Universal relations for neutron stars refer to parameter connections between macroscopic stellar quantities that exhibit a remarkable insensitivity to the underlying stellar core microphysics, which is parametrized through the equation of state (EoS). These relations...
An advanced MCMC sampler with the capability to run with parallel tempering, multiple model types, and unknown counts within each model type using Reversible Jump MCMC techniques. One of the main applications is parameter estimation for gravitational wave sources....
Bilby (Bayesian Inference Library) is an open-source Python package designed to perform Bayesian parameter estimation and model selection for gravitational-wave (GW) signals. It offers a flexible, modular, and user-friendly framework that allows researchers to analyze...
B-pop is a modular, Python-based software package designed to generate realistic populations of binary compact objects—such as binary neutron stars (BNS), neutron star–black hole binaries (NSBH), and binary black holes (BBH)—for use in gravitational-wave (GW)...
GWFish is a flexible, open-source software package designed to perform Fisher matrix–based forecasts for gravitational-wave (GW) detector networks. Its primary purpose is to evaluate the expected performance of current and future GW observatories in estimating source...
