FOC F/48 Point Spread Function - Cycle 2

Details FOC F/48 Point Spread Function - Cycle 2 FOC F/48 Point Spread Function - Cycle 2

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.4236p&link_type=abstract

HST Proposal ID #4236

Other

Hst Proposal Id #4236

Scientific paper

The aim is to obtain ST/FOC instrumental point spread functions (PSFs) to facilitate the restoration of science data obtained through the f/96 optical relay. The structure of the PSF has to be measured with high photometric accuracy, otherwise it is not possible to discriminate the fine structure present in the PSF, from fine structure that may be intrinsic to the astronomical object itself.

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