Red Leak and Signal-to-NoiseEstimates for UV GrismCoating Study

Details Red Leak and Signal-to-NoiseEstimates for UV GrismCoating Study Red Leak and Signal-to-NoiseEstimates for UV GrismCoating Study

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001wfc..rept....1d&link_type=abstract

Instrument Science Report WFC3 2001-01, 12 pages

Physics

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

Scientific paper

The WFC3 UVIS (ultraviolet and visible) channel includes a grism as one of 48 spectral elements. We present the nominal pass band and signal-to-noise measurements for three grism coatings that differ in transmittance and red leak characteristics. We find that for typical slitless spectroscopy application high throughput is preferable to red leak rejection.

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