update ast 8.6.2

1 files changed, 0 insertions, 151 deletions

diff --git a/ast/erfa/pr00.c b/ast/erfa/pr00.c
deleted file mode 100644
index 0cdf7d3..0000000
--- a/ast/erfa/pr00.c
+++ /dev/null
@@ -1,151 +0,0 @@
-#include "erfa.h"
-
-void eraPr00(double date1, double date2, double *dpsipr, double *depspr)
-/*
-**  - - - - - - - -
-**   e r a P r 0 0
-**  - - - - - - - -
-**
-**  Precession-rate part of the IAU 2000 precession-nutation models
-**  (part of MHB2000).
-**
-**  Given:
-**     date1,date2    double  TT as a 2-part Julian Date (Note 1)
-**
-**  Returned:
-**     dpsipr,depspr  double  precession corrections (Notes 2,3)
-**
-**  Notes:
-**
-**  1) 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.
-**
-**  2) The precession adjustments are expressed as "nutation
-**     components", corrections in longitude and obliquity with respect
-**     to the J2000.0 equinox and ecliptic.
-**
-**  3) Although the precession adjustments are stated to be with respect
-**     to Lieske et al. (1977), the MHB2000 model does not specify which
-**     set of Euler angles are to be used and how the adjustments are to
-**     be applied.  The most literal and straightforward procedure is to
-**     adopt the 4-rotation epsilon_0, psi_A, omega_A, xi_A option, and
-**     to add dpsipr to psi_A and depspr to both omega_A and eps_A.
-**
-**  4) This is an implementation of one aspect of the IAU 2000A nutation
-**     model, formally adopted by the IAU General Assembly in 2000,
-**     namely MHB2000 (Mathews et al. 2002).
-**
-**  References:
-**
-**     Lieske, J.H., Lederle, T., Fricke, W. & Morando, B., "Expressions
-**     for the precession quantities based upon the IAU (1976) System of
-**     Astronomical Constants", Astron.Astrophys., 58, 1-16 (1977)
-**
-**     Mathews, P.M., Herring, T.A., Buffet, B.A., "Modeling of nutation
-**     and precession   New nutation series for nonrigid Earth and
-**     insights into the Earth's interior", J.Geophys.Res., 107, B4,
-**     2002.  The MHB2000 code itself was obtained on 9th September 2002
-**     from ftp://maia.usno.navy.mil/conv2000/chapter5/IAU2000A.
-**
-**     Wallace, P.T., "Software for Implementing the IAU 2000
-**     Resolutions", in IERS Workshop 5.1 (2002).
-**
-**  Copyright (C) 2013-2016, NumFOCUS Foundation.
-**  Derived, with permission, from the SOFA library.  See notes at end of file.
-*/
-{
-   double t;
-
-/* Precession and obliquity corrections (radians per century) */
-   static const double PRECOR = -0.29965 * ERFA_DAS2R,
-                       OBLCOR = -0.02524 * ERFA_DAS2R;
-
-
-/* Interval between fundamental epoch J2000.0 and given date (JC). */
-   t = ((date1 - ERFA_DJ00) + date2) / ERFA_DJC;
-
-/* Precession rate contributions with respect to IAU 1976/80. */
-   *dpsipr = PRECOR * t;
-   *depspr = OBLCOR * t;
-
-   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.
-**  
-*/