UVIS Cycle 17 Contamination Monitor

Details UVIS Cycle 17 Contamination Monitor UVIS Cycle 17 Contamination Monitor

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11907b&link_type=abstract

HST Proposal ID #11907. Cycle 17

Physics

Scientific paper

The UV throughput of WFC3 during Cycle 17 is monitored via weekly
standard star observations in a subset of key filters covering 200-600nm
and F606W, F814W as controls on the red end. The data will provide a
measure of throughput levels as a function of time and wavelength,
allowing for detection of the presence of possible contaminants.;

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