It takes an UFTI observation comprising four object frames and a dark frame to make a calibrated, untrimmed mosaic automatically. Photometry of the point source using a fixed 5-arcsecond aperture is calculated for each jitter frame and the mosaic. The analysis of each star is appended to this file. This recipe works well for faint sources in moderately crowded fields. The flat field is created by combining normalised object frames using the median at each pixel.
Registration is performed using common point sources in the overlap regions.
If the recipe cannot identify sufficient common objects, the script resorts to using the telescope offsets transformed to pixels. The resampling applies non-integer shifts of origin using bilinear interpolation. There is no rotation to align the Cartesian axes with the cardinal directions. The recipe makes the mosaics by applying offsets in intensity to give the most consistent result amongst the overlapping regions. The mosaic is not trimmed to the dimensions of a single frame, thus the noise will be greater in the peripheral areas having received less exposure time.