| 1 | #include "slalib.h" | 
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| 2 | #include "slamac.h" | 
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| 3 | #include <ctype.h> | 
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| 4 | void slaPreces ( char sys[3], double ep0, double ep1, | 
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| 5 | double *ra, double *dc ) | 
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| 6 | /* | 
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| 7 | **  - - - - - - - - - - | 
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| 8 | **   s l a P r e c e s | 
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| 9 | **  - - - - - - - - - - | 
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| 10 | ** | 
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| 11 | **  Precession - either FK4 (Bessel-Newcomb, pre-IAU1976) or | 
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| 12 | **  FK5 (Fricke, post-IAU1976) as required. | 
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| 13 | ** | 
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| 14 | **  Given: | 
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| 15 | **     sys        char[]     precession to be applied: "FK4" or "FK5" | 
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| 16 | **     ep0,ep1    double     starting and ending epoch | 
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| 17 | **     ra,dc      double     RA,Dec, mean equator & equinox of epoch ep0 | 
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| 18 | ** | 
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| 19 | **  Returned: | 
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| 20 | **     *ra,*dc    double     RA,Dec, mean equator & equinox of epoch ep1 | 
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| 21 | ** | 
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| 22 | **  Called:    slaDranrm, slaPrebn, slaPrec, slaDcs2c, | 
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| 23 | **             slaDmxv, slaDcc2s | 
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| 24 | ** | 
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| 25 | **  Notes: | 
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| 26 | ** | 
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| 27 | **  1)  The epochs are Besselian if sys='FK4' and Julian if 'FK5'. | 
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| 28 | **      For example, to precess coordinates in the old system from | 
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| 29 | **      equinox 1900.0 to 1950.0 the call would be: | 
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| 30 | **          slaPreces ( "FK4", 1900.0, 1950.0, &ra, &dc ) | 
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| 31 | ** | 
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| 32 | **  2)  This routine will not correctly convert between the old and | 
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| 33 | **      the new systems - for example conversion from B1950 to J2000. | 
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| 34 | **      For these purposes see slaFk425, slaFk524, slaFk45z and | 
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| 35 | **      slaFk54z. | 
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| 36 | ** | 
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| 37 | **  3)  If an invalid sys is supplied, values of -99.0,-99.0 will | 
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| 38 | **      be returned for both ra and dc. | 
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| 39 | ** | 
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| 40 | **  Last revision:   22 December 1993 | 
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| 41 | ** | 
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| 42 | **  Copyright P.T.Wallace.  All rights reserved. | 
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| 43 | */ | 
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| 44 | { | 
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| 45 | double pm[3][3], v1[3], v2[3]; | 
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| 46 |  | 
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| 47 | /* Validate sys */ | 
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| 48 | if ( ( toupper ( sys[0] ) != 'F' ) | 
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| 49 | || ( toupper ( sys[1] ) != 'K' ) | 
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| 50 | || ( sys[2] != '4' && sys[2] != '5' ) ) { | 
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| 51 | *ra = -99.0;          /* Error */ | 
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| 52 | *dc = -99.0; | 
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| 53 | } else { | 
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| 54 |  | 
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| 55 | /* Generate appropriate precession matrix */ | 
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| 56 | if ( sys[2] == '4' ) | 
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| 57 | slaPrebn ( ep0, ep1, pm ); | 
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| 58 | else | 
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| 59 | slaPrec ( ep0, ep1, pm ); | 
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| 60 |  | 
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| 61 | /* Convert RA,Dec to x,y,z */ | 
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| 62 | slaDcs2c ( *ra, *dc, v1 ); | 
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| 63 |  | 
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| 64 | /* Precess */ | 
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| 65 | slaDmxv ( pm, v1, v2 ); | 
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| 66 |  | 
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| 67 | /* Back to RA,Dec */ | 
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| 68 | slaDcc2s ( v2, ra, dc ); | 
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| 69 | *ra = slaDranrm ( *ra ); | 
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| 70 | } | 
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| 71 | } | 
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