Monitor the Long-Term Stability of FGS 3 - Early 1996

Details Monitor the Long-Term Stability of FGS 3 - Early 1996 Monitor the Long-Term Stability of FGS 3 - Early 1996

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.6326j&link_type=abstract

HST Proposal ID #6326

Physics

Hst Proposal Id #6326

Scientific paper

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

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