Institut für Astronomie und AstrophysikAbteilung AstronomieWaldhäuser Str. 64, D-72076 Tübingen, Germany |
GSSSXYAD
Convert (X,Y) coordinates in a STScI Guide Star image to RA and Dec
The sky coordinates may be printed and/or returned in variables.
GSSSxyad, gsa, x, y, ra, dec, [ /PRINT ]
GSA - The GSSS Astrometry structure extracted from a FITS header by GSSSEXTAST X - The X pixel coordinate(s) of the image, scalar or vector Y - The Y pixel coordinate(s) of the image, scalar or vector
RA - The RA coordinate of the given pixel(s) in *degrees* DEC - The DEC coordinate of the given pixel(s) in *degrees* Both RA and Dec will be returned as double precision
/PRINT - If this keyword is set and non-zero, then coordinates will be displayed at the terminal
Given a FITS header,hdr, from a GSSS image, print the astronomical coordinates of (X,Y) = (200.23, 100.16) at the terminal IDL> GSSSExtast, hdr, gsa ;Extract astrometry structure IDL> GSSSxyad, gsa, 200.23, 100.16, /print
For most purpose users can simply use XYAD, which will call GSSSXYAD if it is passed a GSSS header.
ASTDISP - print RA, Dec in a standard format
01-JUL-90 Version 1 written by Eric W. Deutsch Vectorized Code W. Landsman March, 1991 14-AUG-91 Fixed error which caused returned RA and DEC to be off by -.5 pixels in both X,Y. Now X,Y follows same protocol as ADXY. 20-AUG-91 Modified to use AstDisp procedure. June 94 Added /PRINT keyword instead of PRFLAG W. Landsman June 94 Converted to IDL V5.0 W. Landsman September 1997 29-JUN-99 Added support for AMD[X,Y]1[2-3] for DSS images by E. Deutsch
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