FOC Point-Spread Function Monitoring - Cycle 4

Details FOC Point-Spread Function Monitoring - Cycle 4 FOC Point-Spread Function Monitoring - Cycle 4

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5762j&link_type=abstract

HST Proposal ID #5762

Computer Science

Hst Proposal Id #5762

Scientific paper

This proposal will image a UV standard star in the F/96 mode in order to monitor the point-spread function of the HST-COSTAR-FOC channel. Data will be taken every 5-7 weeks, following a planned COSTAR DOB move to ensure that the FOC keeps pace with desorption. The COSTAR DOB and COSTAR FOC lines can be used as generic SUs to plug in whenever such adjustments are needed (e.g. to compensate for secondary mirror moves).

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