WFC3 Data Handbook V. 4.0

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10.3	UVIS Scanned Images

For UVIS data, use the flt.fits which contains all the nominal instrumental calibrations (bias, dark, and flat) just as for staring-mode observations. At press time, we are not aware of any publications detailing a custom analysis of spatially-scanned UVIS data; such analyses are under development by the investigators of HST programs 12588/13464, 12685, 12879/13344, 12909, etc.