Star-field identification algorithm in the observatory environment

Marija S. Scholl

doi:10.1117/12.255191

21 October 1996 Star-field identification algorithm in the observatory environment

Marija S. Scholl

Proceedings Volume 2817, Infrared Spaceborne Remote Sensing IV; (1996) https://doi.org/10.1117/12.255191
Event: SPIE's 1996 International Symposium on Optical Science, Engineering, and Instrumentation, 1996, Denver, CO, United States

Abstract

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.

Citation Download Citation

Marija S. Scholl "Star-field identification algorithm in the observatory environment", Proc. SPIE 2817, Infrared Spaceborne Remote Sensing IV, (21 October 1996); https://doi.org/10.1117/12.255191

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