Simulation of WFC3 observations
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Updated
Apr 21, 2019 - Python
Simulation of WFC3 observations
Python tools for HST WFC3 data calibration and analysis
PACMAN is a pipeline to reduce and analyze data collected by Hubble Wide Field Camera 3 (HST/WFC3) using either the G102 or G141 grism.
Pipeline and SQL database interface for the Hubble WFC3/UVIS charge transfer efficiency (CTE) monitor.
This repository contains the S/W used by STScI to estimate persistence in WFC3/IR images
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