SWarp: Resampling and Co-adding FITS Images Together

Details SWarp: Resampling and Co-adding FITS Images Together SWarp: Resampling and Co-adding FITS Images Together

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ascl.soft10068b&link_type=abstract

Astrophysics Source Code Library, record ascl:1010.068

Astronomy and Astrophysics

Astrophysics

Scientific paper

SWarp is a program that resamples and co-adds together FITS images using any arbitrary astrometric projection defined in the WCS standard. It operates on pre-reduced images and their weight-maps. Based on the astrometric and photometric calibrations derived at an earlier phase of the pipeline, SWarp re-maps ("warps") the pixels to a perfect projection system, and co-adds them in an optimum way, according to their relative weights. SWarp's astrometric engine is based on a customized version of Calabretta's WCSLib 2.6 and supports all of the projections defined in the 2000 version of the WCS proposal.

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