces)h(ma)m(y)g(need)f(to)h(b)s
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(b)s(efore)g(escap)s(e)h(sequences)f(can)h(b)s(e)f(in)m(terpretted.)0
@@ -115245,9 +110966,9 @@ e(indicating)h(whic)m(h)f(wrapp)s(er)f(functions)h(are)h(to)g(b)s(e)f
b(A)33 b(\014le)g(con)m(taining)i(C)d(functions)h(with)f(pre-de\014ned)
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3335 y(application)42 b(using)e(options)h(of)g(the)g(ast)p
-Fq(_)p FF(link)f(command.)71 b(\(see)42 b Fu(x)p FF(3.3)g(and)e(App)s
+Fp(_)p FF(link)f(command.)71 b(\(see)42 b Fu(x)p FF(3.3)g(and)e(App)s
(endix)f(E\).)71 b(AST)227 3448 y(is)37 b(distributed)f(with)g(suc)m(h)
-h(a)g(\014le)f(\(called)j Fq(grf_pgplot.c)p FF(\))33
+h(a)g(\014le)f(\(called)j Fp(grf_pgplot.c)p FF(\))33
b(whic)m(h)k(calls)h(PGPLOT)d(functions)i(to)227 3561
y(implemen)m(t)30 b(the)f(required)g(functionalit)m(y)-8
b(.)42 b(This)28 b(\014le)i(can)f(b)s(e)g(used)f(as)h(a)h(template)g
@@ -115261,7 +110982,7 @@ g(w)m(a)m(y)g(do)g(not)g(need)g(to)g(ha)m(v)m(e)h(the)g(pre-de\014ned)d
(names)i(used)f(in)g(the)227 4200 y(link-time)32 b(metho)s(d)d(describ)
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m(terfaces)i(of)f(the)f(wrapp)s(er)f(routines,)i(see)g(either)f(the)h
-Fq(grf_pgplot.c)c FF(\014le)j(included)0 4550 y(in)e(the)h(AST)e
+Fp(grf_pgplot.c)c FF(\014le)j(included)0 4550 y(in)e(the)h(AST)e
(source)i(distribution,)f(or)g(the)h(reference)g(do)s(cumen)m(tation)g
(for)f(the)g(astGrfSet)h(metho)s(d.)p eop end
%%Page: 187 197
@@ -115288,16 +111009,16 @@ h(usual)f(compiler)h(options)0 1678 y(for)d(\014nding)f(C)h(include)g
b(with)e(AST)h(F)-9 b(acilities)0 2690 y FF(C)40 b(programs)f(whic)m(h)
h(use)g(AST)f(facilities)k(ma)m(y)d(b)s(e)g(link)m(ed)g(b)m(y)g
(including)g(execution)h(of)f(the)h(command)0 2803 y(\\ast)p
-Fq(_)p FF(link")33 b(on)f(the)g(compiler)h(command)e(line.)46
+Fp(_)p FF(link")33 b(on)f(the)g(compiler)h(command)e(line.)46
b(Th)m(us,)31 b(to)i(compile)g(and)e(link)h(a)h(program)e(called)i
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3416 y FF(Note)27 b(the)f(use)g(of)g(bac)m(kw)m(ard)g(quote)h(c)m
-(haracters,)i(whic)m(h)c(cause)i(the)f(\\ast)p Fq(_)p
+(haracters,)i(whic)m(h)c(cause)i(the)f(\\ast)p Fp(_)p
FF(link")h(command)f(to)g(b)s(e)g(executed)0 3529 y(and)g(its)h(result)
g(substituted)f(in)m(to)i(the)e(compiler)i(command.)39
b(An)26 b(alternativ)m(e)j(is)e(to)g(sa)m(v)m(e)i(the)e(output)f(from)0
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+3642 y(\\ast)p Fp(_)p FF(link")32 b(in)f(\(sa)m(y\))i(a)e(shell)h(v)-5
b(ariable)31 b(and)g(use)g(this)g(instead.)43 b(Y)-8
b(ou)32 b(ma)m(y)f(\014nd)f(this)h(a)h(little)h(faster)e(if)g(y)m(ou)0
3755 y(are)g(building)e(soft)m(w)m(are)j(rep)s(eatedly)f(during)e(dev)m
@@ -115310,23 +111031,23 @@ e(ha)m(v)m(e)i(used)d(the)h(default)g(metho)s(d)g(whic)m(h)g(assumes)0
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-(applied)g(to)h(the)f(\\ast)p Fq(_)p FF(link")0 4368
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(k)-5 b(age,)31 b(y)m(ou)0 4642 y(could)e(link)g(with)g(the)g
(AST/PGPLOT)f(in)m(terface)j(b)m(y)d(using)h(the)g(\\)p
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a Fs(36)138 5419 y Fr(If)33 b(y)n(ou)g(ha)n(v)n(e)f(not)h(installed)h
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-y Fr(Use)20 b(the)f(\\)p Fm(\000)p Fr(pgp")g(option)h(instead)g(if)g(y)
+y Fr(Use)20 b(the)f(\\)p Fl(\000)p Fr(pgp")g(option)h(instead)g(if)g(y)
n(ou)f(wish)h(to)f(use)h(the)f(Starlink)g(v)n(ersion)g(of)i(PGPLOT)f
(whic)n(h)f(uses)h(GKS)f(to)h(generate)0 5693 y(its)26
b(output.)p eop end
@@ -115340,7 +111061,7 @@ b(of)h(Starlink's)g(AD)m(AM)h(programming)e(en)m(vironmen)m(t)h
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799 y(cluding)30 b(execution)i(of)e(the)h(command)f(\\ast)p
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(follo)m(ws:)227 1048 y Ft(alink)42 b(adamprog.c)d(`ast_link_adam`)0
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(haracters.)0 1473 y(By)e(default,)g(AST)f(error)g(messages)i(pro)s
@@ -115350,12 +111071,12 @@ Fq(_)p FF(link)p Fq(_)p FF(adam")h(on)g(the)f(command)g(line,)h(as)g
(b)m(y)g(AST)g(is)h(consisten)m(t)0 1698 y(with)c(the)h
Fx(inherite)-5 b(d)33 b(status)f FF(error)e(handling)g(normally)g(used)
g(in)g(Starlink)g(soft)m(w)m(are.)0 1861 y(Switc)m(hes)43
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b(in)d(order)h(to)g(link)g(with)f(additional)i(AST-related)f
(facilities,)j(suc)m(h)c(as)h(a)g(graphics)g(in)m(terface.)52
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+b(See)0 2087 y(the)31 b(\\ast)p Fp(_)p FF(link)p Fp(_)p
FF(adam")g(command)f(description)h(in)f(App)s(endix)e(E)j(for)f
(details)h(of)g(the)f(options)h(a)m(v)-5 b(ailable.)p
eop end
@@ -115451,84 +111172,84 @@ TeXDict begin 191 200 bop 3643 52 a FF(191)0 351 y Fz(B)134
b(AST)44 b(F)-11 b(unction)44 b(Descriptions)p 0 578
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%%Page: 215 225
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%%Page: 229 239
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%%Page: 230 240
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(matc)n(h)g(another)f(F)-7 b(rame)25 b(whic)n(h)h(b)r(elongs)f(to)h
(the)h(same)e(class)g(as)g(the)427 2240 y(template,)35
b(or)d(to)h(a)f(deriv)n(ed)g(\(more)g(sp)r(ecialised\))h(class.)52
@@ -118671,7 +114392,7 @@ b(F)-7 b(or)32 b(example,)i(a)e(SkyF)-7 b(rame)32 b(template)h(will)427
b(but)h(will)f(not)g(matc)n(h)f(a)g(basic)h(F)-7 b(rame.)54
b(Con)n(v)n(ersely)-7 b(,)34 b(a)f(basic)g(F)-7 b(rame)427
2439 y(template)28 b(will)g(matc)n(h)f(an)n(y)g(class)g(of)g(F)-7
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f(that)h(a)e(F)-7 b(rame)25 b(of)g(an)n(y)g(class)f(can)h(b)r(e)g(used)
g(to)g(matc)n(h)g(a)g(CmpF)-7 b(rame,)26 b(if)f(that)427
2671 y(CmpF)-7 b(rame)27 b(con)n(tains)e(a)h(F)-7 b(rame)26
@@ -118684,7 +114405,7 @@ b(ho)n(w)n(ev)n(er,)d(the)j(MaxAxes)427 2771 y(and)j(MinAxes)h
n(um)n(b)r(er)g(of)427 2970 y(axes)g(in)i(the)f(target,)g(and)f(the)i
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(to)h(the)h(n)n(um)n(b)r(er)427 3070 y(of)f(axes)e(in)i(the)g(target.)
