WFC3 System Throughput on the UVIS Build 2 detector

Details WFC3 System Throughput on the UVIS Build 2 detector WFC3 System Throughput on the UVIS Build 2 detector

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007wfc..rept....7b&link_type=abstract

Instrument Science Report WFC3 2007-07, 8 pages

Computer Science

Performance

Hubble Space Telescope, Hst, Space Telescope Science Institute, Wide Field Camera 3, Wfc3, Uvis Build 2

Scientific paper

The UVIS spare detector (UVIS build 2) is currently installed in WFC3 during ambient ground testing. We have performed testing of the end-to-end system throughput on the UVIS channel, and find that it performs better than expectations. The result is that the unfiltered (clear) performance of the UVIS spare detector is much closer to that of the flight detector (UVIS build 1). Comparing the 4 chips on the two detectors, chip 2 of the flight detector still offers the best performance, but the performance of the other 3 chips (chip 1 on the flight detector and chips 1 & 2 of the spare detector) are comparable. Background

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