FGS3 Red Transfer Function Reference Calibration

Details FGS3 Red Transfer Function Reference Calibration FGS3 Red Transfer Function Reference Calibration

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7681n&link_type=abstract

HST Proposal ID #7681

Astronomy and Astrophysics

Astronomy

Hst Proposal Id #7681

Scientific paper

The purpose of this proposal is to obtain red reference Transfer Functions through the PUPIL, CLEAR and NEUTRAL DENSITY filters at the center of the fov of FGS #3 {the astrometer}. These Transfer Functions will be used to deduce the presence of secondary stars in multiple systems, and to calibrate the non-zero angular diameter of extended sources.

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