-340 3203 y Fi(\017)45 b Fj(If)40 b(using)g(a)f(CmpF)-7
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b(rame)40 b(as)f(a)g(template)h(frame,)i(the)f(MinAxes)e(and)h(MaxAxes)
f(for)g(the)h(template)427 3302 y(are)33 b(determined)g(b)n(y)h(the)f
(MinAxes)h(and)f(MaxAxes)g(v)-5 b(alues)33 b(of)g(the)h(comp)r(onen)n
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(MinAxes)i(attributes)g(in)g(the)h(comp)r(onen)n(t)427
3601 y(template)28 b(F)-7 b(rames,)27 b(b)r(efore)g(com)n(bining)g
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3834 y(whic)n(h)23 b(ha)n(v)n(e)e(an)h(iden)n(tical)g(v)-5
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b(the)g(Domain)427 4564 y(attribute)j(of)g(the)h(template)f(has)f(the)i
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(restricting)f(the)h(searc)n(h)e(in)i(the)h(same)e(manner,)427
4963 y(but)30 b(is)e(a)h(more)f(con)n(v)n(enien)n(t)f(in)n(terface)h
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g(matc)n(h)g(a)g(F)-7 b(rame)29 b(whic)n(h)g(has)g(the)g(same)g(n)n(um)
n(b)r(er)g(of)g(axes)f(as)h(itself.)427 5295 y(Ho)n(w)n(ev)n(er,)i(for)
g(some)g(classes)f(of)h(template,)i(this)f(default)f(b)r(eha)n(viour)g
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(eci\014ed)h(in)p eop end
%%Page: 233 243
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12 v 0 779 a Fz(astFitsChan)707 b Fe(Create)37 b(a)h(FitsChan)705
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b(An)n(y)30 b(sequence)f(of)h(FITS-conforming)e(header)h(cards)227
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(FitsChan,)j(y)n(ou)d(ha)n(v)n(e)g(the)h(option)f(of)h(sp)r(ecifying)g
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@@ -118812,8 +114533,8 @@ g(cards)g(to)h(an)g(external)f(data)h(store\).)46 b(If)227
y(astFindFits)28 b(or)f(astRead\).)227 3528 y(Co)r(ordinate)i(system)g
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b(is)f(written)h(to)g(\(or)f(read)g(from\))h(a)f(FitsChan,)227
3728 y(the)22 b(v)-5 b(alue)22 b(of)g(the)g(FitsChan's)g(Enco)r(ding)f
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@@ -118864,12 +114585,12 @@ b(\(e.g.)67 b(the)39 b(NA)-7 b(TIVE)38 b(enco)r(ding\),)227
%%Page: 234 244
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%%Page: 243 253
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eop end
%%Page: 266 276
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%%Page: 274 284
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@@ -123693,24 +119414,24 @@ g(the)g(MatrixMap)f(is)g(created\))g(to)h(giv)n(e)e(a)i(new)f(column-v)
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%%Page: 297 307
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@@ -123765,24 +119486,24 @@ g(the)g(matrix)f(is)g(not)h(square,)f(one)g(or)g(more)f(of)i(the)g
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eop end
%%Page: 298 308
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end
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%%Page: 322 332
@@ -125747,7 +121468,7 @@ b(AST)30 b(FUNCTION)g(DESCRIPTIONS)p 0 351 3780 12 v
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%%Page: 323 333
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eop end
%%Page: 324 334
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eop end
%%Page: 325 335
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@@ -126667,9 +122388,9 @@ g(features)h(in)g(the)h(data)e(b)n(y)h(smo)r(othing)g(them,)i(and)e
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%%Page: 339 349
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%%Page: 342 352
@@ -127511,14 +123232,14 @@ b(AST)30 b(FUNCTION)g(DESCRIPTIONS)p 0 351 3780 12 v
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%%Page: 343 353
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%%Page: 367 377
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-(Applicabilit)m(y:)259 1509 y(Region)427 1609 y Fj(All)d(Regions)f(ha)n
+1207 y Fi(In)n(teger)g(\(b)r(o)r(olean\).)0 1365 y Fd(Class)k
+(Applicabilit)m(y:)259 1509 y(Region)427 1609 y Fi(All)d(Regions)f(ha)n
(v)n(e)f(this)i(attribute.)p 0 1817 3780 12 v 0 1948
a Fz(AlignO\013set)383 b Fe(Align)37 b(SkyF)-10 b(rames)38
b(using)h(the)f(o\013set)1400 2063 y(co)s(ordinate)e(system?)3115
1948 y Fz(AlignO\013set)0 2260 y Fd(Description:)44 b
-Fj(This)26 b(attribute)g(is)g(a)g(b)r(o)r(olean)f(v)-5
+Fi(This)26 b(attribute)g(is)g(a)g(b)r(o)r(olean)f(v)-5
b(alue)26 b(whic)n(h)g(con)n(trols)e(ho)n(w)i(a)f(SkyF)-7
b(rame)25 b(b)r(eha)n(v)n(es)g(when)h(it)h(is)f(used)227
2360 y(\(b)n(y)c(astFindF)-7 b(rame)22 b(or)e(astCon)n(v)n(ert\))h(as)g
@@ -133725,8 +129446,8 @@ b(are)f(aligned)h(if)h(a)g(matc)n(h)f(o)r(ccurs.)227
2588 y(If)21 b(the)g(template)g(and)f(target)g(SkyF)-7
b(rames)19 b(b)r(oth)i(ha)n(v)n(e)e(de\014ned)i(o\013set)g(co)r
(ordinate)e(systems)h(\(i.e.)35 b(the)21 b(SkyRefIs)227
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+2688 y(attribute)j(is)g(set)f(to)h(either)f Ft(")p Fi(Origin)p
+Ft(")f Fi(or)h Ft(")g Fi(P)n(ole)p Ft(")p Fi(\),)g(and)g(they)h(b)r
(oth)g(ha)n(v)n(e)f(a)g(non-zero)f(v)-5 b(alue)23 b(for)h
(AlignO\013set,)227 2788 y(then)h(alignmen)n(t)e(o)r(ccurs)g(within)h
(the)g(o\013set)g(co)r(ordinate)f(systems)g(\(that)h(is,)h(a)e(UnitMap)
@@ -133734,19 +129455,19 @@ i(will)f(alw)n(a)n(ys)d(b)r(e)k(used)227 2887 y(to)e(align)f(the)g(t)n
(w)n(o)g(SkyF)-7 b(rames\).)35 b(If)23 b(either)f(the)h(template)g(or)e
(target)h(SkyF)-7 b(rame)22 b(has)g(zero)f(\(the)i(default)g(v)-5
b(alue\))227 2987 y(for)35 b(AlignO\013set,)j(or)d(if)h(either)f(SkyF)
--7 b(rame)35 b(has)g(SkyRefIs)h(set)g(to)f Ft(")p Fj(Ignored)p
-Ft(")p Fj(,)h(then)g(alignmen)n(t)f(o)r(ccurring)227
+-7 b(rame)35 b(has)g(SkyRefIs)h(set)g(to)f Ft(")p Fi(Ignored)p
+Ft(")p Fi(,)h(then)g(alignmen)n(t)f(o)r(ccurring)227
