Stars
A pythonic interface for radio astronomy interferometry data (uvfits, measurement sets, uvh5, others)
VIPCALs is a fully automated calibration pipeline for Very Long Baseline Interferometry (VLBI) data. It was developed as part of the SMILE (Search for Milli-Lenses) project to process thousands of …
Create HTCondor DAGs and submit files for radio astronomy cube imaging
Replace zsh's default completion selection menu with fzf!
A collaborative note taking, wiki and documentation platform that scales. Built with Django and React.
Book repository for The Turing Way: a how to guide for reproducible, ethical and collaborative data science
This is an implementation of Segmentation based Radio Frequency Intereference (RFI) mitigation.
Repository for the scripts that were used to benchmark the parallel imaging performance using tclean within CASA 6
This is the port of the VLA pipeline from CASA 5.x to 6.x by @autocorr to which polarization calibration has been added in by @ksand017
[NeurIPS 2024] Depth Anything V2. A More Capable Foundation Model for Monocular Depth Estimation
Concatenate multiple channel images into a single FITS cube
A library of algorithms for aperture synthesis radio telescopes
Label line using matplotlib.
JAX bindings to the Flatiron Institute Non-uniform Fast Fourier Transform (FINUFFT) library
[CVPR 2024] Depth Anything: Unleashing the Power of Large-Scale Unlabeled Data. Foundation Model for Monocular Depth Estimation
Friends don't let friends make certain types of data visualization - What are they and why are they bad.
A python package to make realistic simulations of ALMA observations of galaxies and point sources.
ALminer: ALMA archive mining and visualization toolkit
[ECCV 2024 Best Paper Candidate & TPAMI 2025] PointLLM: Empowering Large Language Models to Understand Point Clouds
nway -- Bayesian cross-matching of astronomical catalogues
Repo to hold all the analysis and cube generation script for MIGHTEE-pol
Density EstimatioN using Masked AutoRegressive Flow
Mock spatially resolved spectral line observations of simulated galaxies.