-
MIT
- Cambridge, MA, USA
- http://space.mit.edu/home/guenther/
- https://orcid.org/0000-0003-4243-2840
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Starred repositories
This code creates the stellar activity grid for exoplanets
⚡ Fast 1D and 2D histogram functions in Python ⚡
Working repository for gPhoton v2 development.
RISE: "Live" Reveal.js JupyterLab Slideshow Extension
sbi is a Python package for simulation-based inference, designed to meet the needs of both researchers and practitioners. Whether you need fine-grained control or an easy-to-use interface, sbi has …
Watch a Sphinx directory and rebuild the documentation when a change is detected. Also includes a hot-reload web server.
🏆 A ranked list of awesome python developer tools and libraries. Updated weekly.
Python 3.8+ toolbox for submitting jobs to Slurm
pySAS is a python wrapper for the Science Analysis Software (SAS) used for analyzing XMM-Newton data. This repository is maintained by the XMM-Newton Guest Observer Facility (GOF) at Goddard Space …
A template for communities to create a custom Code of Conduct and enforcement procedures.
Log-norm temp distribution of APEC plasmas fitted with BXA
OpenSSF Scorecard - Security health metrics for Open Source
Ziggy, a portable, scalable infrastructure for science data processing pipelines, is the child of the Transiting Exoplanet Survey Satellite (TESS) pipeline and the grandchild of the Kepler Pipeline.
Democratising Archival X-ray Astronomy (DAXA) is an easy-to-use Python module for downloading multi-mission X-ray telescope data and processing it into usable archives. Users can acquire entire arc…
Manifold Markov chain Monte Carlo methods in Python
A modular X-ray spectral-timing astronomy modelling package
Jupyter-friendly Python interface for C++ MINUIT2
SAOImage DS9 is an astronomical imaging and data visualization application.
fit solar system small body multiple systems with non-Keplerian orbits including quadrupole shapes
Subtract H I Lyman-alpha and O I airglow emission from HST-COS G130M spectra and reconstruct stellar emission profiles.
Code for fitting the attenuated Lyman alpha profiles of nearby low-mass stars.