3087 y(within)29 b(the)f(co)r(ordinate)e(system)h(sp)r(eci\014ed)h(b)n
(y)f(the)h(AlignSystem)g(attribute.)0 3244 y Fd(T)m(yp)s(e:)227
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+3344 y Fi(In)n(teger)f(\(b)r(o)r(olean\).)0 3502 y Fd(Class)k
(Applicabilit)m(y:)259 3647 y(SkyF)-8 b(rame)427 3747
-y Fj(All)28 b(SkyF)-7 b(rames)27 b(ha)n(v)n(e)f(this)i(attribute.)p
+y Fi(All)28 b(SkyF)-7 b(rames)27 b(ha)n(v)n(e)f(this)i(attribute.)p
0 3954 V 0 4086 a Fz(AlignSideBand)227 b Fe(Should)38
b(the)g(SideBand)h(attribute)1183 4186 y(b)s(e)g(tak)m(en)f(in)m(to)f
(accoun)m(t)g(when)1157 4285 y(aligning)f(this)j(DSBSp)s(ecF)-10
b(rame)1117 4400 y(with)37 b(another)h(DSBSp)s(ecF)-10
b(rame?)2903 4086 y Fz(AlignSideBand)0 4597 y Fd(Description:)44
-b Fj(This)28 b(attribute)g(con)n(trols)e(ho)n(w)h(a)g(DSBSp)r(ecF)-7
+b Fi(This)28 b(attribute)g(con)n(trols)e(ho)n(w)h(a)g(DSBSp)r(ecF)-7
b(rame)27 b(b)r(eha)n(v)n(es)g(when)h(an)f(attempt)h(is)f(made)h(to)f
(align)227 4697 y(it)i(with)g(another)f(DSBSp)r(ecF)-7
b(rame)28 b(using)g(astFindF)-7 b(rame)28 b(or)g(astCon)n(v)n(ert.)38
@@ -133777,7 +129498,7 @@ b(rame,)24 b(ev)n(en)e(though)h(those)g(frequencies)f(refer)g(to)h
b(alue)28 b(for)f(AlignSideBand)g(is)h(zero.)p eop end
%%Page: 417 427
TeXDict begin 417 426 bop 3643 52 a FF(417)227 351 y
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+Fi(When)23 b(astFindF)-7 b(rame)22 b(or)g(astCon)n(v)n(ert)e(is)i(used)
h(on)f(t)n(w)n(o)f(DSBSp)r(ecF)-7 b(rames)23 b(\(p)r(oten)n(tially)f
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(systems)g(and/or)f(sidebands\),)k(it)e(returns)f(a)g(Mapping)g(whic)n
@@ -133786,7 +129507,7 @@ b(p)r(osition)f(in)i(one)e(DSBSp)r(ecF)-7 b(rame)34 b(in)n(to)g(the)g
(corresp)r(onding)e(p)r(osition)i(in)g(the)g(other.)55
b(The)34 b(Mapping)g(is)227 650 y(made)28 b(up)g(of)f(the)h(follo)n
(wing)f(steps)g(in)h(the)g(indicated)g(order:)340 908
-y Fi(\017)45 b Fj(If)28 b(b)r(oth)g(DSBSp)r(ecF)-7 b(rames)27
+y Fh(\017)45 b Fi(If)28 b(b)r(oth)g(DSBSp)r(ecF)-7 b(rames)27
b(ha)n(v)n(e)f(a)h(v)-5 b(alue)28 b(of)f(1)g(for)g(the)h(AlignSideBand)
f(attribute,)h(map)f(v)-5 b(alues)27 b(from)427 1007
y(the)39 b(target's)f(curren)n(t)g(sideband)g(\(giv)n(en)g(b)n(y)h(its)
@@ -133797,13 +129518,13 @@ g(SideBand)f(attribute\))h(to)g(the)g(observ)n(ed)e(sideband)427
b(If)28 b(either)h(of)f(the)h(t)n(w)n(o)e(DSBSp)r(ecF)-7
b(rames)29 b(ha)n(v)n(e)e(a)h(v)-5 b(alue)28 b(of)g(zero)g(for)f(its)
427 1306 y(AlignSideBand)h(attribute,)g(then)g(this)g(step)f(is)h
-(omitted.)340 1437 y Fi(\017)45 b Fj(Map)25 b(the)g(v)-5
+(omitted.)340 1437 y Fh(\017)45 b Fi(Map)25 b(the)g(v)-5
b(alues)24 b(from)g(the)h(sp)r(ectral)f(system)g(of)h(the)g(target)e
(to)i(the)g(sp)r(ectral)e(system)i(of)f(the)h(template.)427
1536 y(This)39 b(Mapping)g(tak)n(es)f(in)n(to)h(accoun)n(t)f(all)h(the)
g(inherited)g(Sp)r(ecF)-7 b(rame)39 b(attributes)g(suc)n(h)g(as)f
(System,)427 1636 y(StdOfRest,)29 b(Unit,)f(etc.)340
-1767 y Fi(\017)45 b Fj(If)28 b(b)r(oth)g(DSBSp)r(ecF)-7
+1767 y Fh(\017)45 b Fi(If)28 b(b)r(oth)g(DSBSp)r(ecF)-7
b(rames)27 b(ha)n(v)n(e)f(a)h(v)-5 b(alue)28 b(of)f(1)g(for)g(the)h
(AlignSideBand)f(attribute,)h(map)f(v)-5 b(alues)27 b(from)427
1866 y(the)37 b(result's)f(observ)n(ed)e(sideband)j(to)f(the)g
@@ -133814,14 +129535,14 @@ f(represen)n(ts)f(the)i(observ)n(ed)f(sideband,)h(this)h(step)f(will)g
b(If)31 b(either)f(of)g(the)g(t)n(w)n(o)g(DSBSp)r(ecF)-7
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+(omitted.)0 2325 y Fd(T)m(yp)s(e:)227 2424 y Fi(In)n(teger)g(\(b)r(o)r
(olean\).)0 2571 y Fd(Class)k(Applicabilit)m(y:)259 2706
-y(DSBSp)s(ecF)-8 b(rame)427 2805 y Fj(All)28 b(DSBSp)r(ecF)-7
+y(DSBSp)s(ecF)-8 b(rame)427 2805 y Fi(All)28 b(DSBSp)r(ecF)-7
b(rames)28 b(ha)n(v)n(e)e(this)i(attribute.)p 0 3000
3780 12 v 0 3132 a Fz(AlignSp)t(ecO\013set)238 b Fe(Align)38
b(Sp)s(ecF)-10 b(rames)38 b(using)h(the)1245 3246 y(o\013set)g(co)s
(ordinate)d(system?)2841 3132 y Fz(AlignSp)t(ecO\013set)0
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+3430 y Fd(Description:)44 b Fi(This)37 b(attribute)g(is)g(a)g(b)r(o)r
(olean)f(v)-5 b(alue)37 b(whic)n(h)g(con)n(trols)e(ho)n(w)h(a)h(Sp)r
(ecF)-7 b(rame)36 b(b)r(eha)n(v)n(es)g(when)h(it)h(is)227
3530 y(used)e(\(b)n(y)g(astFindF)-7 b(rame)36 b(or)f(astCon)n(v)n
@@ -133841,13 +129562,13 @@ y(in)j(the)g(Sp)r(ecF)-7 b(rames)30 b(b)r(eing)h(aligned)e(so)h(that)h
(a)f(giv)n(en)g(o\013set)g(v)-5 b(alue)30 b(in)h(one)f(is)h(mapp)r(ed)g
(to)f(the)h(same)f(o\013set)227 4152 y(v)-5 b(alue)28
b(in)g(the)g(other.)0 4299 y Fd(T)m(yp)s(e:)227 4398
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-(y:)259 4680 y(Sp)s(ecF)-8 b(rame)427 4779 y Fj(All)28
+y Fi(In)n(teger)f(\(b)r(o)r(olean\).)0 4545 y Fd(Class)k(Applicabilit)m
+(y:)259 4680 y(Sp)s(ecF)-8 b(rame)427 4779 y Fi(All)28
b(Sp)r(ecF)-7 b(rames)27 b(ha)n(v)n(e)g(this)h(attribute.)p
0 4974 V 0 5106 a Fz(AlignStdOfRest)221 b Fe(Standard)38
b(of)g(rest)g(to)g(use)i(when)1367 5205 y(aligning)c(Sp)s(ecF)-10
b(rames)2850 5106 y Fz(AlignStdOfRest)0 5394 y Fd(Description:)44
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+b Fi(This)34 b(attribute)f(con)n(trols)f(ho)n(w)h(a)f(Sp)r(ecF)-7
b(rame)34 b(b)r(eha)n(v)n(es)e(when)h(it)h(is)f(used)g(\(b)n(y)h
(astFindF)-7 b(rame)32 b(or)227 5494 y(astCon)n(v)n(ert\))26
b(as)h(a)g(template)h(to)g(matc)n(h)f(another)g(\(target\))g(Sp)r(ecF)
@@ -133856,12 +129577,12 @@ b(as)h(a)g(template)h(to)g(matc)n(h)f(another)g(\(target\))g(Sp)r(ecF)
b(See)32 b(the)f(StdOfRest)h(attribute)g(for)e(a)h(desription)g(of)g
(the)h(v)-5 b(alues)31 b(whic)n(h)227 5693 y(ma)n(y)c(b)r(e)h(assigned)
f(to)g(this)h(attribute.)37 b(The)28 b(default)g(AlignStdOfRest)g(v)-5
-b(alue)27 b(is)h Ft(")p Fj(Helio)p Ft(")f Fj(\(heliographic\).)p
+b(alue)27 b(is)h Ft(")p Fi(Helio)p Ft(")f Fi(\(heliographic\).)p
eop end
