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slalib/subet.f
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83
slalib/subet.f
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SUBROUTINE sla_SUBET (RC, DC, EQ, RM, DM)
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*+
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* - - - - - -
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* S U B E T
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* - - - - - -
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*
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* Remove the E-terms (elliptic component of annual aberration)
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* from a pre IAU 1976 catalogue RA,Dec to give a mean place
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* (double precision)
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*
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* Given:
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* RC,DC dp RA,Dec (radians) with E-terms included
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* EQ dp Besselian epoch of mean equator and equinox
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*
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* Returned:
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* RM,DM dp RA,Dec (radians) without E-terms
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*
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* Called:
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* sla_ETRMS, sla_DCS2C, sla_,DVDV, sla_DCC2S, sla_DRANRM
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*
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* Explanation:
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* Most star positions from pre-1984 optical catalogues (or
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* derived from astrometry using such stars) embody the
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* E-terms. This routine converts such a position to a
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* formal mean place (allowing, for example, comparison with a
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* pulsar timing position).
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*
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* Reference:
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* Explanatory Supplement to the Astronomical Ephemeris,
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* section 2D, page 48.
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*
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* P.T.Wallace Starlink 10 May 1990
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*
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* Copyright (C) 1995 Rutherford Appleton Laboratory
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*
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* License:
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* This program is free software; you can redistribute it and/or modify
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* it under the terms of the GNU General Public License as published by
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* the Free Software Foundation; either version 2 of the License, or
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* (at your option) any later version.
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*
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* This program is distributed in the hope that it will be useful,
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* but WITHOUT ANY WARRANTY; without even the implied warranty of
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* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
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* GNU General Public License for more details.
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*
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* You should have received a copy of the GNU General Public License
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* along with this program (see SLA_CONDITIONS); if not, write to the
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* Free Software Foundation, Inc., 59 Temple Place, Suite 330,
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* Boston, MA 02111-1307 USA
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*
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*-
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IMPLICIT NONE
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DOUBLE PRECISION RC,DC,EQ,RM,DM
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DOUBLE PRECISION sla_DRANRM,sla_DVDV
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DOUBLE PRECISION A(3),V(3),F
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INTEGER I
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* E-terms
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CALL sla_ETRMS(EQ,A)
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* Spherical to Cartesian
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CALL sla_DCS2C(RC,DC,V)
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* Include the E-terms
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F=1D0+sla_DVDV(V,A)
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DO I=1,3
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V(I)=F*V(I)-A(I)
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END DO
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* Cartesian to spherical
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CALL sla_DCC2S(V,RM,DM)
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* Bring RA into conventional range
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RM=sla_DRANRM(RM)
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END
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