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Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
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XYXY
To use a pair of headers to convert X/Y positions from one frame
to another.
XYXY, hdra, hdrb, xa, ya, [ xb, yb ]
hdra - The header containing the plate solution describing the
frame of reference being converted FROM.
hdra - The header containing the plate solution describing the
frame of reference being converted TO.
xa - A scalar or vector containing the x coordinate(s) to convert.
ya - A scalar or vector containing the y coordinate(s) to convert.
Must have the same number of elements as 'xa'.
xb - The converted x coordinate(s). If this parameter is not
specified, it is returned through 'xa'.
yb - The converted y coordinate(s). If this parameter is not
specified, it is returned through 'ya'.
The procedures 'xyad' and 'adxy' are used to perform the
conversion. The equinoxes of each header are checked with
"get_equinox" to make sure that they are identical, and "precess"
is used if they are not. HEULER used if the headers have a different
coordinate system (e.g. Celestial, Galactic, Ecliptic)
Note that all X,Y coordinates are in the IDL convention (starting with
0,0) and not the FITS convention (first pixel is 1,1)
GET_EQUINOX(), EXTAST, XYAD, ADXY, PRECESS, HEULER
Written by Michael R. Greason, Hughes-STX, 13 April 1992.
Updated to use ASTROMETRY structures. J.D.Offenberg, HSTX, Jan 1993
Converted to IDL V5.0 W. Landsman September 1997
Check coordinate system J. Ballet/ W. Landsman April 2004
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