Repatch (from linux) of OSX IRAF

1 files changed, 140 insertions, 0 deletions

diff --git a/math/slalib/hfk5z.f b/math/slalib/hfk5z.f
new file mode 100644
index 00000000..2f6d53b2
--- /dev/null
+++ b/math/slalib/hfk5z.f
@@ -0,0 +1,140 @@
+      SUBROUTINE slHF5Z (RH,DH,EPOCH,R5,D5,DR5,DD5)
+*+
+*     - - - - - -
+*      H F 5 Z
+*     - - - - - -
+*
+*  Transform a Hipparcos star position into FK5 J2000, assuming
+*  zero Hipparcos proper motion.
+*
+*  (double precision)
+*
+*  Given:
+*     RH        d      Hipparcos RA (radians)
+*     DH        d      Hipparcos Dec (radians)
+*     EPOCH     d      Julian epoch (TDB)
+*
+*  Returned (all FK5, equinox J2000, epoch EPOCH):
+*     R5        d      RA (radians)
+*     D5        d      Dec (radians)
+*
+*  Called:  slDS2C, slDAVM, slDMXV, slDMXM,
+*           slDIMV, slDVXV, slDC6S, slDA2P
+*
+*  Notes:
+*
+*  1)  The proper motion in RA is dRA/dt rather than cos(Dec)*dRA/dt.
+*
+*  2)  The FK5 to Hipparcos transformation consists of a pure
+*      rotation and spin;  zonal errors in the FK5 catalogue are
+*      not taken into account.
+*
+*  3)  The published orientation and spin components are interpreted
+*      as "axial vectors".  An axial vector points at the pole of the
+*      rotation and its length is the amount of rotation in radians.
+*
+*  4)  It was the intention that Hipparcos should be a close
+*      approximation to an inertial frame, so that distant objects
+*      have zero proper motion;  such objects have (in general)
+*      non-zero proper motion in FK5, and this routine returns those
+*      fictitious proper motions.
+*
+*  5)  The position returned by this routine is in the FK5 J2000
+*      reference frame but at Julian epoch EPOCH.
+*
+*  6)  See also slFK5H, slHFK5, sla_FK5ZHZ.
+*
+*  Reference:
+*
+*     M.Feissel & F.Mignard, Astron. Astrophys. 331, L33-L36 (1998).
+*
+*  P.T.Wallace   Starlink   30 December 1999
+*
+*  Copyright (C) 1999 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 RH,DH,EPOCH,R5,D5,DR5,DD5
+
+      DOUBLE PRECISION AS2R
+      PARAMETER (AS2R=0.484813681109535994D-5)
+
+*  FK5 to Hipparcos orientation and spin (radians, radians/year)
+      DOUBLE PRECISION EPX,EPY,EPZ
+      DOUBLE PRECISION OMX,OMY,OMZ
+
+      PARAMETER ( EPX = -19.9D-3 * AS2R,
+     :            EPY =  -9.1D-3 * AS2R,
+     :            EPZ = +22.9D-3 * AS2R )
+
+      PARAMETER ( OMX = -0.30D-3 * AS2R,
+     :            OMY = +0.60D-3 * AS2R,
+     :            OMZ = +0.70D-3 * AS2R )
+
+      DOUBLE PRECISION PH(3),ORTN(3),R5H(3,3),S5(3),SH(3),T,VST(3),
+     :                 RST(3,3),R5HT(3,3),PV5E(6),VV(3),W,R,V
+
+      DOUBLE PRECISION slDA2P
+
+
+
+*  Hipparcos barycentric position vector (normalized).
+      CALL slDS2C(RH,DH,PH)
+
+*  FK5 to Hipparcos orientation matrix.
+      ORTN(1) = EPX
+      ORTN(2) = EPY
+      ORTN(3) = EPZ
+      CALL slDAVM(ORTN,R5H)
+
+*  Hipparcos wrt FK5 spin vector.
+      S5(1) = OMX
+      S5(2) = OMY
+      S5(3) = OMZ
+
+*  Rotate the spin vector into the Hipparcos frame.
+      CALL slDMXV(R5H,S5,SH)
+
+*  Time interval from J2000 to epoch.
+      T = EPOCH-2000D0
+
+*  Axial vector:  accumulated Hipparcos wrt FK5 spin over that interval.
+      VST(1) = OMX*T
+      VST(2) = OMY*T
+      VST(3) = OMZ*T
+
+*  Express the accumulated spin as a rotation matrix.
+      CALL slDAVM(VST,RST)
+
+*  Rotation matrix:  accumulated spin, then FK5 to Hipparcos.
+      CALL slDMXM(R5H,RST,R5HT)
+
+*  De-orient & de-spin the vector into FK5 J2000 at epoch.
+      CALL slDIMV(R5HT,PH,PV5E)
+      CALL slDVXV(SH,PH,VV)
+      CALL slDIMV(R5HT,VV,PV5E(4))
+
+*  FK5 position/velocity 6-vector to spherical.
+      CALL slDC6S(PV5E,W,D5,R,DR5,DD5,V)
+      R5 = slDA2P(W)
+
+      END