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

  • The LIGO Scientific Collaboration
  • , The Virgo Collaboration
  • , the KAGRA Collaboration
  • , R. Abbott
  • , H. Abe
  • , F. Acernese
  • , K. Ackley
  • , N. Adhikari
  • , R. X. Adhikari
  • , V. K. Adkins
  • , V. B. Adya
  • , C. Affeldt
  • , D. Agarwal
  • , M. Agathos
  • , K. Agatsuma
  • , N. Aggarwal
  • , O. D. Aguiar
  • , L. Aiello
  • , A. Ain
  • , P. Ajith
  • T. Akutsu, S. Albanesi, R. A. Alfaidi, A. Allocca, P. A. Altin, A. Amato, C. Anand, S. Anand, A. Ananyeva, S. B. Anderson, W. G. Anderson, M. Ando, T. Andrade, N. Andres, M. Andrés-Carcasona, T. Andrić, S. V. Angelova, S. Ansoldi, J. M. Antelis, S. Antier, T. Apostolatos, E. Z. Appavuravther, S. Appert, S. K. Apple, K. Arai, A. Araya, M. C. Araya, J. S. Areeda, M. Arène, N. Aritomi, N. Arnaud, M. Arogeti, S. M. Aronson, K. G. Arun, H. Asada, Y. Asali, G. Ashton, Y. Aso, M. Assiduo, S. Assis de Souza Melo, S. M. Aston, P. Astone, F. Aubin, K. AultONeal, C. Austin, S. Babak, F. Badaracco, M. K.M. Bader, C. Badger, S. Bae, Y. Bae, A. M. Baer, S. Bagnasco, Y. Bai, J. Baird, R. Bajpai, T. Baka, M. Ball, G. Ballardin, S. W. Ballmer, A. Balsamo, G. Baltus, S. Banagiri, B. Banerjee, D. Bankar, J. C. Barayoga, C. Barbieri, B. C. Barish, D. Barker, P. Barneo, F. Barone, B. Barr, L. Barsotti, M. Barsuglia, D. Barta, J. Bartlett, M. A. Barton, I. Bartos, S. Basak, R. Bassiri, A. Basti, M. Bawaj, J. C. Bayley, M. Bazzan, B. R. Becher, B. Bécsy, V. M. Bedakihale, F. Beirnaert, M. Bejger, I. Belahcene, V. Benedetto, D. Beniwal, M. G. Benjamin, T. F. Bennett, J. D. Bentley, M. BenYaala, S. Bera, M. Berbel, F. Bergamin, B. K. Berger, S. Bernuzzi, C. P.L. Berry, D. Bersanetti, A. Bertolini, J. Betzwieser, D. Beveridge, R. Bhandare, A. V. Bhandari, U. Bhardwaj, R. Bhatt, D. Bhattacharjee, S. Bhaumik, A. Bianchi, I. A. Bilenko, G. Billingsley, S. Bini, R. Birney, O. Birnholtz, S. Biscans, M. Bischi, S. Biscoveanu, A. Bisht, B. Biswas, M. Bitossi, M. A. Bizouard, J. K. Blackburn, C. D. Blair, D. G. Blair, R. M. Blair, F. Bobba, N. Bode, M. Boër, G. Bogaert, M. Boldrini, G. N. Bolingbroke, L. D. Bonavena, F. Bondu, E. Bonilla, R. Bonnand, P. Booker, B. A. Boom, R. Bork, V. Boschi, N. Bose, S. Bose, V. Bossilkov, V. Boudart, Y. Bouffanais, A. Bozzi, C. Bradaschia, P. R. Brady, A. Bramley, A. Branch, M. Branchesi, J. E. Brau, M. Breschi, T. Briant, J. H. Briggs, A. Brillet, M. Brinkmann, P. Brockill, A. F. Brooks, J. Brooks, D. D. Brown, S. Brunett, G. Bruno, R. Bruntz, J. Bryant, F. Bucci, T. Bulik, H. J. Bulten, A. Buonanno, K. Burtnyk, R. Buscicchio, D. Buskulic, C. Buy, R. L. Byer, G. S.Cabourn Davies, G. Cabras, R. Cabrita, L. Cadonati, M. Caesar, G. Cagnoli, C. Cahillane, J. Calderón Bustillo, J. D. Callaghan, T. A. Callister, E. Calloni, J. Cameron, J. B. Camp, M. Canepa, S. Canevarolo, M. Cannavacciuolo, K. C. Cannon, H. Cao, Z. Cao, E. Capocasa, E. Capote, G. Carapella, F. Carbognani, M. Carlassara, J. B. Carlin, M. F. Carney, M. Carpinelli, G. Carrillo, G. Carullo, T. L. Carver, J. Casanueva Diaz, C. Casentini, G. Castaldi, S. Caudill, M. Cavaglià, F. Cavalier, R. Cavalieri, G. Cella, P. Cerdá-Durán, E. Cesarini, W. Chaibi, S. Chalathadka Subrahmanya, E. Champion, C. H. Chan, C. L. Chan, C. L. Chan, K. Chan, M. Chan, K. Chandra, I. P. Chang, P. Chanial, S. Chao, C. Chapman-Bird, P. Charlton, E. A. Chase, E. Chassande-Mottin
  • California Institute of Technology
  • Tokyo Institute of Technology
  • Salerno
  • Complesso Universitario di Monte Sant'Angelo
  • Monash University
  • University of Wisconsin-Milwaukee
  • Louisiana State University
  • Australian National University
  • Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • Leibniz Universität Hannover
  • The Inter-University Centre for Astronomy and Astrophysics
  • University of Cambridge
  • Friedrich Schiller Universität
  • University of Birmingham
  • Northwestern University
  • Instituto Nacional de Pesquisas Espaciais
  • Cardiff University
  • INFN
  • Tata Institute of Fundamental Research
  • National Astronomical Observatory of Japan
  • Università degli Studi di Torino
  • INFN Sezione di Torino
  • University of Glasgow
  • Complesso Universitario di Monte S.Angelo
  • Université Claude Bernard Lyon 1
  • University of Tokyo
  • University of Barcelona
  • IN2P3 Institut National de Physique Nucleaire et de Physique des Particules
  • Institució Catalana de Recerca i Estudis Avançats
  • Gran Sasso Science Institute
  • University of Strathclyde
  • Università di Udine
  • Sezione di Trieste
  • Embry-Riddle Aeronautical University
  • Observatoire de la Côte d'Azur
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  • American University
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  • LIGO Livingston Observatory
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  • University of Louvain
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  • King's College London
  • Korea Institute of Science and Technology Information
  • National Institute Mathematical Sciences
  • Christopher Newport University
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  • Dipartimento di Medicina, Chirurgia e Odontoiatria “Scuola Medica Salernitana"
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  • University of Valencia
  • Universität Hamburg
  • Rochester Institute of Technology
  • National Tsing Hua University
  • Chinese University of Hong Kong
  • Fukuoka University

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Abstract

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.
Original languageEnglish
Article number063F01
JournalProgress of Theoretical and Experimental Physics
Volume2022
Issue number6
DOIs
Publication statusPublished - 01 Jun 2022

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