update ast 8.6.2

1 files changed, 0 insertions, 141 deletions

diff --git a/ast/erfa/eceq06.c b/ast/erfa/eceq06.c
deleted file mode 100644
index e1ba72d..0000000
--- a/ast/erfa/eceq06.c
+++ /dev/null
@@ -1,141 +0,0 @@
-#include "erfa.h"
-
-void eraEceq06(double date1, double date2, double dl, double db,
-               double *dr, double *dd)
-/*
-**  - - - - - - - - - -
-**   e r a E c e q 0 6
-**  - - - - - - - - - -
-**
-**  Transformation from ecliptic coordinates (mean equinox and ecliptic
-**  of date) to ICRS RA,Dec, using the IAU 2006 precession model.
-**
-**  Given:
-**     date1,date2 double TT as a 2-part Julian date (Note 1)
-**     dl,db       double ecliptic longitude and latitude (radians)
-**
-**  Returned:
-**     dr,dd       double ICRS right ascension and declination (radians)
-**
-**  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) No assumptions are made about whether the coordinates represent
-**     starlight and embody astrometric effects such as parallax or
-**     aberration.
-**
-**  3) The transformation is approximately that from ecliptic longitude
-**     and latitude (mean equinox and ecliptic of date) to mean J2000.0
-**     right ascension and declination, with only frame bias (always
-**     less than 25 mas) to disturb this classical picture.
-**
-**  Called:
-**     eraS2c       spherical coordinates to unit vector
-**     eraEcm06     J2000.0 to ecliptic rotation matrix, IAU 2006
-**     eraTrxp      product of transpose of r-matrix and p-vector
-**     eraC2s       unit vector to spherical coordinates
-**     eraAnp       normalize angle into range 0 to 2pi
-**     eraAnpm      normalize angle into range +/- pi
-**
-**  Copyright (C) 2013-2016, NumFOCUS Foundation.
-**  Derived, with permission, from the SOFA library.  See notes at end of file.
-*/
-{
-   double rm[3][3], v1[3], v2[3], a, b;
-
-
-/* Spherical to Cartesian. */
-   eraS2c(dl, db, v1);
-
-/* Rotation matrix, ICRS equatorial to ecliptic. */
-   eraEcm06(date1, date2, rm);
-
-/* The transformation from ecliptic to ICRS. */
-   eraTrxp(rm, v1, v2);
-
-/* Cartesian to spherical. */
-   eraC2s(v2, &a, &b);
-
-/* Express in conventional ranges. */
-   *dr = eraAnp(a);
-   *dd = eraAnpm(b);
-
-}
-/*----------------------------------------------------------------------
-**  
-**  
-**  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.
-**  
-*/