From 40e5a5811c6ffce9b0974e93cdd927cbcf60c157 Mon Sep 17 00:00:00 2001
From: Joe Hunkeler <jhunkeler@gmail.com>
Date: Tue, 11 Aug 2015 16:51:37 -0400
Subject: Repatch (from linux) of OSX IRAF

---
 math/slalib/dtp2v.f | 74 +++++++++++++++++++++++++++++++++++++++++++++++++++++
 1 file changed, 74 insertions(+)
 create mode 100644 math/slalib/dtp2v.f

(limited to 'math/slalib/dtp2v.f')

diff --git a/math/slalib/dtp2v.f b/math/slalib/dtp2v.f
new file mode 100644
index 00000000..077df7a8
--- /dev/null
+++ b/math/slalib/dtp2v.f
@@ -0,0 +1,74 @@
+      SUBROUTINE slDTPV (XI, ETA, V0, V)
+*+
+*     - - - - - -
+*      D T P V
+*     - - - - - -
+*
+*  Given the tangent-plane coordinates of a star and the direction
+*  cosines of the tangent point, determine the direction cosines
+*  of the star.
+*
+*  (double precision)
+*
+*  Given:
+*     XI,ETA    d       tangent plane coordinates of star
+*     V0        d(3)    direction cosines of tangent point
+*
+*  Returned:
+*     V         d(3)    direction cosines of star
+*
+*  Notes:
+*
+*  1  If vector V0 is not of unit length, the returned vector V will
+*     be wrong.
+*
+*  2  If vector V0 points at a pole, the returned vector V will be
+*     based on the arbitrary assumption that the RA of the tangent
+*     point is zero.
+*
+*  3  This routine is the Cartesian equivalent of the routine slDTPS.
+*
+*  P.T.Wallace   Starlink   11 February 1995
+*
+*  Copyright (C) 1995 Rutherford Appleton Laboratory
+*
+*  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 (see SLA_CONDITIONS); if not, write to the
+*    Free Software Foundation, Inc., 51 Franklin Street, Fifth Floor,
+*    Boston, MA  02110-1301  USA
+*
+*  Copyright (C) 1995 Association of Universities for Research in Astronomy Inc.
+*-
+
+      IMPLICIT NONE
+
+      DOUBLE PRECISION XI,ETA,V0(3),V(3)
+
+      DOUBLE PRECISION X,Y,Z,F,R
+
+
+      X=V0(1)
+      Y=V0(2)
+      Z=V0(3)
+      F=SQRT(1D0+XI*XI+ETA*ETA)
+      R=SQRT(X*X+Y*Y)
+      IF (R.EQ.0D0) THEN
+         R=1D-20
+         X=R
+      END IF
+      V(1)=(X-(XI*Y+ETA*X*Z)/R)/F
+      V(2)=(Y+(XI*X-ETA*Y*Z)/R)/F
+      V(3)=(Z+ETA*R)/F
+
+      END
-- 
cgit