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/* |
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*+ |
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* Name: |
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* palPreces |
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* Purpose: |
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* Precession - either FK4 or FK5 as required. |
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* Language: |
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* Starlink ANSI C |
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12
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* Type of Module: |
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* Library routine |
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15
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* Invocation: |
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* void palPreces ( const char sys[3], double ep0, double ep1, |
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* double *ra, double *dc ); |
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* Arguments: |
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* sys = const char [3] (Given) |
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* Precession to be applied: FK4 or FK5. Case insensitive. |
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* ep0 = double (Given) |
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* Starting epoch. |
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* ep1 = double (Given) |
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* Ending epoch |
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* ra = double * (Given & Returned) |
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* On input the RA mean equator & equinox at epoch ep0. On exit |
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* the RA mean equator & equinox of epoch ep1. |
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* dec = double * (Given & Returned) |
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* On input the dec mean equator & equinox at epoch ep0. On exit |
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* the dec mean equator & equinox of epoch ep1. |
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* Description: |
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* Precess coordinates using the appropriate system and epochs. |
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36
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* Authors: |
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* PTW: Patrick T. Wallace |
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* TIMJ: Tim Jenness (JAC, Hawaii) |
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* {enter_new_authors_here} |
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* Notes: |
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* - Uses palPrec for FK5 data and palPrebn for FK4 data. |
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* - The epochs are Besselian if SYSTEM='FK4' and Julian if 'FK5'. |
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* For example, to precess coordinates in the old system from |
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* equinox 1900.0 to 1950.0 the call would be: |
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* palPreces( "FK4", 1900.0, 1950.0, &ra, &dc ); |
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* - This routine will NOT correctly convert between the old and |
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* the new systems - for example conversion from B1950 to J2000. |
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* For these purposes see palFk425, palFk524, palFk45z and |
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* palFk54z. |
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* - If an invalid SYSTEM is supplied, values of -99D0,-99D0 will |
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* be returned for both RA and DC. |
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53
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54
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* History: |
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* 2012-03-02 (TIMJ): |
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* Initial version |
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57
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* Adapted with permission from the Fortran SLALIB library. |
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* {enter_further_changes_here} |
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60
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* Copyright: |
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* Copyright (C) 1995 Rutherford Appleton Laboratory |
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* Copyright (C) 2012 Science and Technology Facilities Council. |
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* All Rights Reserved. |
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65
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* Licence: |
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* This program is free software; you can redistribute it and/or |
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67
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* modify it under the terms of the GNU General Public License as |
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68
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* published by the Free Software Foundation; either version 3 of |
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69
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* the License, or (at your option) any later version. |
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70
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* |
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71
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* This program is distributed in the hope that it will be |
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72
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* useful, but WITHOUT ANY WARRANTY; without even the implied |
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73
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* warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR |
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74
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* PURPOSE. See the GNU General Public License for more details. |
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75
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* |
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76
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* You should have received a copy of the GNU General Public License |
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77
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* along with this program; if not, write to the Free Software |
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78
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* Foundation, Inc., 51 Franklin Street, Fifth Floor, Boston, |
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79
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* MA 02110-1301, USA. |
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80
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81
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* Bugs: |
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82
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* {note_any_bugs_here} |
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83
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*- |
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84
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*/ |
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85
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86
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#if HAVE_CONFIG_H |
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87
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# include |
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#endif |
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89
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90
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#include "pal.h" |
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91
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#include "pal1sofa.h" |
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92
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93
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#include |
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94
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95
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#if HAVE__STRNICMP || defined(_WIN32) || defined(_WIN64) |
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96
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# define strncasecmp _strnicmp |
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#endif |
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98
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99
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2
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void palPreces ( const char sys[3], double ep0, double ep1, |
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100
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double *ra, double *dc ) { |
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101
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102
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double pm[3][3]; |
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103
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double v1[3]; |
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104
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double v2[3]; |
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105
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106
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/* Generate appropriate precession matrix */ |
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107
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2
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50
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if ( strncasecmp( "FK4", sys, 3 ) == 0 ) { |
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108
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2
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palPrebn( ep0, ep1, pm ); |
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109
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0
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0
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} else if (strncasecmp( "FK5", sys, 3 ) == 0 ) { |
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110
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0
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palPrec( ep0, ep1, pm ); |
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111
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} else { |
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112
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0
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*ra = -99.0; |
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113
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0
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*dc = -99.0; |
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114
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0
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return; |
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115
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} |
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116
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117
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/* Convert RA,Dec to x,y,z */ |
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118
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2
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eraS2c( *ra, *dc, v1 ); |
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119
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120
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/* Precess */ |
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121
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2
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eraRxp( pm, v1, v2 ); |
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122
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123
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/* Back to RA,Dec */ |
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124
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2
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eraC2s( v2, ra, dc ); |
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125
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2
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*ra = eraAnp( *ra ); |
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126
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} |