wfc3

Calibration for HST/WFC3, HST/ACS, and HST/STIS

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.

LINEAR Extraction and Modeling of Slitless Spectroscopy (mostly for WFC3/IR)

Experimenting with existing and new models for charge carrier trapping

Python API to work with aXe-style reference files stored in the HDF5 format.

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

Tools for HST reference files.

Python GUI to estimate WFC3/UVIS postflash setting