All-sky search for long-duration gravitational-wave transients in the first part of the fourth LIGO-Virgo-KAGRA observing run

Authors

• A. G. Abac
• I. Abouelfettouh
• F. Acernese
• Teviet Creighton, The University of Texas Rio Grande ValleyFollow
• Mario C. Diaz, The University of Texas Rio Grande ValleyFollow
• Raul A. Espinosa, The University of Texas Rio Grande Valley
• J. Lawrence, The University of Texas Rio Grande Valley
• Francisco Llamas Villarreal, The University of Texas Rio Grande Valley
• Soma Mukherjee, The University of Texas Rio Grande ValleyFollow
• Volker Quetschke, The University of Texas Rio Grande ValleyFollow
• Miriam Ramos Arevalo, The University of Texas Rio Grande ValleyFollow
• Wenhui Wang, The University of Texas Rio Grande Valley

Document Type

Article

Publication Date

4-27-2026

Abstract

We present an all-sky search for long-duration gravitational waves (GWs) from the first part of the LIGO-Virgo-KAGRA fourth observing run (O4), called O4a and comprising data taken between May 24, 2023, and January 16, 2024. The GW signals targeted by this search are the so-called “long-duration” ( ≳1  s) transients expected from a variety of astrophysical processes, including nonaxisymmetric deformations in magnetars or eccentric binary coalescences. We make minimal assumptions on the emitted GW waveforms in terms of morphologies and durations. Overall, our search targets signals with durations of ∼1–1000  s and frequency content in the range 16–2048 Hz. In the absence of significant detections, we report the sensitivity limits of our search in terms of root-sum-square signal amplitude (ℎrss) of reference waveforms. These limits improve upon the results from the third LIGO-Virgo-KAGRA observing run (O3) by about 30% on average. Moreover, this analysis demonstrates substantial progress in our ability to search for long-duration GW signals owing to enhancements in pipeline detection efficiencies. As detector sensitivities continue to advance and observational runs grow longer, unmodeled long-duration searches will increasingly be able to explore a range of compelling astrophysical scenarios involving neutron stars and black holes.

Comments

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.

Recommended Citation

LIGO Scientific Collaboration, Virgo Collaboration, and KAGRA Collaboration, A. G. Abac, I. Abouelfettouh, et al. “All-Sky Search for Long-Duration Gravitational-Wave Transients in the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run.” Physical Review D 113, no. 8 (2026): 082004. https://doi.org/10.1103/83j3-pgk1.  

Creative Commons License

This work is licensed under a Creative Commons Attribution 4.0 International License.

Publication Title

Physical Review D

DOI

10.1103/83j3-pgk1