update ast

1 files changed, 0 insertions, 160 deletions

diff --git a/ast/erfa/gmst82.c b/ast/erfa/gmst82.c
deleted file mode 100644
index 5ddf032..0000000
--- a/ast/erfa/gmst82.c
+++ /dev/null
@@ -1,160 +0,0 @@
-#include "erfa.h"
-
-double eraGmst82(double dj1, double dj2)
-/*
-**  - - - - - - - - - -
-**   e r a G m s t 8 2
-**  - - - - - - - - - -
-**
-**  Universal Time to Greenwich mean sidereal time (IAU 1982 model).
-**
-**  Given:
-**     dj1,dj2    double    UT1 Julian Date (see note)
-**
-**  Returned (function value):
-**                double    Greenwich mean sidereal time (radians)
-**
-**  Notes:
-**
-**  1) The UT1 date dj1+dj2 is a Julian Date, apportioned in any
-**     convenient way between the arguments dj1 and dj2.  For example,
-**     JD(UT1)=2450123.7 could be expressed in any of these ways,
-**     among others:
-**
-**             dj1            dj2
-**
-**         2450123.7          0          (JD method)
-**          2451545        -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 and MJD methods are good compromises
-**     between resolution and convenience.  The date & time method is
-**     best matched to the algorithm used:  maximum accuracy (or, at
-**     least, minimum noise) is delivered when the dj1 argument is for
-**     0hrs UT1 on the day in question and the dj2 argument lies in the
-**     range 0 to 1, or vice versa.
-**
-**  2) The algorithm is based on the IAU 1982 expression.  This is
-**     always described as giving the GMST at 0 hours UT1.  In fact, it
-**     gives the difference between the GMST and the UT, the steady
-**     4-minutes-per-day drawing-ahead of ST with respect to UT.  When
-**     whole days are ignored, the expression happens to equal the GMST
-**     at 0 hours UT1 each day.
-**
-**  3) In this function, the entire UT1 (the sum of the two arguments
-**     dj1 and dj2) is used directly as the argument for the standard
-**     formula, the constant term of which is adjusted by 12 hours to
-**     take account of the noon phasing of Julian Date.  The UT1 is then
-**     added, but omitting whole days to conserve accuracy.
-**
-**  Called:
-**     eraAnp       normalize angle into range 0 to 2pi
-**
-**  References:
-**
-**     Transactions of the International Astronomical Union,
-**     XVIII B, 67 (1983).
-**
-**     Aoki et al., Astron. Astrophys. 105, 359-361 (1982).
-**
-**  Copyright (C) 2013-2014, NumFOCUS Foundation.
-**  Derived, with permission, from the SOFA library.  See notes at end of file.
-*/
-{
-/* Coefficients of IAU 1982 GMST-UT1 model */
-   double A = 24110.54841  -  ERFA_DAYSEC / 2.0;
-   double B = 8640184.812866;
-   double C = 0.093104;
-   double D =  -6.2e-6;
-
-/* Note: the first constant, A, has to be adjusted by 12 hours */
-/* because the UT1 is supplied as a Julian date, which begins  */
-/* at noon.                                                    */
-
-   double d1, d2, t, f, gmst;
-
-
-/* Julian centuries since fundamental epoch. */
-   if (dj1 < dj2) {
-      d1 = dj1;
-      d2 = dj2;
-   } else {
-      d1 = dj2;
-      d2 = dj1;
-   }
-   t = (d1 + (d2 - ERFA_DJ00)) / ERFA_DJC;
-
-/* Fractional part of JD(UT1), in seconds. */
-   f = ERFA_DAYSEC * (fmod(d1, 1.0) + fmod(d2, 1.0));
-
-/* GMST at this UT1. */
-   gmst = eraAnp(ERFA_DS2R * ((A + (B + (C + D * t) * t) * t) + f));
-
-   return gmst;
-
-}
-/*----------------------------------------------------------------------
-**  
-**  
-**  Copyright (C) 2013-2014, 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.
-**  
-*/