upgrade AST

1 files changed, 0 insertions, 169 deletions

diff --git a/ast/erfa/fk5hz.c b/ast/erfa/fk5hz.c
deleted file mode 100644
index 4134f7c..0000000
--- a/ast/erfa/fk5hz.c
+++ /dev/null
@@ -1,169 +0,0 @@
-#include "erfa.h"
-
-void eraFk5hz(double r5, double d5, double date1, double date2,
-              double *rh, double *dh)
-/*
-**  - - - - - - - - -
-**   e r a F k 5 h z
-**  - - - - - - - - -
-**
-**  Transform an FK5 (J2000.0) star position into the system of the
-**  Hipparcos catalogue, assuming zero Hipparcos proper motion.
-**
-**  Given:
-**     r5           double   FK5 RA (radians), equinox J2000.0, at date
-**     d5           double   FK5 Dec (radians), equinox J2000.0, at date
-**     date1,date2  double   TDB date (Notes 1,2)
-**
-**  Returned:
-**     rh           double   Hipparcos RA (radians)
-**     dh           double   Hipparcos Dec (radians)
-**
-**  Notes:
-**
-**  1) This function converts a star position from the FK5 system to
-**     the Hipparcos system, in such a way that the Hipparcos proper
-**     motion is zero.  Because such a star has, in general, a non-zero
-**     proper motion in the FK5 system, the function requires the date
-**     at which the position in the FK5 system was determined.
-**
-**  2) The TT date date1+date2 is a Julian Date, apportioned in any
-**     convenient way between the two arguments.  For example,
-**     JD(TT)=2450123.7 could be expressed in any of these ways,
-**     among others:
-**
-**            date1          date2
-**
-**         2450123.7           0.0       (JD method)
-**         2451545.0       -1421.3       (J2000 method)
-**         2400000.5       50123.2       (MJD method)
-**         2450123.5           0.2       (date & time method)
-**
-**     The JD method is the most natural and convenient to use in
-**     cases where the loss of several decimal digits of resolution
-**     is acceptable.  The J2000 method is best matched to the way
-**     the argument is handled internally and will deliver the
-**     optimum resolution.  The MJD method and the date & time methods
-**     are both good compromises between resolution and convenience.
-**
-**  3) The FK5 to Hipparcos transformation is modeled as a pure
-**     rotation and spin;  zonal errors in the FK5 catalogue are not
-**     taken into account.
-**
-**  4) The position returned by this function is in the Hipparcos
-**     reference system but at date date1+date2.
-**
-**  5) See also eraFk52h, eraH2fk5, eraHfk5z.
-**
-**  Called:
-**     eraS2c       spherical coordinates to unit vector
-**     eraFk5hip    FK5 to Hipparcos rotation and spin
-**     eraSxp       multiply p-vector by scalar
-**     eraRv2m      r-vector to r-matrix
-**     eraTrxp      product of transpose of r-matrix and p-vector
-**     eraPxp       vector product of two p-vectors
-**     eraC2s       p-vector to spherical
-**     eraAnp       normalize angle into range 0 to 2pi
-**
-**  Reference:
-**
-**     F.Mignard & M.Froeschle, 2000, Astron.Astrophys. 354, 732-739.
-**
-**  Copyright (C) 2013-2016, NumFOCUS Foundation.
-**  Derived, with permission, from the SOFA library.  See notes at end of file.
-*/
-{
-   double t, p5e[3], r5h[3][3], s5h[3], vst[3], rst[3][3], p5[3],
-          ph[3], w;
-
-
-/* Interval from given date to fundamental epoch J2000.0 (JY). */
-   t = - ((date1 - ERFA_DJ00) + date2) / ERFA_DJY;
-
-/* FK5 barycentric position vector. */
-   eraS2c(r5, d5, p5e);
-
-/* FK5 to Hipparcos orientation matrix and spin vector. */
-   eraFk5hip(r5h, s5h);
-
-/* Accumulated Hipparcos wrt FK5 spin over that interval. */
-   eraSxp(t, s5h, vst);
-
-/* Express the accumulated spin as a rotation matrix. */
-   eraRv2m(vst, rst);
-
-/* Derotate the vector's FK5 axes back to date. */
-   eraTrxp(rst, p5e, p5);
-
-/* Rotate the vector into the Hipparcos system. */
-   eraRxp(r5h, p5, ph);
-
-/* Hipparcos vector to spherical. */
-   eraC2s(ph, &w, dh);
-   *rh = eraAnp(w);
-
-   return;
-
-}
-/*----------------------------------------------------------------------
-**  
-**  
-**  Copyright (C) 2013-2016, NumFOCUS Foundation.
-**  All rights reserved.
-**  
-**  This library is derived, with permission, from the International
-**  Astronomical Union's "Standards of Fundamental Astronomy" library,
-**  available from http://www.iausofa.org.
-**  
-**  The ERFA version is intended to retain identical functionality to
-**  the SOFA library, but made distinct through different function and
-**  file names, as set out in the SOFA license conditions.  The SOFA
-**  original has a role as a reference standard for the IAU and IERS,
-**  and consequently redistribution is permitted only in its unaltered
-**  state.  The ERFA version is not subject to this restriction and
-**  therefore can be included in distributions which do not support the
-**  concept of "read only" software.
-**  
-**  Although the intent is to replicate the SOFA API (other than
-**  replacement of prefix names) and results (with the exception of
-**  bugs;  any that are discovered will be fixed), SOFA is not
-**  responsible for any errors found in this version of the library.
-**  
-**  If you wish to acknowledge the SOFA heritage, please acknowledge
-**  that you are using a library derived from SOFA, rather than SOFA
-**  itself.
-**  
-**  
-**  TERMS AND CONDITIONS
-**  
-**  Redistribution and use in source and binary forms, with or without
-**  modification, are permitted provided that the following conditions
-**  are met:
-**  
-**  1 Redistributions of source code must retain the above copyright
-**    notice, this list of conditions and the following disclaimer.
-**  
-**  2 Redistributions in binary form must reproduce the above copyright
-**    notice, this list of conditions and the following disclaimer in
-**    the documentation and/or other materials provided with the
-**    distribution.
-**  
-**  3 Neither the name of the Standards Of Fundamental Astronomy Board,
-**    the International Astronomical Union nor the names of its
-**    contributors may be used to endorse or promote products derived
-**    from this software without specific prior written permission.
-**  
-**  THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
-**  "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
-**  LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
-**  FOR A PARTICULAR PURPOSE ARE DISCLAIMED.  IN NO EVENT SHALL THE
-**  COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
-**  INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
-**  BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
-**  LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
-**  CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
-**  LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
-**  ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
-**  POSSIBILITY OF SUCH DAMAGE.
-**  
-*/