STIS Cycle 17 MAMA Dark Monitor

Details STIS Cycle 17 MAMA Dark Monitor STIS Cycle 17 MAMA Dark Monitor

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11857p&link_type=abstract

HST Proposal ID #11857. Cycle 17

Physics

Scientific paper

This proposal monitors the behavior of the dark current in each of the MAMA detectors. The basic monitor takes two 1380s ACCUM darks each week with each detector. The weekly pairs of exposures for each detector are linked so that they are taken at opposite ends of the same SAA free interval. This pairing of exposures will make it easier to separate long and short term temporal variability from temperature dependent changes. For the FUV MAMA darks, additional exposures are taken once every six months. These are groups of six 1314 s FUV-MAMA TIME-TAG darks distributed over a 6 to 7 orbit interval during the same SAA free interval. This will give more information on the brightness of the FUV MAMA dark current as a function of the amount of time that the HV has been on.;

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