The normal HST engineering telemetry data from 13,979 acquisitions on 4882 stars have been processed. The FGS guidance data can reveal duplicity with separations ranging from approximately 30 mas, for the brighter stars, with small magnitude differences, up to the neighborhood of 500 mas, and in some cases to 1000 mas. The fraction of guide stars indicating duplicity is a function of the statistical criteria used, but is over 5% at a very high level of confidence. It is possible that if some some of the brighter and closer pairs could be identified as nearby, that their orbital motions would be rapid enough to allow mass and distance determination on the time scale of a decade if followed with ground-based interferometric and spectroscopic instruments.
A brief catalog of doubles is given, nearly all of which are of
certain duplicity. Information for accessing on-line catalogs of large
numbers of stars with lesser, but nevertheless strong, probabilities
of duplicity and also for the solutions for duplicity from all acquisitions
is provided.
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