Monitor the Long-Term Stability of FGS 3 Still

Details Monitor the Long-Term Stability of FGS 3 Still Monitor the Long-Term Stability of FGS 3 Still

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.6325l&link_type=abstract

HST Proposal ID #6325

Physics

Hst Proposal Id #6325

Scientific paper

The goal of these measurements is to monitor the internal positional stability of the FGSs by measuring many stars in the M35 check field repeatedly over a one year period. The results of these measurements are the stability characteristics of the FGS to allow an estimate of differential corrections to OFAD and Plate Scale. This is an ecliptic field. During each of two primary orientations, we will secure observations over a 130 day span, roughly every 30 days. THIS IS AN FGS 3 TEST.

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