A Joint Fermi-GBM and Swift-BAT Analysis of Gravitational-wave Candidates from the Third Gravitational-wave Observing Run

Collaboration; KAGRA Collaboration; Fermi Gamma-Ray Burst Monitor Team; The LIGO Scientific Collaboration

doi:10.3847/1538-4357/ad1eed

A Joint Fermi-GBM and Swift-BAT Analysis of Gravitational-wave Candidates from the Third Gravitational-wave Observing Run

Collaboration
, KAGRA Collaboration
, Fermi Gamma-Ray Burst Monitor Team
, The LIGO Scientific Collaboration

Universities Space Research Association
NASA Marshall Space Flight Center
University of Alabama in Huntsville
Center for Space Plasma and Aeronomic Research
Université Paris-Saclay
Politecnico di Bari
INFN Sezione di Bari
Louisiana State University
Jacobs Space Exploration Group
Florida Institute of Technology
International Space Science Institute
Max Planck Institut für Extraterrestrische Physik
University of Maryland
NASA Goddard Space Flight Center
Oskar Klein Centre
University of Alabama
Pennsylvania State University
Pennsylvania State University
University of Toronto
University of Maryland, College Park
Biochemical and Environmental Engineering
California Institute of Technology
Tokyo Institute of Technology
University of Salerno
INFN Sezione di Napoli
Monash University
University of Wisconsin-Milwaukee
Australian National University
Max-Planck-Institut fuer Gravitationsphysik
Leibniz Universität Hannover
Inter-University Centre for Astronomy and Astrophysics India
University of Cambridge
Friedrich-Schiller University
University of Birmingham
Northwestern University
Instituto Nacional de Pesquisas Espaciais
Cardiff University
Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
Tata Institute of Fundamental Research
National Astronomical Observatory
University of Turin
INFN Sezione di Torino
University of Glasgow
University of Naples Federico II
IGFL, Université de Lyon, Université Lyon 1
Astroparticule and Cosmol APC
University of Tokyo
Research Center for the Early Universe
University of Barcelona
Université Savoie Mont Blanc
Pompeu Fabra University (UPF)
Gran Sasso Science Institute
University of Strathclyde
and Physics University of Udine
INFN Sezione di Trieste
Embry-Riddle Aeronautical University, Prescott
Université Côte d'Azur
University of Amsterdam
University of Athens
INFN Sezione di Perugia
University of Camerino
American University
California State University Fullerton
European Gravitational Observatory (EGO)
College of Computing
Chennai Mathematical Institute
Hirosaki University
Columbia University
University of Portsmouth
The Graduate University for Advanced Studies
University of Urbino Carlo Bo
Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
LIGO Livingston
Sezione di Roma
University of Louvain
Science Park 105
King's College London
Korea Institute of Science and Technology Information
National Institute for Mathematical Sciences
Christopher Newport University
Universiteit Utrecht
University of Oregon
Syracuse University
University of Liège
University of Milano-Bicocca
INFN Sezione di Milano-Bicocca
INAF
LIGO Hanford
University of Salerno
Massachusetts Institute of Technology
Wigner Research Centre for Physics
University of Florida
Stanford University
University of Pisa
University of Perugia
University of Padova
INFN
Bard College
Montana State University
Institute for Plasma Research
Ghent University
Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences
University of Sannio at Benevento
The University of Adelaide
The University of Texas Rio Grande Valley
California State University-Los Angeles
University of São Paulo
Sezione di Genova
The University of Western Australia
RRCAT
Missouri University of Science and Technology
Vrije Universiteit Amsterdam
Moscow State University
Università di Trento
Trento Institute for Fundamental Physics and Applications
University of the West of Scotland
Bar-Ilan University
University of Rome
Institut FOTON-UMR6082
Indian Institute of Technology Bombay
Laboratori Nazionali del Gran Sasso
Sorbonne Université
University of Warsaw
Université de Toulouse
Villanova University
Universidade de Santiago de Compostela
Stony Brook University
Flatiron Institute
University of Genoa
Beijing Normal University
