GHRS Sensitivity Monitor -- Cycle 3

Details GHRS Sensitivity Monitor -- Cycle 3 GHRS Sensitivity Monitor -- Cycle 3

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993hst..prop.5041s&link_type=abstract

HST Proposal ID #5041

Physics

Hst Proposal Id #5041

Scientific paper

This proposal defines the long term sensitivity monitoring program for the Goddard High Resolution Spectrograph. It uses three UV standard stars, BD+28d4211, and BD+75d325. 1) BD+28d4211 will be the long term standard, and will allow cross-calibration with FOS. 2) BD+75d325 will provide backup during SMOV and will be observed as a close-out in Cycle 3. 3) AGK+81d266 will be observed to provide a baseline for the SMOV focus test. The exposure times are short and the medium resolution gratings will be used with the LSA.

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