Issue |
A&A
Volume 663, July 2022
|
|
---|---|---|
Article Number | A155 | |
Number of page(s) | 22 | |
Section | Numerical methods and codes | |
DOI | https://doi.org/10.1051/0004-6361/202141634 | |
Published online | 28 July 2022 |
The Gravitational Wave Universe Toolbox
A software package to simulate observations of the gravitational wave universe with different detectors*,**
1
Department of Astrophysics/IMAPP, Radboud University,
PO Box 9010,
6500 GL
Nijmegen,
The Netherlands
e-mail: sxyi@ihep.ac.cn
2
SRON, Netherlands Institute for Space Research,
Sorbonnelaan 2,
3584 CA
Utrecht, The Netherlands
3
Institute of Astronomy,
KU Leuven, Celestijnenlaan 200D,
3001
Leuven,
Belgium
4
Leiden Observatory, Leiden University,
PO Box 9513,
2300 RA
Leiden,
The Netherlands
5
Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences,
19B Yuquan Road,
Beijing
100049,
PR China
Received:
25
June
2021
Accepted:
29
March
2022
Context. As the importance of gravitational wave (GW) astrophysics increases rapidly, astronomers interested in GWs who are not experts in this field sometimes need to get a quick idea of what GW sources can be detected by certain detectors, and the accuracy of the measured parameters.
Aims. The GW-Toolbox is a set of easy-to-use, flexible tools to simulate observations of the GW universe with different detectors, including ground-based interferometers (advanced LIGO, advanced VIRGO, KAGRA, Einstein Telescope, Cosmic Explorer, and also customised interferometers), space-borne interferometers (LISA and a customised design), and pulsar timing arrays mimicking the current working arrays (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 star binaries, supermassive black hole binary mergers and inspirals, Galactic double white dwarfs in ultra-compact orbit, extreme-mass-ratio inspirals, and stochastic GW backgrounds.
Methods. We collected methods to simulate source populations and determine their detectability with various detectors. Our aim is to provide a comprehensive description of the methodology and functionality of the GW-Toolbox.
Results. The GW-Toolbox produces results that are consistent with previous findings in the literature, and the tools can be accessed via a website interface or as a Python package. In the future, this package will be upgraded with more functions.
Key words: gravitational waves / stars: neutron / stars: black holes / methods: numerical
© ESO 2022
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