GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
journal contribution
posted on 2023-05-21, 11:37 authored by Abbott, BP, Abbott, R, Karelle SiellezKarelle Siellez, Zweizig, J, Boyle, M, Hemberger, D, Kidder, LE, Lovelace, G, Ossokine, S, Scheel, M, Szilagi, B, Teukolsky, SWe report the observation of a gravitational-wave signal produced by the coalescence of two stellar-mass black holes. The signal, GW151226, was observed by the twin detectors of the Laser Interferometer Gravitational-Wave Observatory (LIGO) on December 26, 2015 at 03:38:53 UTC. The signal was initially identified within 70 s by an online matched-filter search targeting binary coalescences. Subsequent off-line analyses recovered GW151226 with a network signal-to-noise ratio of 13 and a significance greater than 5σ.
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Publication title
Physical Review LettersVolume
116Issue
24Article number
241103Number
241103Pagination
1-14ISSN
0031-9007Department/School
School of Natural SciencesPublisher
American Physical SocPlace of publication
One Physics Ellipse, College Pk, USA, Md, 20740-3844Rights statement
© 2016 American Physical Society. This article is available under the terms of the Creative Commons Attribution 3.0 Unported (CC BY 3.0) License (https://creativecommons.org/licenses/by/3.0/). Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI.Socio-economic Objectives
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