GWTC-4.0: Methods for Identifying and Characterizing Gravitational-wave Transients
Publication date
2026-06-20
Authors
The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration
Editors
Advisors
Supervisors
Document Type
Article
Metadata
Show full item recordCollections
License
cc_by
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.
Keywords
Gravitational wave astronomy (675), Gravitational wave detectors (676), Gravitational wave sources (677), Neutron stars (1108), Stellar mass black holes (1611), Astronomy and Astrophysics, Space and Planetary Science
Citation
The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration 2026, 'GWTC-4.0 : Methods for Identifying and Characterizing Gravitational-wave Transients', Astrophysical Journal Letters, vol. 1004, no. 2, L21. https://doi.org/10.3847/2041-8213/ae447b