Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO

The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration)

doi:10.3847/1538-4365/acdc9f

Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO

The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration)

Applied Mathematics and Statistics

California Institute of Technology
Institute of Science Tokyo
University of Salerno
National Institute for Nuclear Physics
Monash University
Pennsylvania State University
University of Wisconsin-Milwaukee
Louisiana State University
Australian National University
Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
Leibniz University Hannover
Inter-University Centre for Astronomy and Astrophysics India
University of Cambridge
Instituto Nacional de Pesquisas Espaciais
Cardiff University
Tata Institute of Fundamental Research
National Astronomical Observatory of Japan (NAOJ)
University of Turin
University of Glasgow
University of Western Australia
Université Savoie Mont Blanc
University of Naples Federico II
University of Minnesota Twin Cities
Maastricht University
National Institute for Subatomic Physics
Université libre de Bruxelles
University of California at Riverside
Université Paris-Saclay
The University of Tokyo
University of Barcelona
ICREA
Gran Sasso Science Institute
University of Udine
Embry-Riddle Aeronautical University
Université Côte d'Azur
National and Kapodistrian University of Athens
University of Camerino
American University Washington DC

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270 Scopus citations

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.

Original language	English
Article number	29
Journal	Astrophysical Journal, Supplement Series
Volume	267
Issue number	2
DOIs	https://doi.org/10.3847/1538-4365/acdc9f
State	Published - Aug 1 2023

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10.3847/1538-4365/acdc9f

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@article{6f348feec210405f8a8af1b0d8c690a4,

title = "Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO",

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.",

author = "\{The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration)\} and R. Abbott and H. Abe and F. Acernese and K. Ackley and S. Adhicary and N. Adhikari and Adhikari, \{R. X.\} and Adkins, \{V. K.\} and Adya, \{V. B.\} and C. Affeldt and D. Agarwal and M. Agathos and Aguiar, \{O. D.\} and L. Aiello and A. Ain and P. Ajith and T. Akutsu and S. Albanesi and Alfaidi, \{R. A.\} and A. Al-Jodah and C. All{\'e}n{\'e} and A. Allocca and M. Almualla and Altin, \{P. A.\} and A. Amato and L. Amez-Droz and A. Amorosi and S. Anand and A. Ananyeva and R. Andersen and Anderson, \{S. B.\} and Anderson, \{W. G.\} and M. Andia and M. Ando and T. Andrade and N. Andres and M. Andr{\'e}s-Carcasona and T. Andri{\'c} and S. Ansoldi and Antelis, \{J. M.\} and S. Antier and M. Aoumi and T. Apostolatos and Appavuravther, \{E. Z.\} and S. Appert and Apple, \{S. K.\} and K. Arai and A. Araya and Araya, \{M. C.\} and C. Markakis",

note = "Publisher Copyright: {\textcopyright} 2023. The Author(s). Published by the American Astronomical Society.",

year = "2023",

month = aug,

day = "1",

doi = "10.3847/1538-4365/acdc9f",

language = "English",

volume = "267",

journal = "Astrophysical Journal, Supplement Series",

issn = "0067-0049",

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T1 - Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO

AU - The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration)

AU - Abbott, R.

AU - Abe, H.

AU - Acernese, F.

AU - Ackley, K.

AU - Adhicary, S.

AU - Adhikari, N.

AU - Adhikari, R. X.

AU - Adkins, V. K.

AU - Adya, V. B.

AU - Affeldt, C.

AU - Agarwal, D.

AU - Agathos, M.

AU - Aguiar, O. D.

AU - Aiello, L.

AU - Ain, A.

AU - Ajith, P.

AU - Akutsu, T.

AU - Albanesi, S.

AU - Alfaidi, R. A.

AU - Al-Jodah, A.

AU - Alléné, C.

AU - Allocca, A.

AU - Almualla, M.

AU - Altin, P. A.

AU - Amato, A.

AU - Amez-Droz, L.

AU - Amorosi, A.

AU - Anand, S.

AU - Ananyeva, A.

AU - Andersen, R.

AU - Anderson, S. B.

AU - Anderson, W. G.

AU - Andia, M.

AU - Ando, M.

AU - Andrade, T.

AU - Andres, N.

AU - Andrés-Carcasona, M.

AU - Andrić, T.

AU - Ansoldi, S.

AU - Antelis, J. M.

AU - Antier, S.

AU - Aoumi, M.

AU - Apostolatos, T.

AU - Appavuravther, E. Z.

AU - Appert, S.

AU - Apple, S. K.

AU - Arai, K.

AU - Araya, A.

AU - Araya, M. C.

AU - Markakis, C.

PY - 2023/8/1

Y1 - 2023/8/1

N2 - 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.

AB - 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.

UR - https://www.scopus.com/pages/publications/85172242508

U2 - 10.3847/1538-4365/acdc9f

DO - 10.3847/1538-4365/acdc9f

M3 - Article

AN - SCOPUS:85172242508

SN - 0067-0049

VL - 267

JO - Astrophysical Journal, Supplement Series

JF - Astrophysical Journal, Supplement Series

IS - 2

M1 - 29

ER -

Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO

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