Passer à la navigation principale Passer à la recherche Passer au contenu principal

First joint observation by the underground gravitational-wave detector KAGRA with GEO 600

  • The LIGO Scientific Collaboration
  • , the Virgo Collaboration
  • , the KAGRA Collaboration
  • California Institute of Technology
  • Tokyo Institute of Technology
  • University of Salerno
  • INFN Sezione di Napoli
  • Monash University
  • University of Wisconsin-Milwaukee
  • Louisiana State University
  • 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
  • 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
  • Laboratoire de Probabilités et Modèles Aléatoires
  • Université Paris-Saclay
  • European Gravitational Observatory (EGO)
  • College of Computing
  • Chennai Mathematical Institute
  • Department of Mathematics and Physics
  • 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
  • University of Maryland, College Park
  • Université de Toulouse
  • Villanova University
  • Universidade de Santiago de Compostela
  • Stony Brook University
  • Flatiron Institute
  • NASA Goddard Space Flight Center
  • 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
  • Pennsylvania State University
  • University of Rhode Island
  • Bellevue College
  • Scuola Normale Superiore di Pisa
  • Eötvös Loránd 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 California, Berkeley
  • Maastricht University
  • Lancaster University
  • Nihon University
  • CCLRC Rutherford Appleton Laboratory
  • Chungnam National University
  • Aoyama Gakuin University
  • Tsinghua University
  • Aristotle University of Thessaloniki
  • University of Toyama
  • Services and Estate Management
  • 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
  • Seoul National University
  • Sungkyunkwan University
  • Université Paris Est, ENPC LIGM, IMAGINE
  • University of Florence
  • National Cheng Kung University
  • Wuhan University
  • National Applied Research Laboratories
  • National Taiwan Normal University
  • NASA Marshall Space Flight Center
  • 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, Nagaoka College
  • 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
  • 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 journalArticleRevue par des pairs

Résumé

We report the results of the first joint observation of the KAGRA detector with GEO 600. KAGRA is a cryogenic and underground gravitational-wave detector consisting of a laser interferometer with 3 km arms, located in Kamioka, Gifu, Japan. GEO 600 is a British-German laser interferometer with 600 m arms, located near Hannover, Germany. GEO 600 and KAGRA performed a joint observing run from April 7 to 20, 2020. We present the results of the joint analysis of the GEO-KAGRA data for transient gravitational-wave signals, including the coalescence of neutron-star binaries and generic unmodeled transients. We also perform dedicated searches for binary coalescence signals and generic transients associated with gamma-ray burst events observed during the joint run. No gravitational-wave events were identified. We evaluate the minimum detectable amplitude for various types of transient signals and the spacetime volume for which the network is sensitive to binary neutron-star coalescences. We also place lower limits on the distances to the gamma-ray bursts analyzed based on the non-detection of an associated gravitational-wave signal for several signal models, including binary coalescences. These analyses demonstrate the feasibility and utility of KAGRA as a member of the global gravitational-wave detector network.

langue originaleAnglais
Numéro d'article063F01
journalProgress of Theoretical and Experimental Physics
Volume2022
Numéro de publication6
Les DOIs
étatPublié - 1 juin 2022
Modification externeOui

Empreinte digitale

Examiner les sujets de recherche de « First joint observation by the underground gravitational-wave detector KAGRA with GEO 600 ». Ensemble, ils forment une empreinte digitale unique.

Contient cette citation