COS/NUV Detector Dark Monitor
Abstract
Perform routine monitoring of NUV MAMA detector dark rate. The main purpose is \nto look for evidence of a change in the dark rate, both to track on-orbit time \ndependence and to check for a detector problem developing. Variations of count rates \nas a function of orbital positions will be analyzed to study the effect of SAA. \nStacked images will help us study the spatial distribution of dark rates on the detector.
- Publication:
-
HST Proposal
- Pub Date:
- November 2018
- Bibcode:
- 2018hst..prop15538M