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+/*
+*+
+* 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
+* Adapted with permission from the Fortran SLALIB library.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 1998 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 Lesser 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 Lesser General Public License for more details.
+*
+* You should have received a copy of the GNU Lesser General
+* License along with this program. If not, see
+* <http://www.gnu.org/licenses/>.
+
+* Bugs:
+* {note_any_bugs_here}
+*-
+*/
+
+#include "pal.h"
+#include "pal1sofa.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 */
+ eraS2c( dl, db, v1 );
+
+ /* Galactic to equatorial */
+ eraTrxp( rmat, v1, v2 );
+
+ /* Cartesian to spherical */
+ eraC2s( v2, dr, dd );
+
+ /* Express in conventional ranges */
+ *dr = eraAnp( *dr );
+ *dd = eraAnpm( *dd );
+
+}