Blue TF Calibration

Details Blue TF Calibration Blue TF Calibration

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996hst..prop.6922h&link_type=abstract

HST Proposal ID #6922

Astronomy and Astrophysics

Astronomy

Hst Proposal Id #6922

Scientific paper

The purpose of this proposal is to obtain blue reference TFs 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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