1 #include "erfa.h"
2 
eraAtcc13(double rc,double dc,double pr,double pd,double px,double rv,double date1,double date2,double * ra,double * da)3 void eraAtcc13(double rc, double dc,
4                double pr, double pd, double px, double rv,
5                double date1, double date2,
6                double *ra, double *da)
7 /*
8 **  - - - - - - - - - -
9 **   e r a A t c c 1 3
10 **  - - - - - - - - - -
11 **
12 **  Transform a star's ICRS catalog entry (epoch J2000.0) into ICRS
13 **  astrometric place.
14 **
15 **  Given:
16 **     rc     double   ICRS right ascension at J2000.0 (radians, Note 1)
17 **     dc     double   ICRS declination at J2000.0 (radians, Note 1)
18 **     pr     double   RA proper motion (radians/year, Note 2)
19 **     pd     double   Dec proper motion (radians/year)
20 **     px     double   parallax (arcsec)
21 **     rv     double   radial velocity (km/s, +ve if receding)
22 **     date1  double   TDB as a 2-part...
23 **     date2  double   ...Julian Date (Note 3)
24 **
25 **  Returned:
26 **     ra,da  double*  ICRS astrometric RA,Dec (radians)
27 **
28 **  Notes:
29 **
30 **  1) Star data for an epoch other than J2000.0 (for example from the
31 **     Hipparcos catalog, which has an epoch of J1991.25) will require a
32 **     preliminary call to eraPmsafe before use.
33 **
34 **  2) The proper motion in RA is dRA/dt rather than cos(Dec)*dRA/dt.
35 **
36 **  3) The TDB date date1+date2 is a Julian Date, apportioned in any
37 **     convenient way between the two arguments.  For example,
38 **     JD(TDB)=2450123.7 could be expressed in any of these ways, among
39 **     others:
40 **
41 **            date1          date2
42 **
43 **         2450123.7           0.0       (JD method)
44 **         2451545.0       -1421.3       (J2000 method)
45 **         2400000.5       50123.2       (MJD method)
46 **         2450123.5           0.2       (date & time method)
47 **
48 **     The JD method is the most natural and convenient to use in cases
49 **     where the loss of several decimal digits of resolution is
50 **     acceptable.  The J2000 method is best matched to the way the
51 **     argument is handled internally and will deliver the optimum
52 **     resolution.  The MJD method and the date & time methods are both
53 **     good compromises between resolution and convenience.  For most
54 **     applications of this function the choice will not be at all
55 **     critical.
56 **
57 **     TT can be used instead of TDB without any significant impact on
58 **     accuracy.
59 **
60 **  Called:
61 **     eraApci13    astrometry parameters, ICRS-CIRS, 2013
62 **     eraAtccq     quick catalog ICRS to astrometric
63 **
64 **  This revision:   2021 April 18
65 **
66 **  Copyright (C) 2013-2021, NumFOCUS Foundation.
67 **  Derived, with permission, from the SOFA library.  See notes at end of file.
68 */
69 {
70 /* Star-independent astrometry parameters */
71    eraASTROM astrom;
72 
73    double w;
74 
75 
76 /* The transformation parameters. */
77    eraApci13(date1, date2, &astrom, &w);
78 
79 /* Catalog ICRS (epoch J2000.0) to astrometric. */
80    eraAtccq(rc, dc, pr, pd, px, rv, &astrom, ra, da);
81 
82 /* Finished. */
83 
84 }
85 /*----------------------------------------------------------------------
86 **
87 **
88 **  Copyright (C) 2013-2021, NumFOCUS Foundation.
89 **  All rights reserved.
90 **
91 **  This library is derived, with permission, from the International
92 **  Astronomical Union's "Standards of Fundamental Astronomy" library,
93 **  available from http://www.iausofa.org.
94 **
95 **  The ERFA version is intended to retain identical functionality to
96 **  the SOFA library, but made distinct through different function and
97 **  file names, as set out in the SOFA license conditions.  The SOFA
98 **  original has a role as a reference standard for the IAU and IERS,
99 **  and consequently redistribution is permitted only in its unaltered
100 **  state.  The ERFA version is not subject to this restriction and
101 **  therefore can be included in distributions which do not support the
102 **  concept of "read only" software.
103 **
104 **  Although the intent is to replicate the SOFA API (other than
105 **  replacement of prefix names) and results (with the exception of
106 **  bugs;  any that are discovered will be fixed), SOFA is not
107 **  responsible for any errors found in this version of the library.
108 **
109 **  If you wish to acknowledge the SOFA heritage, please acknowledge
110 **  that you are using a library derived from SOFA, rather than SOFA
111 **  itself.
112 **
113 **
114 **  TERMS AND CONDITIONS
115 **
116 **  Redistribution and use in source and binary forms, with or without
117 **  modification, are permitted provided that the following conditions
118 **  are met:
119 **
120 **  1 Redistributions of source code must retain the above copyright
121 **    notice, this list of conditions and the following disclaimer.
122 **
123 **  2 Redistributions in binary form must reproduce the above copyright
124 **    notice, this list of conditions and the following disclaimer in
125 **    the documentation and/or other materials provided with the
126 **    distribution.
127 **
128 **  3 Neither the name of the Standards Of Fundamental Astronomy Board,
129 **    the International Astronomical Union nor the names of its
130 **    contributors may be used to endorse or promote products derived
131 **    from this software without specific prior written permission.
132 **
133 **  THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
134 **  "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
135 **  LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS
136 **  FOR A PARTICULAR PURPOSE ARE DISCLAIMED.  IN NO EVENT SHALL THE
137 **  COPYRIGHT HOLDER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT,
138 **  INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING,
139 **  BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES;
140 **  LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER
141 **  CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT
142 **  LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN
143 **  ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE
144 **  POSSIBILITY OF SUCH DAMAGE.
145 **
146 */
147