Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/140384
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Type: Journal article
Title: Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO
Author: Abbott, R.
Abe, H.
Acernese, F.
Ackley, K.
Adhicary, S.
Adhikari, N.
Adhikari, R.X.
Adkins, V.K.
Adya, V.B.
Affeldt, C.
Agarwal, D.
Agathos, M.
Aguiar, O.D.
Aiello, L.
Ain, A.
Ajith, P.
Akutsu, T.
Albanesi, S.
Alfaidi, R.A.
Al-Jodah, A.
et al.
Citation: Astrophysical Journal Supplement Series, 2023; 267(2):29-1-29-28
Publisher: American Astronomical Society
Issue Date: 2023
ISSN: 0067-0049
1538-4365
Statement of
Responsibility: 
The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration : R. Abbott ... D. Beniwal ... G. N. Bolingbroke ... D. D. Brown ... H. Cao ... A. A. Ciobanu ... A. Grado ... Z. J. Holmes ... K. Jenner ... J. Munch ... S. Muusse ... S. W. S. Ng ... D. J. Ottaway ..., M. Pathak ... T. J. Roocke ..., M. G. Schiworski ... H. Takeda ... T. Tanaka ... P. J. Veitch ... et al.
Abstract: The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in 2019 April and lasting six months, O3b starting in 2019 November and lasting five months, and O3GK starting in 2020 April and lasting two weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org. The main data set, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages.
Keywords: Gravitational wave astronomy; Experimental data
Rights: © 2023. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
DOI: 10.3847/1538-4365/acdc9f
Grant ID: ARC
Published version: http://dx.doi.org/10.3847/1538-4365/acdc9f
Appears in Collections:Physics publications

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