Dark Count Statistics for GHRS Detectors

Details Dark Count Statistics for GHRS Detectors Dark Count Statistics for GHRS Detectors

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.4012l&link_type=abstract

HST Proposal ID #4012

Physics

Hst Proposal Id #4012

Scientific paper

The proposed observations will obtain the statistical data needed to plan an operational strategy for observing faint targets with the GHRS. The proposed test involves only the use of Side 2, since only this side of the GHRS can benefit from the results of this test at the present time. Because of the loss of the GHRS low-resolution mode (G140L), many observing programs that had originally specified G140L have been changed to use G160M. Hence, the problem of reducing the GHRS dark-count becomes even more acute. The proposed tests should give us the information needed to evaluate by how much the dark-count can be reduced by the appropriate operational strategy (see Question 3).

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