%%Page: 418 428
TeXDict begin 418 427 bop 0 52 a FF(418)1994 b Fy(C)91
b(AST)29 b(A)-8 b(TTRIBUTE)31 b(DESCRIPTIONS)227 351
-y Fj(When)38 b(astFindF)-7 b(rame)38 b(or)e(astCon)n(v)n(ert)g(is)i
+y Fi(When)38 b(astFindF)-7 b(rame)38 b(or)e(astCon)n(v)n(ert)g(is)i
(used)f(on)h(t)n(w)n(o)f(Sp)r(ecF)-7 b(rames)37 b(\(p)r(oten)n(tially)h
(describing)e(di\013eren)n(t)227 451 y(sp)r(ectral)31
b(co)r(ordinate)e(systems\),)j(it)f(returns)g(a)f(Mapping)h(whic)n(h)g
@@ -133869,36 +129590,36 @@ b(co)r(ordinate)e(systems\),)j(it)f(returns)g(a)f(Mapping)h(whic)n(h)g
551 y(one)38 b(Sp)r(ecF)-7 b(rame)37 b(in)n(to)h(the)g(corresp)r
(onding)e(p)r(osition)h(in)h(the)g(other.)67 b(The)38
b(Mapping)f(is)h(made)f(up)i(of)e(the)227 650 y(follo)n(wing)27
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-b Fj(Map)33 b(v)-5 b(alues)33 b(from)g(the)h(system)f(used)g(b)n(y)g
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(the)h(target)e(\(w)n(a)n(v)n(elength,)i(apparen)n(t)e(radial)g(v)n
(elo)r(cit)n(y)-7 b(,)34 b(etc\))427 1009 y(to)k(the)g(system)f(sp)r
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(target's)f(rest)g(frequency)g(if)427 1109 y(necessary)-7
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b(alues)30 b(from)g(the)h(target's)e(standard)g(of)i(rest)f(to)g(the)h
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1340 y(AlignStdOfRest)35 b(attribute,)h(using)e(the)h(Ep)r(o)r(c)n(h,)g
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f(sp)r(eci\014ed)g(b)n(y)g(the)h(AlignSystem)f(attribute,)h(to)f(the)h
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+2162 y Fd(T)m(yp)s(e:)227 2262 y Fi(String.)0 2410 y
Fd(Class)31 b(Applicabilit)m(y:)259 2545 y(Sp)s(ecF)-8
-b(rame)427 2645 y Fj(All)28 b(Sp)r(ecF)-7 b(rames)27
+b(rame)427 2645 y Fi(All)28 b(Sp)r(ecF)-7 b(rames)27
b(ha)n(v)n(e)g(this)h(attribute.)p 0 2842 3780 12 v 0
2973 a Fz(AlignSystem)219 b Fe(Co)s(ordinate)36 b(system)i(in)h(whic)m
(h)f(to)g(align)1629 3088 y(the)g(F)-10 b(rame)3037 2973
-y Fz(AlignSystem)0 3256 y Fd(Description:)44 b Fj(This)34
+y Fz(AlignSystem)0 3256 y Fd(Description:)44 b Fi(This)34
b(attribute)f(con)n(trols)f(ho)n(w)h(a)g(F)-7 b(rame)32
b(b)r(eha)n(v)n(es)h(when)g(it)h(is)f(used)h(\(b)n(y)f(astFindF)-7
b(rame)33 b(or)f(ast-)227 3355 y(Con)n(v)n(ert\))h(as)g(a)g(template)h
@@ -133910,12 +129631,12 @@ b(will)i(b)r(e)g(aligned)f(b)n(y)h(the)f(matc)n(h.)227
f(to)g(this)h(attribute,)i(and)d(its)h(default)g(v)-5
b(alue,)37 b(dep)r(end)f(on)g(the)g(class)227 3679 y(of)i(F)-7
b(rame)37 b(and)h(are)e(describ)r(ed)i(in)g(the)g Ft(")p
-Fj(Applicabilit)n(y)p Ft(")f Fj(section)h(b)r(elo)n(w.)66
+Fi(Applicabilit)n(y)p Ft(")f Fi(section)h(b)r(elo)n(w.)66
b(In)38 b(general,)h(the)f(AlignSystem)227 3778 y(attribute)28
b(will)g(accept)f(an)n(y)g(of)h(the)g(v)-5 b(alues)27
b(whic)n(h)g(ma)n(y)g(b)r(e)h(assigned)f(to)g(the)h(System)g
(attribute.)227 3902 y(The)c(Mapping)g(returned)g(b)n(y)f(AST)p
-Ft(_)p Fj(FINDFRAME)i(or)f(AST)p Ft(_)p Fj(CONVER)-7
+Ft(_)p Fi(FINDFRAME)i(or)f(AST)p Ft(_)p Fi(CONVER)-7
b(T)23 b(will)i(use)f(the)g(co)r(ordinate)f(system)227
4002 y(sp)r(eci\014ed)30 b(b)n(y)g(the)g(AlignSystem)g(attribute)g(as)f
(an)g(in)n(termediate)g(co)r(ordinate)g(system.)43 b(The)30
@@ -133927,33 +129648,33 @@ b(will)g(then)g(map)g(these)g(p)r(ositions)f(from)g(the)h(in)n
(termediate)227 4301 y(co)r(ordinate)27 b(system)g(in)n(to)g(the)h
(second)f(F)-7 b(rame,)27 b(using)h(the)g(attributes)f(of)h(the)g
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+y Fi(String.)0 4697 y Fd(Class)31 b(Applicabilit)m(y:)259
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(for)g(a)f(basic)h(F)-7 b(rame)35 b(alw)n(a)n(ys)f(equals)h
-Ft(")p Fj(Cartesian)p Ft(")p Fj(,)h(and)g(ma)n(y)f(not)h(b)r(e)427
+Ft(")p Fi(Cartesian)p Ft(")p Fi(,)h(and)g(ma)n(y)f(not)h(b)r(e)427
5031 y(altered.)259 5163 y Fd(CmpF)-8 b(rame)427 5262
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%%Page: 439 449
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eop end
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%%Page: 473 483
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eop end
%%Page: 474 484
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%%Page: 490 500
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%%Page: 491 501
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%%Page: 493 503
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%%Page: 495 505
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%%Page: 496 506
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end
%%Page: 503 513
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%%Page: 505 515
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eop end
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%%Page: 536 546
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%%Page: 537 547
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(from)g(absolute)g(to)h(o\013set)f(co)r(ordinates)p eop
end
%%Page: 550 560
@@ -143881,7 +139602,7 @@ TeXDict begin 550 559 bop 0 52 a FF(550)2251 b Fy(D)91
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eop end
@@ -143948,7 +139669,7 @@ eop end
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%%Page: 552 562
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2118 y(connect)e(it)h(to)g(an)f(external)f(data)h(store)g(b)n(y)g
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%%Page: 557 567
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eop end
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%%Page: 559 569
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eop end
%%Page: 560 570
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%%Page: 561 571
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%%Page: 562 572
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eop end
