diff --git a/palMap.c b/palMap.c index 0b7fd44..fb7bbbc 100644 --- a/palMap.c +++ b/palMap.c @@ -43,13 +43,42 @@ * Convert star RA,Dec from mean place to geocentric apparent. * Authors: +* PTW: Patrick T. Wallace * TIMJ: Tim Jenness (JAC, Hawaii) * {enter_new_authors_here} * Notes: * - Calls palMappa and palMapqk + * - The reference systems and timescales used are IAU 2006. +* - EQ is the Julian epoch specifying both the reference frame and +* the epoch of the position - usually 2000. For positions where +* the epoch and equinox are different, use the routine palPm to +* apply proper motion corrections before using this routine. +* +* - The distinction between the required TDB and TT is always +* negligible. Moreover, for all but the most critical +* applications UTC is adequate. +* +* - The proper motions in RA are dRA/dt rather than cos(Dec)*dRA/dt. +* +* - This routine may be wasteful for some applications because it +* recomputes the Earth position/velocity and the precession- +* nutation matrix each time, and because it allows for parallax +* and proper motion. Where multiple transformations are to be +* carried out for one epoch, a faster method is to call the +* palMappa routine once and then either the palMapqk routine +* (which includes parallax and proper motion) or palMapqkz (which +* assumes zero parallax and proper motion). +* +* - The accuracy is sub-milliarcsecond, limited by the +* precession-nutation model (see palPrenut for details). +* +* - The accuracy is further limited by the routine palEvp, called +* by palMappa, which computes the Earth position and velocity. +* See iauEpv00 for details on that calculation. + * History: * 2012-03-01 (TIMJ): * Initial version @@ -57,6 +86,7 @@ * {enter_further_changes_here} * Copyright: +* Copyright (C) 2001 Rutherford Appleton Laboratory * Copyright (C) 2012 Science and Technology Facilities Council. * All Rights Reserved.