University of Melbourne
Dipartimento di Scienze Biomediche
INFN Sezione di Catania
University of Rome “Tor Vergata”
INFN Roma Tor Vergata
University of Valencia
Universität Hamburg
Rochester Institute of Technology
National Tsing Hua University
The Chinese University of Hong Kong
Fukuoka University
Charles Sturt University, Wagga Wagga
Tamkang University
National Central University
Academia Sinica, Institute Of Physics
INAF Osservatorio Astronomico di Padova
Swinburne University of Technology
Université Libre de Bruxelles
Universitat de les Illes Balears
Texas Tech University
University of Minnesota Twin Cities
University of Rhode Island
Bellevue College
Scuola Normale Superiore di Pisa
Eötvös Loránd University
Maastricht University
The University of Sheffield
University of Parma
University of Utah
Carleton College, USA
University of Zurich
Perimeter Institute for Theoretical Physics
Université de Strasbourg
West Virginia University
University of Chicago
Montclair State University
Cooperative Institute for Research in the Atmosphere
Institute of Nuclear Research ATOMKI
The University of Texas at Austin
Università degli Studi della Basilicata
Universidade de Minho
Niigata University
Osaka City University
Vanderbilt University
Xiao Hong Shan
University of Szeged
Cornell University
University of British Columbia
Osservatorio Astronomico di Capodimonte
University of Mississippi
University of Michigan, Ann Arbor
Texas A&M University
Ulsan National Institute of Science and Technology
Shanghai Astronomical Observatory Chinese Academy of Sciences
University of Toyama
University of California, Berkeley
Lancaster University
Nihon University
CCLRC Rutherford Appleton Laboratory
Chungnam National University
Aoyama Gakuin University
Tsinghua University
Aristotle University of Thessaloniki
Directorate of Construction
University of Antwerp
University of Białystok
Ewha Womans University
National Astronomical Observatories-CAS
University of Chinese Academy of Sciences
University of Southampton
University of Amsterdam
Chung-Ang University
University of Washington Bothell
Institute of Applied Physics of the Russian Academy of Sciences
Inje University
Myongji University
KEK (High Energy Accelerator Research Organization)
Institute of Mathematics of the Polish Academy of Sciences
National Centre for Nuclear Research
Instituto de Fisica Teorica
Nagoya University
Université de Montréal/Polytechnique
Université de Nice
Seoul National University
Sungkyunkwan University
Université Gustave Eiffel
University of Florence
National Cheng Kung University
Wuhan University
National Applied Research Laboratories
National Taiwan Normal University
CNRS
Kenyon College
Tongji University
University of Trieste
Indian Institute of Technology Madras
Saha Institute of Nuclear Physics
ISAS/JAXA
Institut des Hautes Études Scientifiques
Ryukoku University
Indian Institute of Science Education and Research Kolkata
University of Notre Dame
Istituto dei Sistemi Complessi
Korea Astronomy and Space Science Institute
Hobart and William Smith Colleges
The Federal University of Rio Grande do Norte
Museo Storico della Fisica e Centro Studi e Ricerche Enrico Fermi
University Roma Tre
University of Arizona
University of California, Riverside
University of Washington
Indian Institute of Technology Gandhinagar
National Institute of Technology
Universidade de Aveiro
Marquette University
Toho University
Gunma University
Chapman University
High Energy Accelerator Research Organization (KEK)
Osaka Institute of Technology
Osservatorio Astrofisico Di Arcetri
Indian Institute of Technology Hyderabad
Indian Institute of Science Education and Research (IISER)
Istituto di Astrofisica e Planetologia Spaziali
Andrews University
Tokyo City University
Kyoto University
Yukawa Institute for Theoretical Physics
Van Swinderen Institute for Particle Physics and Gravity
Vrjie Universiteit Brussel
High Energy Accelerator Research Organization (KEK)
National Defense Academy of Japan
University of Florida
Nagaoka University of Technology
Tata Institute of Fundamental Research, Mumbai
Technical University of Eindhoven
Sejong University
Concordia University Wisconsin
National Yang Ming Chiao Tung University
Rikkyo University

