WFC3 TV3 Testing: UVIS Window Contamination

Computer Science – Performance

Scientific paper

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Hubble Space Telescope, Hst, Space Telescope Science Institute, Wide Field Camera 3, Wfc3, Thermal Vacuum Testing, Uvis Flight Detector

Scientific paper

During the most recent WFC3 thermal vacuum (TV) testing campaign, it was discovered that the outer window of the UVIS flight detector (UVIS-1- ) is contaminated. The contamination appears to be the mineral residue of an earlier condensation event which has been traced to a period of acceptance testing at Ball Aerospace. These features have been dubbed "droplets" due to their appearance at the time of discovery. We characterized the impact of these features on UVIS channel performance with a series of tests using both point source and flat-field illumination. In large-aperture (10 pixel radius) photometry of point sources stepped across a strong window feature, the feature does not significantly increase the photometric scatter. For small-aperture (3 pixel radius) photometry of point sources stepped across a strong window feature, the photometric scatter increases from ~0.5% to ~1%, with little to no mitigation via flat-fielding, because light in the core of the point spread function is redirected to the near wings. However, the effect of these droplets can be mitigated through appropriate dithering of observations.

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