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Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
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ADXY
Use a FITS header to convert astronomical to pixel coordinates
Use an image header to compute X and Y positions, given the
RA and Dec (or longitude, latitude) in decimal degrees.
ADXY, HDR ;Prompt for Ra and DEC
ADXY, hdr, a, d, x, y, [ /PRINT, ALT= ]
HDR - FITS Image header containing astrometry parameters
A - Right ascension in decimal DEGREES, scalar or vector
D - Declination in decimal DEGREES, scalar or vector
If A and D are not supplied, user will be prompted to supply
them in either decimal degrees or HR,MIN,SEC,DEG,MN,SC format.
X - row position in pixels, same number of elements as A and D
Y - column position in pixels
X and Y will be in standard IDL convention (first pixel is 0) and not
the FITS convention (first pixel is 1). As in FITS an integral
value corresponds to the center of a pixel.
/PRINT - If this keyword is set and non-zero, then results are displayed
at the terminal.
ALT - single character 'A' through 'Z' or ' ' specifying an alternate
astrometry system present in the FITS header. The default is
to use the primary astrometry or ALT = ' '. If /ALT is set,
then this is equivalent to ALT = 'A'. See Section 3.3 of
Greisen & Calabretta (2002, A&A, 395, 1061) for information about
alternate astrometry keywords.
If less than 5 parameters are supplied, or if the /PRINT keyword is
set, then the X and Y positions are displayed at the terminal.
If the procedure is to be used repeatedly with the same header,
then it would be faster to use AD2XY.
AD2XY, ADSTRING(), EXTAST, GETOPT(), TEN()
W. Landsman HSTX January, 1988
Use astrometry structure W. Landsman January, 1994
Changed default ADSTRING format W. Landsman September, 1995
Converted to IDL V5.0 W. Landsman September 1997
Check if latitude/longitude reversed in CTYPE keyword W. L. Feb. 2004
Added ALT keyword W. Landsman September 2004
Work for non-spherical coordinate transformation W. Landsman May 2005
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