%%Page: 563 573
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%%Page: 564 574
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%%Page: 566 576
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3440 y(tance\))32 b(ha)m(v)m(e)g(b)s(een)d(added)h(to)h(the)g(F)-8
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-5063 y(new)30 b(facilities.)p eop end
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+(\(the)f(curren)m(t)f(v)m(ersion\):)p eop end
+%%Page: 626 636
+TeXDict begin 626 635 bop 0 52 a FF(626)2016 b Fy(H)91
+b(CHANGES)31 b(AND)g(NEW)g(FEA)-8 b(TURES)111 351 y FF(1.)46
+b(F)-8 b(undamen)m(tal)35 b(p)s(ositional)h(astronom)m(y)f
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+(C\).)g(Copies)h(of)f(these)227 690 y(libraries)j(are)g(bundled)d(with)
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+(adv)-5 b(an)m(tage)27 b(of)e(these)0 1291 y(new)30 b(facilities.)p
+eop end
%%Trailer
userdict /end-hook known{end-hook}if
diff --git a/sun211.tex b/sun211.tex
index c5e6551..f4ba5e7 100644
--- a/sun211.tex
+++ b/sun211.tex
@@ -17,17 +17,17 @@
\newcommand{\stardocsource} {sun\stardocnumber}
% Variable part - replace [xxx] as appropriate.
-\newcommand{\stardocnumber} {211.26}
+\newcommand{\stardocnumber} {211.27}
\newcommand{\stardocauthors} {R.F. Warren-Smith \& D.S. Berry}
-\newcommand{\stardocdate} {4th October 2011}
+\newcommand{\stardocdate} {16th February 2012}
\newcommand{\stardoctitle} {AST\\
A Library for Handling\\
World Coordinate Systems\\
in Astronomy}
-\newcommand{\stardoccopyright} {Copyright (C) 2009 Science \& Technology Facilities Council}
+\newcommand{\stardoccopyright} {Copyright (C) 2012 Science \& Technology Facilities Council}
\newcommand{\stardoctitlehtml} {AST - A Library for Handling World Coordinate
Systems in Astronomy}
-\newcommand{\stardocversion} {V6.0}
+\newcommand{\stardocversion} {V7.0}
\newcommand{\stardocmanual} {Programmer's Guide\\(C Version)}
\newcommand{\stardocmanualhtml}{Programmer's Guide (C Version)}
\newcommand{\stardocabstract} {
@@ -778,10 +778,11 @@ are described here:
\begin{enumerate}
\item {\bf{Minimum Software Dependencies.}}
-The AST library depends on no other other software\footnote{It now comes with a
-minimal cut-down version of the widely-available SLALIB positional astronomy
-library (\xref{SUN/67}{sun67}{}), including just those functions needed
-by AST, and the previous dependency on SLALIB is no longer present}.
+The AST library depends on no other other software\footnote{It comes with
+bundled copies of the IAU SOFA and Starlink PAL libraries which are built
+at the same time as the other AST internal libraries. Alternatively, external
+PAL and SOFA libraries may be used by specifying the ``{\tt
+--with-external\_pal}'' option when configuring AST}.
\item {\bf{Environment Independence.}}
AST is designed so that it can operate in a variety of ``programming
@@ -47959,20 +47960,16 @@ in a non-standard location.} is on your PATH.
}
}
\sstdiytopic{
- SLALIB
+ SOFA \& PAL
}{
- The AST distribution includes a cut down subset of the C version of
- the SLALIB library written by Pat Wallace. This subset contains only
- the functions needed by the AST library. It is built as part of the
- process of building AST and is distributed under GPL (and is thus
- compatible with the AST license). Previous version of this script
- allowed AST applications to be linked against external SLALIB
- libraries (either Fortran or C) rather than the internal version.
- The current version of this script does not provide this option,
- and always uses the internal SLALIB library. However, for backward
- compatibility, this script still allows the {\tt{"}}-fsla{\tt{"}} and {\tt{"}}-csla{\tt{"}} flags
- (previously used for selecting which version of SLALIB to use) to be
- specified, but they will be ignored.
+ The AST distribution includes bundled copies of the IAU SOFA and
+ Starlink PAL libraries. These will be used for fundamental
+ positional astronomy calculations unless the {\tt{"}}--with-external\_pal{\tt{"}}
+ option was used when AST was configured. If {\tt{"}}--with-external\_pal{\tt{"}}
+ is used, this script will include {\tt{"}}-lpal{\tt{"}} in the returned list of
+ linking options, and the user should then ensure that extrnal copies
+ of the PAL and SOFA libraries are available (SOFA functions are used
+ within PAL).
}
}
\sstroutine{
@@ -52221,12 +52218,10 @@ function \htmlref{astTuneC}{astTuneC}.
\end{enumerate}
-\subsection{\xlabel{changes}\xlabel{list_of_most_recent_changes}Changes
-Introduced in V6.0-1}
+\subsection{Changes Introduced in V6.0-1}
-The following describes the most significant changes which have
-occurred in the AST library between versions V6.0 and V6.0-1 (the
-current version):
+The following describes the most significant changes which
+occurred in the AST library between versions V6.0 and V6.0-1:
\begin{enumerate}
@@ -52242,6 +52237,25 @@ be used when aligning SkyFrames if the \htmlref{AlignSystem}{AlignSystem} attrib
\end{enumerate}
+\subsection{\xlabel{changes}\xlabel{list_of_most_recent_changes}Changes
+Introduced in V7.0.0}
+
+The following describes the most significant changes which have
+occurred in the AST library between versions V6.0-1 and V7.0.0 (the
+current version):
+
+\begin{enumerate}
+
+\item Fundamental positional astronomy calculations are now performed
+using the IAU SOFA library where possible, and the Starlink PAL library
+otherwise (the PAL library contains a subset of the Fortran Starlink SLALIB
+library re-written in C). Copies of these libraries are bundled with AST
+and so do not need to be obtained or built separately, although external
+copies of SOFA and PAL can be used if necessary by including the
+``{\tt --with-external\_pal}'' option when configuring AST.
