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authorWilliam Joye <wjoye@cfa.harvard.edu>2019-05-10 15:55:01 (GMT)
committerWilliam Joye <wjoye@cfa.harvard.edu>2019-05-10 15:55:01 (GMT)
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upgrade ast 8.7.1
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-#include "erfa.h"
-
-void eraG2icrs ( double dl, double db, double *dr, double *dd )
-/*
-** - - - - - - - - - -
-** e r a G 2 i c r s
-** - - - - - - - - - -
-**
-** Transformation from Galactic Coordinates to ICRS.
-**
-** Given:
-** dl double galactic longitude (radians)
-** db double galactic latitude (radians)
-**
-** Returned:
-** dr double ICRS right ascension (radians)
-** dd double ICRS declination (radians)
-**
-** Notes:
-**
-** 1) The IAU 1958 system of Galactic coordinates was defined with
-** respect to the now obsolete reference system FK4 B1950.0. When
-** interpreting the system in a modern context, several factors have
-** to be taken into account:
-**
-** . The inclusion in FK4 positions of the E-terms of aberration.
-**
-** . The distortion of the FK4 proper motion system by differential
-** Galactic rotation.
-**
-** . The use of the B1950.0 equinox rather than the now-standard
-** J2000.0.
-**
-** . The frame bias between ICRS and the J2000.0 mean place system.
-**
-** The Hipparcos Catalogue (Perryman & ESA 1997) provides a rotation
-** matrix that transforms directly between ICRS and Galactic
-** coordinates with the above factors taken into account. The
-** matrix is derived from three angles, namely the ICRS coordinates
-** of the Galactic pole and the longitude of the ascending node of
-** the galactic equator on the ICRS equator. They are given in
-** degrees to five decimal places and for canonical purposes are
-** regarded as exact. In the Hipparcos Catalogue the matrix
-** elements are given to 10 decimal places (about 20 microarcsec).
-** In the present ERFA function the matrix elements have been
-** recomputed from the canonical three angles and are given to 30
-** decimal places.
-**
-** 2) The inverse transformation is performed by the function eraIcrs2g.
-**
-** Called:
-** eraAnp normalize angle into range 0 to 2pi
-** eraAnpm normalize angle into range +/- pi
-** eraS2c spherical coordinates to unit vector
-** eraTrxp product of transpose of r-matrix and p-vector
-** eraC2s p-vector to spherical
-**
-** Reference:
-** Perryman M.A.C. & ESA, 1997, ESA SP-1200, The Hipparcos and Tycho
-** catalogues. Astrometric and photometric star catalogues
-** derived from the ESA Hipparcos Space Astrometry Mission. ESA
-** Publications Division, Noordwijk, Netherlands.
-**
-** Copyright (C) 2013-2016, NumFOCUS Foundation.
-** Derived, with permission, from the SOFA library. See notes at end of file.
-*/
-{
- double v1[3], v2[3];
-
-/*
-** L2,B2 system of galactic coordinates in the form presented in the
-** Hipparcos Catalogue. In degrees:
-**
-** P = 192.85948 right ascension of the Galactic north pole in ICRS
-** Q = 27.12825 declination of the Galactic north pole in ICRS
-** R = 32.93192 longitude of the ascending node of the Galactic
-** plane on the ICRS equator
-**
-** ICRS to galactic rotation matrix, obtained by computing
-** R_3(-R) R_1(pi/2-Q) R_3(pi/2+P) to the full precision shown:
-*/
- double r[3][3] = { { -0.054875560416215368492398900454,
- -0.873437090234885048760383168409,
- -0.483835015548713226831774175116 },
- { +0.494109427875583673525222371358,
- -0.444829629960011178146614061616,
- +0.746982244497218890527388004556 },
- { -0.867666149019004701181616534570,
- -0.198076373431201528180486091412,
- +0.455983776175066922272100478348 } };
-
-
-/* Spherical to Cartesian. */
- eraS2c(dl, db, v1);
-
-/* Galactic to ICRS. */
- eraTrxp(r, v1, v2);
-
-/* Cartesian to spherical. */
- eraC2s(v2, dr, dd);
-
-/* Express in conventional ranges. */
- *dr = eraAnp(*dr);
- *dd = eraAnpm(*dd);
-
-/* 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.
-**
-*/