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Algorithm

The program uses local spherical coordinate transformations centred at the RA and DEC of each image frame. It is assumed that all the images lie in the same plane as the first image. The validity of this approximation depends on the size of the final image in degrees and the number of pixels. As a rough guide, for a 512 x 512 pixel final image it is accurate for up to a 5 degree by 5 degree field.



Next: Direction of X-axis Up: Astrometry Prev: Astrometry