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

Résumé

We present Fermi Gamma-ray Burst Monitor (Fermi-GBM) and Swift Burst Alert Telescope (Swift-BAT) searches for gamma-ray/X-ray counterparts to gravitational-wave (GW) candidate events identified during the third observing run of the Advanced LIGO and Advanced Virgo detectors. Using Fermi-GBM onboard triggers and subthreshold gamma-ray burst (GRB) candidates found in the Fermi-GBM ground analyses, the Targeted Search and the Untargeted Search, we investigate whether there are any coincident GRBs associated with the GWs. We also search the Swift-BAT rate data around the GW times to determine whether a GRB counterpart is present. No counterparts are found. Using both the Fermi-GBM Targeted Search and the Swift- BAT search, we calculate flux upper limits and present joint upper limits on the gamma-ray luminosity of each GW. Given these limits, we constrain theoretical models for the emission of gamma rays from binary black hole mergers.

langue originale	Anglais
Numéro d'article	149
journal	Astrophysical Journal
Volume	964
Numéro de publication	2
Les DOIs	https://doi.org/10.3847/1538-4357/ad1eed
état	Publié - 1 avr. 2024
Modification externe	Oui

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10.3847/1538-4357/ad1eed

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@article{9b8a51ff00094d34a8a0d60fcfb026f6,

title = "A Joint Fermi-GBM and Swift-BAT Analysis of Gravitational-wave Candidates from the Third Gravitational-wave Observing Run",

abstract = "We present Fermi Gamma-ray Burst Monitor (Fermi-GBM) and Swift Burst Alert Telescope (Swift-BAT) searches for gamma-ray/X-ray counterparts to gravitational-wave (GW) candidate events identified during the third observing run of the Advanced LIGO and Advanced Virgo detectors. Using Fermi-GBM onboard triggers and subthreshold gamma-ray burst (GRB) candidates found in the Fermi-GBM ground analyses, the Targeted Search and the Untargeted Search, we investigate whether there are any coincident GRBs associated with the GWs. We also search the Swift-BAT rate data around the GW times to determine whether a GRB counterpart is present. No counterparts are found. Using both the Fermi-GBM Targeted Search and the Swift- BAT search, we calculate flux upper limits and present joint upper limits on the gamma-ray luminosity of each GW. Given these limits, we constrain theoretical models for the emission of gamma rays from binary black hole mergers.",

author = "Collaboration and \{KAGRA Collaboration\} and \{Fermi Gamma-Ray Burst Monitor Team\} and \{The LIGO Scientific Collaboration\} and C. Fletcher and J. Wood and R. Hamburg and P. Veres and Hui, \{C. M.\} and E. Bissaldi and Briggs, \{M. S.\} and E. Burns and Cleveland, \{W. H.\} and Giles, \{M. M.\} and A. Goldstein and Hristov, \{B. A.\} and D. Kocevski and S. Lesage and B. Mailyan and C. Malacaria and S. Poolakkil and \{von Kienlin\}, A. and Wilson-Hodge, \{C. A.\} and M. Crnogor{\v c}evi{\'c} and J. DeLaunay and A. Tohuvavohu and R. Caputo and Cenko, \{S. B.\} and S. Laha and T. Parsotan and R. Abbott and H. Abe and F. Acernese and K. Ackley 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 K. Agatsuma and N. Aggarwal 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. Allocca and Altin, \{P. A.\} and A. Amato and S. Chaty",

year = "2024",

month = apr,

day = "1",

doi = "10.3847/1538-4357/ad1eed",

language = "English",

volume = "964",

journal = "Astrophysical Journal",

issn = "0004-637X",

number = "2",

}

TY - JOUR

T1 - A Joint Fermi-GBM and Swift-BAT Analysis of Gravitational-wave Candidates from the Third Gravitational-wave Observing Run

AU - Collaboration

AU - KAGRA Collaboration

AU - Fermi Gamma-Ray Burst Monitor Team

AU - The LIGO Scientific Collaboration

AU - Fletcher, C.