+
+\end{enumerate}
+
Programs which are statically linked will need to be re-linked in
order to take advantage of these new facilities.
diff --git a/timeframe.c b/timeframe.c
index 7acc586..6fed52a 100644
--- a/timeframe.c
+++ b/timeframe.c
@@ -1180,14 +1180,14 @@ static const char *Format( AstFrame *this_frame, int axis, double value, int *st
/* Convert the MJD into a set of numeric date fields, plus day fraction,
and format them. */
- palSlaDjcl( mjd, &iy, &im, &id, &fd, &j );
+ palDjcl( mjd, &iy, &im, &id, &fd, &j );
d = format_buff;
d += sprintf( d, "%4d-%2.2d-%2.2d", iy, im, id );
/* If required, convert the day fraction into a set of numerical time
fields. */
if( ndp >= 0 ) {
- palSlaDd2tf( ndp, fd, sign, ihmsf );
+ palDd2tf( ndp, fd, sign, ihmsf );
/* Format the time fields. */
if( ndp > 0 ) {
diff --git a/timemap.c b/timemap.c
index 66a75a8..98b2292 100644
--- a/timemap.c
+++ b/timemap.c
@@ -498,33 +498,33 @@ static void AddArgs( int cvttype, double *cvtargs, int *status ) {
break;
case AST__MJDTOBEP:
- cvtargs[ 2 ] = palSlaEpb( cvtargs[ 0 ] ) - palSlaEpb( 0.0 ) - cvtargs[ 1 ];
- cvtargs[ 3 ] = palSlaEpb2d( cvtargs[ 1 ] ) - palSlaEpb2d( 0.0 ) - cvtargs[ 0 ];
+ cvtargs[ 2 ] = palEpb( cvtargs[ 0 ] ) - palEpb( 0.0 ) - cvtargs[ 1 ];
+ cvtargs[ 3 ] = palEpb2d( cvtargs[ 1 ] ) - palEpb2d( 0.0 ) - cvtargs[ 0 ];
break;
case AST__BEPTOMJD:
- cvtargs[ 2 ] = palSlaEpb2d( cvtargs[ 0 ] ) - palSlaEpb2d( 0.0 ) - cvtargs[ 1 ];
- cvtargs[ 3 ] = palSlaEpb( cvtargs[ 1 ] ) - palSlaEpb( 0.0 ) - cvtargs[ 0 ];
+ cvtargs[ 2 ] = palEpb2d( cvtargs[ 0 ] ) - palEpb2d( 0.0 ) - cvtargs[ 1 ];
+ cvtargs[ 3 ] = palEpb( cvtargs[ 1 ] ) - palEpb( 0.0 ) - cvtargs[ 0 ];
break;
case AST__MJDTOJEP:
- cvtargs[ 2 ] = palSlaEpj( cvtargs[ 0 ] ) - palSlaEpj( 0.0 ) - cvtargs[ 1 ];
- cvtargs[ 3 ] = palSlaEpj2d( cvtargs[ 1 ] ) - palSlaEpj2d( 0.0 ) - cvtargs[ 0 ];
+ cvtargs[ 2 ] = palEpj( cvtargs[ 0 ] ) - palEpj( 0.0 ) - cvtargs[ 1 ];
+ cvtargs[ 3 ] = palEpj2d( cvtargs[ 1 ] ) - palEpj2d( 0.0 ) - cvtargs[ 0 ];
break;
case AST__JEPTOMJD:
- cvtargs[ 2 ] = palSlaEpj2d( cvtargs[ 0 ] ) - palSlaEpj2d( 0.0 ) - cvtargs[ 1 ];
- cvtargs[ 3 ] = palSlaEpj( cvtargs[ 1 ] ) - palSlaEpj( 0.0 ) - cvtargs[ 0 ];
+ cvtargs[ 2 ] = palEpj2d( cvtargs[ 0 ] ) - palEpj2d( 0.0 ) - cvtargs[ 1 ];
+ cvtargs[ 3 ] = palEpj( cvtargs[ 1 ] ) - palEpj( 0.0 ) - cvtargs[ 0 ];
break;
case AST__TTTOTDB:
- palSlaGeoc( cvtargs[ 2 ], cvtargs[ 3 ], &r, &z );
+ palGeoc( cvtargs[ 2 ], cvtargs[ 3 ], &r, &z );
cvtargs[ 4 ] = 0.001*r*AST__AU;
cvtargs[ 5 ] = 0.001*z*AST__AU;
break;
case AST__TDBTOTT:
- palSlaGeoc( cvtargs[ 2 ], cvtargs[ 3 ], &r, &z );
+ palGeoc( cvtargs[ 2 ], cvtargs[ 3 ], &r, &z );
cvtargs[ 4 ] = 0.001*r*AST__AU;
cvtargs[ 5 ] = 0.001*z*AST__AU;
break;
@@ -1294,8 +1294,12 @@ double astDat_( double in, int forward, int *status ){
------------------------------- */
if( forward ) {
+/* 2012 July 1 */
+ if ( in >= 56109.0 ) {
+ result = 35.0;
+
/* 2009 January 1 */
- if ( in >= 54832.0 ) {
+ } else if ( in >= 54832.0 ) {
result = 34.0;
/* 2006 January 1 */
@@ -1456,8 +1460,12 @@ double astDat_( double in, int forward, int *status ){
} else {
+/* 2012 July 1 */
+ if( in >= 56109.0 + 35.0/SPD ) {
+ result = -35.0;
+
/* 2009 January 1 */
- if( in >= 54832.0 + 34.0/SPD ) {
+ } else if( in >= 54832.0 + 34.0/SPD ) {
result = -34.0;
/* 2006 January 1 */
@@ -3857,13 +3865,13 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
if ( forward ) {
for ( point = 0; point < npoint; point++ ) {
if ( time[ point ] != AST__BAD ) {
- time[ point ] = palSlaEpb( time[ point ] ) + args[ 2 ];
+ time[ point ] = palEpb( time[ point ] ) + args[ 2 ];
}
}
} else {
for ( point = 0; point < npoint; point++ ) {
if ( time[ point ] != AST__BAD ) {
- time[ point ] = palSlaEpb2d( time[ point ] ) + args[ 3 ];
+ time[ point ] = palEpb2d( time[ point ] ) + args[ 3 ];
}
}
}
@@ -3875,13 +3883,13 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
if ( forward ) {
for ( point = 0; point < npoint; point++ ) {
if ( time[ point ] != AST__BAD ) {
- time[ point ] = palSlaEpb2d( time[ point ] ) + args[ 2 ];
+ time[ point ] = palEpb2d( time[ point ] ) + args[ 2 ];
}
}
} else {
for ( point = 0; point < npoint; point++ ) {
if ( time[ point ] != AST__BAD ) {
- time[ point ] = palSlaEpb( time[ point ] ) + args[ 3 ];
+ time[ point ] = palEpb( time[ point ] ) + args[ 3 ];
}
}
}
@@ -3893,13 +3901,13 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
if ( forward ) {
for ( point = 0; point < npoint; point++ ) {
if ( time[ point ] != AST__BAD ) {
- time[ point ] = palSlaEpj( time[ point ] ) + args[ 2 ];
+ time[ point ] = palEpj( time[ point ] ) + args[ 2 ];
}
}
} else {
for ( point = 0; point < npoint; point++ ) {
if ( time[ point ] != AST__BAD ) {
- time[ point ] = palSlaEpj2d( time[ point ] ) + args[ 3 ];
+ time[ point ] = palEpj2d( time[ point ] ) + args[ 3 ];
}
}
}
@@ -3911,13 +3919,13 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
if ( forward ) {
for ( point = 0; point < npoint; point++ ) {
if ( time[ point ] != AST__BAD ) {
- time[ point ] = palSlaEpj2d( time[ point ] ) + args[ 2 ];
+ time[ point ] = palEpj2d( time[ point ] ) + args[ 2 ];
}
}
} else {
for ( point = 0; point < npoint; point++ ) {
if ( time[ point ] != AST__BAD ) {
- time[ point ] = palSlaEpj( time[ point ] ) + args[ 3 ];
+ time[ point ] = palEpj( time[ point ] ) + args[ 3 ];
}
}
}
@@ -4300,7 +4308,7 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
gmstx = time[ point ] + args[ 1 ]/D2PI;
tdb = Gmsta( gmstx, args[ 0 ], 0, status )
+ args[ 0 ] + (32 + TTOFF)/SPD;
- time[ point ] += palSlaEqeqx( tdb )/D2PI;
+ time[ point ] += palEqeqx( tdb )/D2PI;
}
}
} else {
@@ -4309,7 +4317,7 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
gmstx = time[ point ] + args[ 1 ]/D2PI;
tdb = Gmsta( gmstx, args[ 0 ], 0, status )
+ args[ 0 ] + (32+TTOFF)/SPD;
- time[ point ] -= palSlaEqeqx( tdb )/D2PI;
+ time[ point ] -= palEqeqx( tdb )/D2PI;
}
}
}
@@ -4324,7 +4332,7 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
gmstx = time[ point ] + args[ 1 ]/D2PI;
tdb = Gmsta( gmstx, args[ 0 ], 0, status )
+ args[ 0 ] + (32+TTOFF)/SPD;
- time[ point ] -= palSlaEqeqx( tdb )/D2PI;
+ time[ point ] -= palEqeqx( tdb )/D2PI;
}
}
} else {
@@ -4333,7 +4341,7 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
gmstx = time[ point ] + args[ 1 ]/D2PI;
tdb = Gmsta( gmstx, args[ 0 ], 0, status )
+ args[ 0 ] + (32 + TTOFF)/SPD;
- time[ point ] += palSlaEqeqx( tdb )/D2PI;
+ time[ point ] += palEqeqx( tdb )/D2PI;
}
}
}
diff --git a/unitmap.c b/unitmap.c
index cab10d8..b4f004d 100644
--- a/unitmap.c
+++ b/unitmap.c
@@ -53,6 +53,7 @@ f The UnitMap class does not define any new routines beyond those
* Authors:
* RFWS: R.F. Warren-Smith (Starlink)
+* DSB: David S Berry (JAC, Hawaii)
* History:
* 7-FEB-1996 (RFWS):
@@ -64,6 +65,9 @@ f The UnitMap class does not define any new routines beyond those
* method.
