Monitor the Long-Term Stability of FGS 3 Revised

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

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.5118j&link_type=abstract

HST Proposal ID #5118

Astronomy and Astrophysics

Astronomy

Hst Proposal Id #5118

Scientific paper

THIS PROPOSAL CONTAINS A SUBSET OF THE LONG-TERM STABILITY TEST. THIS PROPOSAL IS NOT TO BE RUN ON THE SPACECRAFT IN THIS FORM. THE TARGET LIST AND EXPOSURE LOGSHEET CONTAIN THE ASTROMETRYPART OF THIS TEST. THE REMAINDER OF THE PROPOSAL IS ADUMMY TO ALLOW IT TO PASS THROUGH RPSS VALIDATION. 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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