Star-field identification algorithm

Details Star-field identification algorithm Star-field identification algorithm

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993optl...18q.399s&link_type=abstract

Optics Letters (ISSN 0146-9592), vol. 18, no. 6, p. 399-401

Physics

Optics

Algorithms, Fault Tolerance, Pattern Recognition, Star Distribution, Astronomical Coordinates, Errors, Real Time Operation, Reference Stars, Stellar Magnitude

Scientific paper

This paper describes the development of a real-time, six-feature algorithm for all-sky star-field identification, which takes into account faulty input data, reference table errors, and systematic errors induced by instruments. An oriented star triplet defined by the visual magnitudes, celestial coordinates, and three stars is the minimum identifiable star pattern element.

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