WFC3 SMOV PROGRAM 11452: UVIS Flat Field Uniformity

Details WFC3 SMOV PROGRAM 11452: UVIS Flat Field Uniformity WFC3 SMOV PROGRAM 11452: UVIS Flat Field Uniformity

Nov 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009wfc..rept...19s&link_type=abstract

Instrument Science Report WFC3 2009-19, 13 pages

Computer Science

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

Scientific paper

The quality of the six ground-based TV3 WFC3/UVIS flat-fields F225W, F275W, F336W, F438W, F606W and F814W, used in the standard calibration of the WFC3/UVIS data, has been analyzed by comparing the magnitude of several stars on different positions of the detector. We find a difference of 1.5% to 4.5% between the ground-based flat-fields and the on-orbit data, with higher uncertainties at shorter wavelengths.

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