6. Fit PSF Map to Extracted Stars

Command: wisp-fit-source-extracted-psf-map

Important Parameters

• srcextract-psfmap-terms

The various systematics removal steps in the pipeline can make use of information about the shape of stars in the images (a.k.a. PRF). That can come from two sources: the find stars step as part of the process fits for a PRF model, and obviously the PSF/PRF fitting step does as well. At the moment, the latter does not produce summary information (e.g. full-width at half maximum, ellpticity, etc.). Furthermore, in many applications, the PSF/PRF fitting step is too computationally expensive, and so it is replaced with a dummy fit. The result is that presently we rely on information from the find stars step.

Fitting the PRF of each individual star (as the find stars step does) results in quite noisy estimated parameters. In order to reduce that noise, this step of the pipeline fits a smooth function of image position and possibly stellar properties (brightness, color, etc. from the catalog) to each of the relevant parameters. Because the fit is based on a large number of stars, the noise gets averaged out to a large extent. The map is then evaluated for each star to produce higher-quality estimates of the PRF parameters.

The step is accomplished by the wisp-fit-source-extracted-psf-map command.