* 10-MAY-2006 (DSB):
* Override astEqual.
+* 17-FEB-2012 (DSB):
+* In Transform, do not copy the coordinate values if the input and
+* output array are the same.
*class--
*/
@@ -889,11 +893,14 @@ static AstPointSet *Transform( AstMapping *this, AstPointSet *in,
/* --------------------------- */
if ( astOK ) {
-/* Loop to copy the values for each coordinate. Use a memory copy for speed. */
+/* Loop to copy the values for each coordinate. Use a memory copy for speed.
+ Do not do the copy if the input and output arrays are the same. */
for ( coord = 0; coord < ncoord_in; coord++ ) {
- (void) memcpy( (void *) ptr_out[ coord ],
- (const void *) ptr_in[ coord ],
- sizeof( double ) * (size_t) npoint );
+ if( ptr_out[ coord ] != ptr_in[ coord ] ) {
+ (void) memcpy( (void *) ptr_out[ coord ],
+ (const void *) ptr_in[ coord ],
+ sizeof( double ) * (size_t) npoint );
+ }
}
}
diff --git a/version.h b/version.h
index d4054f1..2496a8b 100644
--- a/version.h
+++ b/version.h
@@ -60,14 +60,14 @@
*-
*/
-/* The current version of AST is 6.0.1 */
-#define AST__VMAJOR 6
+/* The current version of AST is 7.0.0 */
+#define AST__VMAJOR 7
#define AST__VMINOR 0
-#define AST__RELEASE 1
+#define AST__RELEASE 0
/* Deprecated macros */
-#define AST_MAJOR_VERS 6
+#define AST_MAJOR_VERS 7
#define AST_MINOR_VERS 0
-#define AST_RELEASE 1
+#define AST_RELEASE 0
#endif /* #if ! defined(VERSION_INCLUDED) */
diff --git a/wcsmap.c b/wcsmap.c
index 48dadb2..1253eb1 100644
--- a/wcsmap.c
+++ b/wcsmap.c
@@ -2760,17 +2760,17 @@ static int Map( AstWcsMap *this, int forward, int npoint, double *in0,
and the latitude is in the range [-90,90] (as required by the WCSLIB
library). Any point with a latitude outside the range [-90,90] is
converted to the equivalent point on the complementary meridian. */
- latitude = AST__DR2D*palSlaDrange( factor*in1[ point ] );
+ latitude = AST__DR2D*palDrange( factor*in1[ point ] );
if ( latitude > 90.0 ){
latitude = 180.0 - latitude;
- longitude = AST__DR2D*palSlaDrange( AST__DPI + factor*in0[ point ] );
+ longitude = AST__DR2D*palDrange( AST__DPI + factor*in0[ point ] );
} else if ( latitude < -90.0 ){
latitude = -180.0 - latitude;
- longitude = AST__DR2D*palSlaDrange( AST__DPI + factor*in0[ point ] );
+ longitude = AST__DR2D*palDrange( AST__DPI + factor*in0[ point ] );
} else {
- longitude = AST__DR2D*palSlaDrange( factor*in0[ point ] );
+ longitude = AST__DR2D*palDrange( factor*in0[ point ] );
}
/* Call the relevant WCSLIB forward projection function. */
@@ -3695,7 +3695,6 @@ static void SetAttrib( AstObject *this_object, const char *setting, int *status
/* Local Variables: */
AstWcsMap *this; /* Pointer to the WcsMap structure */
double dval; /* Attribute value */
- int ival; /* Attribute value */
int len; /* Length of setting string */
int nc; /* Number of characters read by astSscanf */
int i; /* Axis index */
diff --git a/wcsmath.h b/wcsmath.h
index 7d947b5..1f8977a 100644
--- a/wcsmath.h
+++ b/wcsmath.h
@@ -15,7 +15,7 @@
*
* You should have received a copy of the GNU Library General Public License
* along with this library; if not, write to the Free Software Foundation,
-* Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
+* Inc., 51 Franklin Street,Fifth Floor, Boston, MA 02110-1301, USA
*
* Correspondence concerning WCSLIB may be directed to:
* Internet email: mcalabre at atnf.csiro.au
diff --git a/wcstrig.c b/wcstrig.c
index 6b0d4b8..d3ba400 100644
--- a/wcstrig.c
+++ b/wcstrig.c
@@ -14,8 +14,8 @@
* General Public License for more details.
*
* You should have received a copy of the GNU Library General Public License
-* along with this library; if not, write to the Free Software Foundation,
-* Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
+* along with this library; if not, write to the Free Software Foundation,
+* Inc., 51 Franklin Street,Fifth Floor, Boston, MA 02110-1301, USA
*
* Correspondence concerning WCSLIB may be directed to:
* Internet email: mcalabre at atnf.csiro.au
diff --git a/wcstrig.h b/wcstrig.h
index 61f3392..36463bb 100644
--- a/wcstrig.h
+++ b/wcstrig.h
@@ -15,7 +15,7 @@
*
* You should have received a copy of the GNU Library General Public License
* along with this library; if not, write to the Free Software Foundation,
-* Inc., 675 Mass Ave, Cambridge, MA 02139, USA.
