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author | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
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committer | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
commit | 40e5a5811c6ffce9b0974e93cdd927cbcf60c157 (patch) | |
tree | 4464880c571602d54f6ae114729bf62a89518057 /math/slalib/subet.f | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'math/slalib/subet.f')
-rw-r--r-- | math/slalib/subet.f | 84 |
1 files changed, 84 insertions, 0 deletions
diff --git a/math/slalib/subet.f b/math/slalib/subet.f new file mode 100644 index 00000000..04ed6f9d --- /dev/null +++ b/math/slalib/subet.f @@ -0,0 +1,84 @@ + SUBROUTINE slSUET (RC, DC, EQ, RM, DM) +*+ +* - - - - - - +* S U E T +* - - - - - - +* +* Remove the E-terms (elliptic component of annual aberration) +* from a pre IAU 1976 catalogue RA,Dec to give a mean place +* (double precision) +* +* Given: +* RC,DC dp RA,Dec (radians) with E-terms included +* EQ dp Besselian epoch of mean equator and equinox +* +* Returned: +* RM,DM dp RA,Dec (radians) without E-terms +* +* Called: +* slETRM, slDS2C, sla_,DVDV, slDC2S, slDA2P +* +* Explanation: +* Most star positions from pre-1984 optical catalogues (or +* derived from astrometry using such stars) embody the +* E-terms. This routine converts such a position to a +* formal mean place (allowing, for example, comparison with a +* pulsar timing position). +* +* Reference: +* Explanatory Supplement to the Astronomical Ephemeris, +* section 2D, page 48. +* +* P.T.Wallace Starlink 10 May 1990 +* +* Copyright (C) 1995 Rutherford Appleton Laboratory +* +* License: +* This program is free software; you can redistribute it and/or modify +* it under the terms of the GNU General Public License as published by +* the Free Software Foundation; either version 2 of the License, or +* (at your option) any later version. +* +* This program is distributed in the hope that it will be useful, +* but WITHOUT ANY WARRANTY; without even the implied warranty of +* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the +* GNU General Public License for more details. +* +* You should have received a copy of the GNU General Public License +* along with this program (see SLA_CONDITIONS); if not, write to the +* Free Software Foundation, Inc., 51 Franklin Street, Fifth Floor, +* Boston, MA 02110-1301 USA +* +* Copyright (C) 1995 Association of Universities for Research in Astronomy Inc. +*- + + IMPLICIT NONE + + DOUBLE PRECISION RC,DC,EQ,RM,DM + + DOUBLE PRECISION slDA2P,slDVDV + DOUBLE PRECISION A(3),V(3),F + + INTEGER I + + + +* E-terms + CALL slETRM(EQ,A) + +* Spherical to Cartesian + CALL slDS2C(RC,DC,V) + +* Include the E-terms + F=1D0+slDVDV(V,A) + DO I=1,3 + V(I)=F*V(I)-A(I) + END DO + +* Cartesian to spherical + CALL slDC2S(V,RM,DM) + +* Bring RA into conventional range + RM=slDA2P(RM) + + END |