Cosmic-ray Identification Step

The cosmic rays and bad pixels are now identified by comparing the input images with the associated blotted,median-cleaned images created.

drizzlepac.drizCR Module

Mask blemishes in dithered data by comparison of an image with a model image and the derivative of the model image.

Authors:

Warren Hack

License:

License

Functions

rundrizCR(imgObjList, configObj[, procSteps])	Execute the driz_cr cosmic-ray rejection step.
drizCR([input, configObj, editpars])	The blotted median images that are now transformed back into the original reference frame, get compared to the original input images to detect any spurious pixels (which may include pixels impacted by cosmic rays) in each input.