This task uses information from the previously created count image in sky coordinates to rotate the detector coordinate model particle background images produced by mosback, model swcx images produced by swcx, and model soft proton images produced by proton into images in sky coordinates. This task was part the XMMGOF esas task 2009-2021. This is a comprehensive rewrite of the original task, which was called by perl wrapper rot-im-det-sky, which was eliminated for SAS-20.
![[none]](../icons/dprev.gif){kind=icon}
