Monitor the Long-Term Stability of FGS 3

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

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7677n&link_type=abstract

HST Proposal ID #7677

Physics

Hst Proposal Id #7677

Scientific paper

The goal of these measurements is to monitor the internal positional stability of FGS3 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 FGS3 which allow an estimate of differential corrections to OFAD and Plate Scale. This is an ecliptic field. During each of two primary orientations, we will obtain observations 3 times per M35 observing season {fall and spring}.

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