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FERMI-LAT OBSERVATIONS of the LIGO EVENT GW150914

  • M. Ackermann
  • , M. Ajello
  • , A. Albert
  • , B. Anderson
  • , M. Arimoto
  • , W. B. Atwood
  • , M. Axelsson
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , M. G. Baring
  • , D. Bastieri
  • , J. Becerra Gonzalez
  • , R. Bellazzini
  • , E. Bissaldi
  • , R. D. Blandford
  • , E. D. Bloom
  • , R. Bonino
  • , E. Bottacini
  • , T. J. Brandt
  • J. Bregeon, R. J. Britto, P. Bruel, R. Buehler, T. H. Burnett, S. Buson, G. A. Caliandro, R. A. Cameron, R. Caputo, M. Caragiulo, P. A. Caraveo, J. M. Casandjian, E. Cavazzuti, E. Charles, A. Chekhtman, J. Chiang, G. Chiaro, S. Ciprini, J. Cohen-Tanugi, L. R. Cominsky, B. Condon, F. Costanza, A. Cuoco, S. Cutini, F. D'Ammando, F. De Palma, R. Desiante, S. W. Digel, N. Di Lalla, M. Di Mauro, L. Di Venere, A. Domnguez, P. S. Drell, R. Dubois, D. Dumora, C. Favuzzi, S. J. Fegan, E. C. Ferrara, A. Franckowiak, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, N. Gehrels, N. Giglietto, M. Giomi, P. Giommi, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, G. A. Gomez-Vargas, J. Granot, D. Green, I. A. Grenier, M. H. Grondin, J. E. Grove, L. Guillemot, S. Guiriec, D. Hadasch, A. K. Harding, E. Hays, J. W. Hewitt, A. B. Hill, D. Horan, T. Jogler, G. Jóhannesson, T. Kamae, S. Kensei, D. Kocevski, M. Kuss, G. La Mura, S. Larsson, L. Latronico, M. Lemoine-Goumard, J. Li, L. Li, F. Longo, F. Loparco, M. N. Lovellette, P. Lubrano, G. M. Madejski, J. Magill, S. Maldera, A. Manfreda, M. Marelli, M. Mayer, M. N. Mazziotta, J. E. McEnery, M. Meyer, P. F. Michelson, N. Mirabal, T. Mizuno, A. A. Moiseev, M. E. Monzani, E. Moretti, A. Morselli, I. V. Moskalenko, S. Murgia, M. Negro, E. Nuss, T. Ohsugi, N. Omodei, M. Orienti, E. Orlando, J. F. Ormes, D. Paneque, J. S. Perkins, M. Pesce-Rollins, F. Piron, G. Pivato, T. A. Porter, J. L. Racusin, S. Rain, R. Rando, S. Razzaque, A. Reimer, O. Reimer, T. Reposeur, S. Ritz, L. S. Rochester, R. W. Romani, P. M.Saz Parkinson, C. Sgr, D. Simone, E. J. Siskind, D. A. Smith, F. Spada, G. Spandre, P. Spinelli, D. J. Suson, H. Tajima, J. G. Thayer, J. B. Thayer, D. J. Thompson, L. Tibaldo, D. F. Torres, E. Troja, Y. Uchiyama, T. M. Venters, G. Vianello, K. S. Wood, M. Wood, G. Zaharijas, S. Zhu, S. Zimmer
  • c/o DESY
  • Clemson University
  • Kavli Institute for Particle Astrophysics and Cosmology
  • Stockholm University
  • Oskar Klein Centre
  • Tokyo Institute of Technology
  • University of California at Santa Cruz
  • KTH Royal Institute of Technology
  • Tokyo Metropolitan University
  • University of Pisa
  • Universite Paris-Saclay
  • INFN Sezione di Trieste
  • University of Trieste
  • Rice University
  • INFN
  • University of Padova
  • NASA Goddard Space Flight Center
  • University of Maryland
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • INFN Sezione di Bari
  • INFN Sezione di Torino
  • University of Turin
  • Laboratoire Univers et Particules de Montpellier
  • University of Johannesburg
  • University of Washington
  • Biochemical and Environmental Engineering
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • Politecnico di Bari
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Science and Research Directorate
  • George Mason University
  • Naval Research Laboratory
  • INFN Sezione di Perugia
  • Sonoma State University
  • UMR 5797
  • Osservatorio Astronomico di Roma
  • INAF Istituto di Radioastronomia
  • University of Bologna
  • Università Telematica Pegaso
  • and Physics University of Udine
  • Hiroshima University
  • Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
  • Pontificia Universidad Católica de Chile
  • Sezione di Roma
  • The Open University of Israel
  • conventionnée avec l'Université d'Orléans
  • CNRS
  • Medical University of Innsbruck
  • University of North Florida
  • University of Southampton
  • University of Iceland
  • University of Tokyo
  • University of Sheffield
  • Max-Planck-Institut für Physik
  • Long Beach VA and University of California
  • University of Denver
  • University of Hong Kong
  • NYCB Real-Time Computing Inc.
  • Purdue University Northwest
  • Nagoya University
  • Max-Planck-Institut für Kernphysik
  • Pompeu Fabra University (UPF)
  • Department of Physics
  • University of Nova Gorica

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

The Fermi Large Area Telescope (LAT) has an instantaneous field of view (FoV) covering of the sky and it completes a survey of the entire sky in high-energy gamma-rays every 3 hr. It enables searches for transient phenomena over timescales from milliseconds to years. Among these phenomena could be electromagnetic counterparts to gravitational wave (GW) sources. In this paper, we present a detailed study of the LAT observations relevant to Laser Interferometer Gravitational-wave Observatory (LIGO) event GW150914, which is the first direct detection of gravitational waves and has been interpreted as being due to the coalescence of two stellar-mass black holes. The localization region for GW150914 was outside the LAT FoV at the time of the GW signal. However, as part of routine survey observations, the LAT observed the entire LIGO localization region within ∼70 minutes of the trigger and thus enabled a comprehensive search for a γ-ray counterpart to GW150914. The study of the LAT data presented here did not find any potential counterparts to GW150914, but it did provide limits on the presence of a transient counterpart above 100 MeV on timescales of hours to days over the entire GW150914 localization region.

langue originaleAnglais
Numéro d'articleL2
journalAstrophysical Journal Letters
Volume823
Numéro de publication1
Les DOIs
étatPublié - 20 mai 2016

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