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The Guide Star Selection System and the Guide Star Catalog for Space Telescope

Published online by Cambridge University Press:  04 August 2017

Jane L. Russell
Jane L. Russell*
Affiliation:
Space Telescope Science Institute Homewood Campus Baltimore, MD 21218

Abstract

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The Guide Star Selection System (GSSS) will provide relative positions of two guide stars and the target for each observation of the Space Telescope as well as photometry for the guide stars. Being developed at the Space Telescope Science Institute, the GSSS is a production system which is based on PDS measurements of Schmidt survey plates. The specified accuracy for the system is +/−0.33 arcsec for the separation of the guide stars and 0.4 mag in the bandpass of the Space Telescope's Fine Guidance Sensors. The GSSS will produce two catalogs which will be used in the operation of the system. The Guide Star Photometry catalog includes photoelectric measurements (+/−0.05 mag) in B and V for six stars over the guide star range, 9.0 to 14.5 visual magnitude, near the central part of each 6 by 6 deg survey plate. The Guide Star Catalog will include the list of all possible guide stars and brighter, positions (at least +/−1 arcsec) and magnitudes (at least +/−0.4 mag) for essentially the whole sky complete to visual magnitude 15.

Type
VIII. Objects
Information
Symposium - International Astronomical Union , Volume 109: Astrometric Techniques , 1986 , pp. 721 - 727
Copyright
Copyright © Reidel 1986 

References

Kinsey, J.H., Denman, R.J., and Evzerov, A. (1984) “Laser Interferometer enhanced Positional Precision of a Scanning Microdensitometer for Astrometric Plate Scanning,” Rev. of Sci. Instr., December.CrossRefGoogle Scholar
Lutz, R.K. (1979) “An Algorithm for the Real Time Analysis of Digitized Images,” Computer Journal, 23, 262–9.Google Scholar
Russell, J. L. and Williams, C.A. (1986) “Testing Schmidt Plates for Astrometric Purposes,” Proceedings of IAU Colloquium 109 on Astrometric Techniques, ed. by Eichhorn, H. K. CrossRefGoogle Scholar
Sanders, W. L., and Schroeder, R., (1980) “Membership in the Open Cluster NGC 6494,” Astron. and Astrophys. 88, 102–107.Google Scholar