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diff --git a/math/slalib/doc/fk5hz.hlp b/math/slalib/doc/fk5hz.hlp new file mode 100644 index 00000000..4d5e5ab0 --- /dev/null +++ b/math/slalib/doc/fk5hz.hlp @@ -0,0 +1,54 @@ +.help fk5hz Jun99 "Slalib Package" +.nf + + SUBROUTINE slF5HZ (R5,D5,EPOCH,RH,DH) + + - - - - - - + F 5 H Z + - - - - - - + + Transform an FK5 (J2000) star position into the frame of the + Hipparcos catalogue, assuming zero Hipparcos proper motion. + + (double precision) + + This routine converts a star position from the FK5 system to + the Hipparcos system, in such a way that the Hipparcos proper + motion is zero. Because such a star has, in general, a non-zero + proper motion in the FK5 system, the routine requires the epoch + at which the position in the FK5 system was determined. + + Given: + R5 d FK5 RA (radians), equinox J2000, epoch EPOCH + D5 d FK5 Dec (radians), equinox J2000, epoch EPOCH + EPOCH d Julian epoch (TDB) + + Returned (all Hipparcos): + RH d RA (radians) + DH d Dec (radians) + + Called: slDS2C, slDAVM, slDIMV, slDMXV, slDC2S + + Notes: + + 1) The FK5 to Hipparcos transformation consists of a pure + rotation and spin; zonal errors in the FK5 catalogue are + not taken into account. + + 2) The published orientation and spin components are interpreted + as "axial vectors". An axial vector points at the pole of the + rotation and its length is the amount of rotation in radians. + + 3) See also slFK5H, slHFK5, slHF5Z. + + Reference: + + M.Feissel & F.Mignard, Astron. Astrophys. 331, L33-L36 (1998). + + P.T.Wallace Starlink 7 October 1998 + + Copyright (C) 1998 Rutherford Appleton Laboratory + Copyright (C) 1995 Association of Universities for Research in Astronomy Inc. + +.fi +.endhelp |