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Institut für Astronomie und AstrophysikAbteilung AstronomieSand 1, D-72076 Tübingen, Germany |
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WCS_GETPOLE
Compute the coordinates of the native pole for a non-polar projection
For non-polar (cylindrical or conic) projections, the native pole is
not at the reference point, and WCS_GETPOLE is used to determine the
position of the native pole. See section 2.4 of the paper
"Representation of Celestial Coordinates in FITS" by Calabretta
Greisen (2002, A&A, 395, 1077, also available at
http://www.aoc.nrao.edu/~egreisen Called by WCS_ROTATE
WCS_GETPOLE, crval, lonpole, theta0, alpha_p, delta_p, LATPOLE= ]
crval - 2 element vector containing standard system coordinates (the
longitude and latitude) of the reference point in degrees
lonpole - native longitude of the celestial North Pole (degrees)
theta0 - native latitude of the fiducial point
alpha_p, delta_p - celestial longitude and latitude of the native pole
(degrees)
LATPOLE - native latitude of the celestial North Pole (degrees)
Written W. Landsman June, 2003
Fix calculation when theta0 is not 0 or 90 February 2004
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