Performance of the star field identification algorithm in the observatory environment

Details Performance of the star field identification algorithm in the observatory environment Performance of the star field identification algorithm in the observatory environment

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994spie.2209..522s&link_type=abstract

Proc. SPIE Vol. 2209, p. 522-533, Space Optics 1994: Earth Observation and Astronomy, M. G. Cerutti-Maori; Philippe Roussel; Eds

Physics

Optics

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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