Monitor the Temporal Stability of the Fgs's AST-SV-7

Details Monitor the Temporal Stability of the Fgs's AST-SV-7 Monitor the Temporal Stability of the Fgs's AST-SV-7

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1418j&link_type=abstract

HST Proposal ID #1418

Physics

Hst Proposal Id #1418

Scientific paper

The goal of these measurements is to monitor the internal positional stability of the FGSs by measuring a few stars in "check fields" repeatedly during the SV period. The results of these measurements are the stability characteristics of the FGS to allow an estimate of the frequency of OFAD re-calibrations. NOW USES WvA positions for PROX and ref frame. 910920 Modified 910920 by F. Benedict to 1) observe Proxima Cen starting 920201 2) do either FGS 1 or FGS 3 THIS IS AN FGS 3 TEST Modified 8 Feb 92 to remove v=16.25 target and change pupil to F583W.

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