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A&A 395, 1061-1075 (2002)
DOI: 10.1051/0004-6361:20021326
Representations of world coordinates in FITS
E. W. Greisen1 and M. R. Calabretta21 National Radio Astronomy Observatory, PO Box O, Socorro, NM 87801-0387, USA
2 Australia Telescope National Facility, PO Box 76, Epping, NSW 1710, Australia
(Received 24 July 2002 / Accepted 9 September 2002)
Abstract
The initial descriptions of the FITS format provided a simplified
method for describing the physical coordinate values of the image
pixels, but deliberately did not specify any of the detailed
conventions required to convey the complexities of actual image
coordinates. Building on conventions in wide use within astronomy,
this paper proposes general extensions to the original methods for
describing the world coordinates of FITS data. In subsequent
papers, we apply these general conventions to the methods by which
spherical coordinates may be projected onto a two-dimensional plane
and to frequency/wavelength/velocity coordinates.
Key words: methods: data analysis -- techniques: image processing -- astronomical data bases: miscellaneous
Offprint request: E. W. Greisen, egreisen@nrao.edu
© ESO 2002
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