update ast

1 files changed, 0 insertions, 133 deletions

diff --git a/ast/pal/palDh2e.c b/ast/pal/palDh2e.c
deleted file mode 100644
index 65434b7..0000000
--- a/ast/pal/palDh2e.c
+++ /dev/null
@@ -1,133 +0,0 @@
-/*
-*+
-*  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:
-*     Convert horizon to equatorial coordinates.
-
-*  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
-*        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 <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;
-}