CSM Mapping of the UVIS Field-of-View

Details CSM Mapping of the UVIS Field-of-View CSM Mapping of the UVIS Field-of-View

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008wfc..rept...45b&link_type=abstract

Instrument Science Report WFC3 2008-45, 3 pages

Computer Science

Hubble Space Telescope, Hst, Space Telescope Science Institute, Wfc3, Wide Field Camera 3, Channel Select Mechanism, Uvis

Scientific paper

UVIS channel flat field images obtained as a function of CSM position have been used to determine the fraction of the WFC3/UVIS field-of-view that is obscured by the CSM when it is in an off-nominal position. The total range of CSM travel between the nominal UVIS and IR channel positions is 330 resolver steps. The UVIS field-of-view is 50% obscured when the CSM reaches 45% of its total travel from the UVIS to IR positions and becomes completely obscured with the CSM at and beyond 75-80% of the distance to the IR position.

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