Star-field identification algorithm in the observatory environment

Details Star-field identification algorithm in the observatory environment Star-field identification algorithm in the observatory environment

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996spie.2817..288s&link_type=abstract

Proc. SPIE Vol. 2817, p. 288-298, Infrared Spaceborne Remote Sensing IV, Marija S. Scholl; Bjorn F. Andresen; Eds.

Physics

Scientific paper

A six-feature, all-sky star field identification algorithm has been developed, integrated with a CCD-based imaging camera and tested at the Table Mountain Observatory. The calibration of the CCD-based camera to minimize the error in the measured star parameters due to instrument error and experimental conditions is described. A set of observatory tests on star fields with this intelligent camera are presented.

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