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+/*
+*+
+* 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
+* Adapted with permission from the Fortran SLALIB library.
+* {enter_further_changes_here}
+
+* Copyright:
+* Copyright (C) 1996 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 "palmac.h"
+#include "pal1sofa.h"
+
+void palEcmat( double date, double rmat[3][3] ) {
+
+/* Mean obliquity (the angle between the ecliptic and mean equator of
+ date). */
+ double eps0 = eraObl06( PAL__MJD0, date );
+
+/* Matrix */
+ palDeuler( "X", eps0, 0.0, 0.0, rmat );
+
+}