Stellar Flux Monitor Proposal

Details Stellar Flux Monitor Proposal Stellar Flux Monitor Proposal

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3173w&link_type=abstract

HST Proposal ID #3173

Computer Science

Hst Proposal Id #3173

Scientific paper

THE PURPOSE OF THIS TEST IS TO MONITOR THE THROUGHPUT AND PSF OF THE WF AND PC IN THE UV AND VISIBLE. Six exposures in six filters in both the WF and PC are taken of a UV flux standard star. The total duration is two orbits. The program should be repeated every four weeks. Along with the internal monitor program, this stellar monitor comprises the regular monitoring program for the throughput and focus of the WFPC and should start to be scheduled when the initial calibration programs cease, that is, in late Mar. or April 1991.

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