AU - Wood, J.

AU - Hamburg, R.

AU - Veres, P.

AU - Hui, C. M.

AU - Bissaldi, E.

AU - Briggs, M. S.

AU - Burns, E.

AU - Cleveland, W. H.

AU - Giles, M. M.

AU - Goldstein, A.

AU - Hristov, B. A.

AU - Kocevski, D.

AU - Lesage, S.

AU - Mailyan, B.

AU - Malacaria, C.

AU - Poolakkil, S.

AU - von Kienlin, A.

AU - Wilson-Hodge, C. A.

AU - Crnogorčević, M.

AU - DeLaunay, J.

AU - Tohuvavohu, A.

AU - Caputo, R.

AU - Cenko, S. B.

AU - Laha, S.

AU - Parsotan, T.

AU - Abbott, R.

AU - Abe, H.

AU - Acernese, F.

AU - Ackley, K.

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 - Agatsuma, K.

AU - Aggarwal, N.

AU - Aguiar, O. D.

AU - Aiello, L.

AU - Ain, A.

AU - Ajith, P.

AU - Akutsu, T.

AU - Albanesi, S.

AU - Alfaidi, R. A.

AU - Allocca, A.

AU - Altin, P. A.

AU - Amato, A.

AU - Chaty, S.

PY - 2024/4/1

Y1 - 2024/4/1

N2 - We present Fermi Gamma-ray Burst Monitor (Fermi-GBM) and Swift Burst Alert Telescope (Swift-BAT) searches for gamma-ray/X-ray counterparts to gravitational-wave (GW) candidate events identified during the third observing run of the Advanced LIGO and Advanced Virgo detectors. Using Fermi-GBM onboard triggers and subthreshold gamma-ray burst (GRB) candidates found in the Fermi-GBM ground analyses, the Targeted Search and the Untargeted Search, we investigate whether there are any coincident GRBs associated with the GWs. We also search the Swift-BAT rate data around the GW times to determine whether a GRB counterpart is present. No counterparts are found. Using both the Fermi-GBM Targeted Search and the Swift- BAT search, we calculate flux upper limits and present joint upper limits on the gamma-ray luminosity of each GW. Given these limits, we constrain theoretical models for the emission of gamma rays from binary black hole mergers.

AB - We present Fermi Gamma-ray Burst Monitor (Fermi-GBM) and Swift Burst Alert Telescope (Swift-BAT) searches for gamma-ray/X-ray counterparts to gravitational-wave (GW) candidate events identified during the third observing run of the Advanced LIGO and Advanced Virgo detectors. Using Fermi-GBM onboard triggers and subthreshold gamma-ray burst (GRB) candidates found in the Fermi-GBM ground analyses, the Targeted Search and the Untargeted Search, we investigate whether there are any coincident GRBs associated with the GWs. We also search the Swift-BAT rate data around the GW times to determine whether a GRB counterpart is present. No counterparts are found. Using both the Fermi-GBM Targeted Search and the Swift- BAT search, we calculate flux upper limits and present joint upper limits on the gamma-ray luminosity of each GW. Given these limits, we constrain theoretical models for the emission of gamma rays from binary black hole mergers.

U2 - 10.3847/1538-4357/ad1eed

DO - 10.3847/1538-4357/ad1eed

M3 - Article

AN - SCOPUS:85189472922

SN - 0004-637X

VL - 964

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 149

ER -

A Joint Fermi-GBM and Swift-BAT Analysis of Gravitational-wave Candidates from the Third Gravitational-wave Observing Run

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