update ast

1 files changed, 0 insertions, 98 deletions

diff --git a/ast/pal/palPrebn.c b/ast/pal/palPrebn.c
deleted file mode 100644
index 989ce59..0000000
--- a/ast/pal/palPrebn.c
+++ /dev/null
@@ -1,98 +0,0 @@
-/*
-*+
-*  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
-*        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"
-
-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);
-
-}