Pixel-based CTI-correction for HST/STIS CCD data
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Updated
Apr 16, 2024 - Python
Pixel-based CTI-correction for HST/STIS CCD data
This repository contains the S/W used by STScI to estimate persistence in WFC3/IR images
Simulation of WFC3 observations
The Illustris Virtual Observatory is an expanded iteration of the Sunpy module(ptorrey) for creating synthetic SDSS, HST, or JWST images of galaxies from the Illustris simulation. For instructions on how to install/use this program, please go to this address:
Package for making superdarks and superbiases for STIS CCD data
📈🐳Converts Forex historical data to different formats via GitHub Actions
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.
Zeus21: Lightning-fast simulations of cosmic dawn
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