+* Inc., 51 Franklin Street,Fifth Floor, Boston, MA 02110-1301, USA
*
* Correspondence concerning WCSLIB may be directed to:
* Internet email: mcalabre at atnf.csiro.au
diff --git a/xmlchan.c b/xmlchan.c
index c5576ad..1a60c5c 100644
--- a/xmlchan.c
+++ b/xmlchan.c
@@ -222,6 +222,7 @@ f The XmlChan class does not define any new routines beyond those
#include "object.h" /* Base Object class */
#include "wcsmap.h" /* Angular conversion constants */
#include "xml.h" /* AST XML facilities */
+#include "sofa.h" /* IAU SOFA functions */
#include "stcresourceprofile.h" /* IVOA StcResourceProfile class */
#include "stcsearchlocation.h" /* IVOA SearchLocation class */
#include "stccatalogentrylocation.h"/* IVOA CatalogEntryLocation class */
@@ -428,7 +429,6 @@ static void Copy( const AstObject *, AstObject *, int * );
static void Delete( AstObject *, int * );
static void Dump( AstObject *, AstChannel *, int * );
static void FillAndLims( AstXmlChan *, AstXmlElement *, AstRegion *, int * );
-static void Geod( double, double, double *, double *, int * );
static void OutputText( AstXmlChan *, const char *, int, int * );
static void ReCentreAnc( AstRegion *, int, AstKeyMap **, int * );
static void ReadClassData( AstChannel *, const char *, int * );
@@ -2918,7 +2918,7 @@ static AstRegion *ConstraintReader( AstXmlChan *this, AstXmlElement *elem,
vec[1] = 0.0;
vec[2] = 0.0;
ElemListD( this, scan->el[0][0], 3, vec, status );
- palSlaDcc2s( vec, cen, cen + 1 );
+ palDcc2s( vec, cen, cen + 1 );
/* Get the offset, and convert to a radial distance in radians. */
rad = acos( ElemValueD( this, scan->el[1][0], 1.0, status ) );
@@ -4643,130 +4643,6 @@ static IVOAScan *FreeIVOAScan( IVOAScan *in, int *status ){
return NULL;
}
-static void Geod( double lat, double lon, double *phi, double *lambda, int *status ){
-/*
-* Name:
-* Geod
-
-* Purpose:
-* Convert a geocentric lat/long to geodetic lat/long at sea level.
-
-* Type:
-* Private function.
-
-* Synopsis:
-* #include "xmlchan.h"
-* void Geod( double lat, double lon, double *phi, double *lambda, int *status )
-
-* Class Membership:
-* FitsChan member function.
-
-* Description:
-* This function converts a position supplied as geocentric lat/lon at
-* sea level into geodetic longitude, latitude. The algorithm is due to
-* Borkowski, and is described in the Explanatory Supplement to the
-* Astronomical Almanac (p206).
-
-* Parameters:
-* lat
-* Geocentric latitude (radians)
-* lon
-* Geocentric longitude (radians).
-* phi
-* Pointer at a location at which to return the geodetic latitude,
-* in radians.
-* lambda
-* Pointer at a location at which to return the geodetic longitude,
-* in radians.
-* status
-* Pointer to the inherited status variable.
-*/
-
-/* Local Constants... */
-#define FL 1.0/298.257 /* Reference spheroid flattening factor */
-#define A0 6378140.0 /* Earth equatorial radius (metres) */
-
-/* Local Variables... */
- double r, e, f, p, q, d, n, g, t, rp, rd, sn, b0, boa, ab2oa;
- double pos[3];
-
-/* Initialise */
- *phi = 0.0;
- *lambda = 0.0;
-
-/* Check the global status. */
- if( !astOK ) return;
-
-/* Convert the supplied geocentric lon/lat to terrestrial Cartesian
- (x,y,z) values. The (x,y,z) system has origin at the centre of the
- earth, Z axis going through the north pole, X axis at (long,lat)=(0,0),
- and Y axis at (long,lat) = (E90,0). Assume an equatorial sea level
- position. */
- palSlaDcs2c( lon, lat, pos );
- pos[ 0 ] *= A0;
- pos[ 1 ] *= A0;
- pos[ 2 ] *= A0;
-
-/* Earth polar radius (metres) */
- b0 = A0*( 1.0 - FL );
-
-/* Useful functions */
- boa = b0/A0;
- ab2oa = ( A0*A0 - b0*b0)/A0;
-
-/* To obtain the proper sign and polynomial solution, the sign of b is
- set to that of z. Note the sign of z. */
- if( pos[ 2 ] > 0.0 ) {
- sn = 1.0;
- } else {
- sn = -1.0;
- }
-
-/* If the supplied position is on the polar axis, the returned values are
- trivial. We check this case because it corresponds to a singularity in
- the main algorithm. */
- r = sqrt( pos[ 0 ]*pos[ 0 ] + pos[ 1 ]*pos[ 1 ] );
- if( r == 0 ) {
- *lambda = 0.0;
- *phi = AST__DPIBY2;
-
- } else {
-
-/* The longitude is unchanged. */
- *lambda = lon;
-
-/* The equator is also a singularity in the main algorithm. If the
- supplied point is on the equator, the answers are trivial. */
- if( pos[ 2 ] == 0.0 ) {
- *phi = 0.0;
-
-/* For all other cases, use the main Borkowski algorithm. */
- } else {
- e = ( sn*boa*pos[ 2 ] - ab2oa )/r;
- f = ( sn*boa*pos[ 2 ] + ab2oa )/r;
- p = 4.0*( e*f + 1.0 )/3.0;
- q = 2.0*( e*e - f*f );
- d = p*p*p + q*q;
-
- if( d < 0.0 ) {
- rp = sqrt( -p );
- n = 2.0*rp*cos( acos( q/(p*rp) )/3.0 );
- } else {
- rd = sqrt( d );
- n = pow( ( rd - q ), 1.0/3.0 ) - pow( (rd + q ), 1.0/3.0 );
- }
-
- g = 0.5* ( sqrt( e*e + n ) + e );
- t = sqrt( g*g + ( f - n*g )/( 2*g - e ) ) - g;
-
- *phi = atan( A0*( 1.0 - t*t )/( 2.0*sn*b0*t ) );
-
- }
- }
-}
-#undef FL
-#undef A0
-
static const char *GetAttrib( AstObject *this_object, const char *attrib, int *status ) {
/*
* Name:
@@ -5933,6 +5809,9 @@ static AstPointList *ObservatoryLocationReader( AstXmlChan *this,
*/
+/* Local Constants: */
+#define A0 6378140.0 /* Earth equatorial radius (metres) */
+
/* Local Variables: */
AstFrame *frm; /* Pointer to obsvtory lon/lat Frame */
AstFrame *obs_frm; /* Pointer to obsvation lon/lat Frame */
@@ -6034,7 +5913,23 @@ static AstPointList *ObservatoryLocationReader( AstXmlChan *this,
pfrm = astAnnul( pfrm );
}
- if( lon != AST__BAD ) Geod( lat, lon, &phi, &lambda, status );
+/* If required, convert from geocentric lon/lat to geodetic lon/lat. */
+ if( lon != AST__BAD ) {
+ double pos[ 3 ], height;
+
+/* Convert the supplied geocentric lon/lat to terrestrial Cartesian
+ (x,y,z) values. The (x,y,z) system has origin at the centre of the
+ earth, Z axis going through the north pole, X axis at (long,lat)=(0,0),
+ and Y axis at (long,lat) = (E90,0). Assume an equatorial sea level
+ position. */
+ palDcs2c( lon, lat, pos );
+ pos[ 0 ] *= A0;
+ pos[ 1 ] *= A0;
+ pos[ 2 ] *= A0;
+
+/* Get the corresponding geodetic lon/lat. */
+ iauGc2gd( 1, pos, &lambda, &phi, &height );
+ }
if( lambda != AST__BAD ) {
obs_frm = astGetFrame( ((AstRegion *) obs)->frameset, AST__CURRENT );
@@ -6068,6 +5963,7 @@ static AstPointList *ObservatoryLocationReader( AstXmlChan *this,
/* Return the pointer to the new Region. */
return (AstPointList *) new;
}
+#undef A0
static void OutputText( AstXmlChan *this, const char *text, int mxlen, int *status ) {
/*
--
Handle World Coordinate Systems in Astronomy
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