Predicted Countrates for the UV WFC3 Calibration Subsystem using Deuterium Lamps

Details Predicted Countrates for the UV WFC3 Calibration Subsystem using Deuterium Lamps Predicted Countrates for the UV WFC3 Calibration Subsystem using Deuterium Lamps

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004wfc..rept....7b&link_type=abstract

Instrument Science Report WFC3 2004-07, 10 pages

Computer Science

Hubble Space Telescope, Hst, Space Telescope Science Institute, Wide Field Camera 3, Wfc3, Calibration Subsystem, Deuterium Lamps

Scientific paper

Predicted WFC3 calibration subsystem countrates have been computed for a number of candidate deuterium (D2) lamps. Based on the calibration system component throughput estimates from Ball, the detector curves from the GSFC Detector Characterization Lab (DCL), and the lamp spectra measured at GSFC, use of any of the lamps in the calibration subsystem should provide sufficient flux to satisfy the CEI specification of 16.7 e-/s/pix in all filters blueward of and including F390N. This report summarizes the various lamps available and provides details of the procedure used for deriving the estimated countrates.

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