The Gravitational Wave Universe Toolbox: A software package to simulate observation of the Gravitational Wave Universe with different detectors
Shu-Xu Yi, Gijs Nelemans, Christiaan Brinkerink, Zuzanna, Kostrzewa-Rutkowska, Sjoerd T. Timmer, Fiorenzo Stoppa, Elena M. Rossi, Simon, F. Portegies Zwart

TL;DR
The GW-Toolbox is a versatile software package that simulates gravitational wave observations across various detectors and source types, aiding researchers in quickly assessing detection prospects and measurement uncertainties.
Contribution
It introduces a comprehensive, user-friendly tool that integrates multiple detectors and source populations for gravitational wave observation simulation, with accessible web and Python interfaces.
Findings
Consistent results with detailed calculations for various source classes.
Supports multiple current and future GW detectors.
Provides an accessible platform for GW observation simulation.
Abstract
Context. As the importance of Gravitational Wave (GW) Astrophysics increases rapidly, astronomers in different fields and with different backgrounds can have the need to get a quick idea of which GW source populations can be detected by which detectors and with what measurement uncertainties. Aims. The GW-Toolbox is an easy-to-use, flexible tool to simulate observations on the GW universe with different detectors, including ground-based interferometers (advanced LIGO, advanced VIRGO, KAGRA, Einstein Telescope, and also customised designs), space-borne interferometers (LISA and a customised design), pulsar timing arrays mimicking the current working ones (EPTA, PPTA, NANOGrav, IPTA) and future ones. We include a broad range of sources such as mergers of stellar mass compact objects, namely black holes, neutron stars and black hole-neutron stars; and supermassive black hole binaries…
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