upgrade ast 8.7.1

1 files changed, 0 insertions, 152 deletions

diff --git a/ast/erfa/atic13.c b/ast/erfa/atic13.c
deleted file mode 100644
index bd70ce5..0000000
--- a/ast/erfa/atic13.c
+++ /dev/null
@@ -1,152 +0,0 @@
-#include "erfa.h"
-
-void eraAtic13(double ri, double di, double date1, double date2,
-               double *rc, double *dc, double *eo)
-/*
-**  - - - - - - - - - -
-**   e r a A t i c 1 3
-**  - - - - - - - - - -
-**
-**  Transform star RA,Dec from geocentric CIRS to ICRS astrometric.
-**
-**  Given:
-**     ri,di  double  CIRS geocentric RA,Dec (radians)
-**     date1  double  TDB as a 2-part...
-**     date2  double  ...Julian Date (Note 1)
-**
-**  Returned:
-**     rc,dc  double  ICRS astrometric RA,Dec (radians)
-**     eo     double  equation of the origins (ERA-GST, Note 4)
-**
-**  Notes:
-**
-**  1) The TDB date date1+date2 is a Julian Date, apportioned in any
-**     convenient way between the two arguments.  For example,
-**     JD(TDB)=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.  For most
-**     applications of this function the choice will not be at all
-**     critical.
-**
-**     TT can be used instead of TDB without any significant impact on
-**     accuracy.
-**
-**  2) Iterative techniques are used for the aberration and light
-**     deflection corrections so that the functions eraAtic13 (or
-**     eraAticq) and eraAtci13 (or eraAtciq) are accurate inverses;
-**     even at the edge of the Sun's disk the discrepancy is only about
-**     1 nanoarcsecond.
-**
-**  3) The available accuracy is better than 1 milliarcsecond, limited
-**     mainly by the precession-nutation model that is used, namely
-**     IAU 2000A/2006.  Very close to solar system bodies, additional
-**     errors of up to several milliarcseconds can occur because of
-**     unmodeled light deflection;  however, the Sun's contribution is
-**     taken into account, to first order.  The accuracy limitations of
-**     the ERFA function eraEpv00 (used to compute Earth position and
-**     velocity) can contribute aberration errors of up to
-**     5 microarcseconds.  Light deflection at the Sun's limb is
-**     uncertain at the 0.4 mas level.
-**
-**  4) Should the transformation to (equinox based) J2000.0 mean place
-**     be required rather than (CIO based) ICRS coordinates, subtract the
-**     equation of the origins from the returned right ascension:
-**     RA = RI - EO.  (The eraAnp function can then be applied, as
-**     required, to keep the result in the conventional 0-2pi range.)
-**
-**  Called:
-**     eraApci13    astrometry parameters, ICRS-CIRS, 2013
-**     eraAticq     quick CIRS to ICRS astrometric
-**
-**  Copyright (C) 2013-2016, NumFOCUS Foundation.
-**  Derived, with permission, from the SOFA library.  See notes at end of file.
-*/
-{
-/* Star-independent astrometry parameters */
-   eraASTROM astrom;
-
-
-/* Star-independent astrometry parameters. */
-   eraApci13(date1, date2, &astrom, eo);
-
-/* CIRS to ICRS astrometric. */
-   eraAticq(ri, di, &astrom, rc, dc);
-
-/* Finished. */
-
-}
-/*----------------------------------------------------------------------
-**  
-**  
-**  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.
-**  
-*/