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kslong edited this page May 29, 2017
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This project contains the S/W needed to estimate persistence in the WFC3/IR detector. The S/W, or a version of it, is used at STScI to create data products available from the HST Archive in MAST.
Note: The master branch for this S/W is the version of the S/W that is being used now for producing the products in MAST. The dev branch however is the one that those who are interested in the latest features, and/or modifying the S/W should begin with.
The master branch works only under version 2.7 of Python, whereas the dev branch is compatible with version 2.7 and 3.4. The code is being developed and is normally run in the astroconda environment. There are no iraf/pyaf dependencies on the dev branch.