Some examples and notes on GWFish from LGWA Workshop

This is the second Review Project course for Masters.

Yuri Levin's website

Searches for nontensorial gravitational waves from known pulsars

Analysis pipeline capable of searching for dark compact objects in the Milky Way through astrometric lensing in real or mock Gaia DR4 data.

Semi-analytic Solvers for Two-component General-relativistic Spherically Symmetric Stars

routines for computing neutron star structure and evolution

Collection of codes for general relativistic magnetohydrodynamics simulations. This includes an extension of the IllinoisGRMHD code (to allow the use of finite temperature EOS tables), along with several supporting codes which work within the EinsteinToolkit and Cactus infrastructure. Also included are several examples for running BNS merger sims.

Supplementary material for the paper "The UTMOST pulsar timing programme I: Overview and first results".

Supplementary material for the paper "Constraints on wide-band radiative changes after a glitch in PSR J1452-6036".

Constructs neutron star models in the context of regularized 4D Einstein-Gauss-Bonnet gravity, using the KEH/CST numerical scheme.

Fourth Open Gravitational-wave Catalog of Compact Binary Mergers (4-OGC). Using the data from LIGO and Virgo from 2015-2020, a comprehensive catalog including 94 detected mergers (90 BBH, 2 BNS, 2 NSBH) and sub-threshold candidates throughout O1, O2, O3a, and O3b..

Code and results for the disruption of axion miniclusters (AMCs) in the Milky Way, as well as radio signals from encounters between AMCs and neutrons stars.

Tesi triennale sulla ricerca del post merger di segnali di onda gravitazionale

Python codes for modeling the physics of neutron starts. The coupled differential equations describing the equation of state and the structural model is solved. Comparison between the classical model and the relativistic model (Tolman-Oppenheimer-Volkov equation) is shown.

Data release for the BBH / BNS search of single-detector LIGO data during O1 and O2.