Core package to analyze gravitational-wave data, find signals, and study their parameters. This package was used in the first direct detection of gravitational waves (GW150914), and is used in the ongoing analysis of LIGO/Virgo data.

a python package for gravitational wave analysis with the F-statistic

An open-source package for neutron star whole workflow Bayesian inference constraining Neutron star EOS package

Python package for solving TOV equation and calculating tidal properties

Shell scripts for spectral-timing analysis of X-ray astronomical data.

Localization of gravitational-wave transients. Mirror of https://git.ligo.org/lscsoft/ligo.skymap

This will be the first official public release of the VItamin code base. VItamin is a python package for producing fast gravitational wave posterior samples.

A library for the Physics of Neutron Stars

Mitigation of periodic as well as narrow-band and spiky/bursty RFI from time-domain filterbank data.

A python package for Bayesian inference of gravitational-wave data

High-performance C++ framework for gamma-ray burst afterglow modeling with Python bindings. Features fast multi-wavelength light curve generation, MCMC parameter inference, and advanced physics models including shock dynamics, radiation mechanisms, and structured jets. Designed for computational efficiency and scientific workflow integration.

Second Open Gravitational-wave Catalog of Compact Binary Mergers. Parameter estimates for O1 and O2 mergers. Sub-threshold BNS/NSBH/BBH candidates.

First Open Gravitational-wave Catalog of Compact Binary Mergers from Advanced LIGO's first observing run.

Third Open Gravitational-wave Catalog of Compact Binary Mergers. Using the data from LIGO and Virgo from 2015-2019, a comprehensive catalog including 57 detected mergers (55 BBH, 2 BNS) and sub-threshold candidates throughout O1, O2, and O3a.

Search for Binary Supernova Ejected OB-type Runaway Stars from Young Open Clusters | Master Thesis Project

A program that automates the data retrieval and data reduction of observational data gathered by NASA's NICER x-ray mission

Constructs neutron star models in the context of Damour-Esposito-Farese (DEF) scalar tensor theory and R^2 gravity model.

Predictions for LISA detectable BH and NS binaries - Wagg et al. (2022)

An implementation of realistic, finite-temperature nuclear-matter models in neutron-star seismology.

Here is a Julia script to solve the TOV equations and calculate (Mass, Radius, and Tidal Deformability).