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Abstract
The Gravitational-Wave Transient Catalog (GWTC) is a collection of candidate gravitational-wave transient signals identified and characterized by the LIGO–Virgo–KAGRA Collaboration. Producing the contents of the GWTC from detector data requires complex analysis methods. These comprise techniques to model the signal; identify the transients in the data; evaluate the quality of the data and mitigate possible instrumental issues; infer the parameters of each transient; compare the data with the waveform models for compact binary coalescences; and handle the large amount of results associated with all of these different analyses. In this paper, we describe the methods employed to produce the catalog’s fourth release, GWTC-4.0, focusing on the analysis of the first part of the fourth observing run of Advanced LIGO, Advanced Virgo and KAGRA.
| Item Type: | Article |
|---|---|
| Date Type: | Publication |
| Status: | Published |
| Schools: | Schools > Physics and Astronomy |
| Additional Information: | Full author list can be seen at https://doi.org/10.3847/2041-8213/ae447b. License information from Publisher: LICENSE 1: URL: https://creativecommons.org/licenses/by/4.0/, Type: cc-by |
| Publisher: | American Astronomical Society |
| ISSN: | 2041-8205 |
| Date of First Compliant Deposit: | 25 June 2026 |
| Date of Acceptance: | 6 February 2026 |
| Last Modified: | 05 Aug 2026 01:51 |
| URI: | https://orca.cardiff.ac.uk/id/eprint/187739 |
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