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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
  • German Electron Synchrotron
  • 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
  • CEA-IRFU/CNRS/Université Paris Diderot
  • National Institute for Nuclear Physics
  • University of Trieste
  • Rice University
  • University of Padua
  • NASA Goddard Space Flight Center
  • University of Maryland
  • University of Turin
  • Université Montpellier 2
  • University of Johannesburg
  • École polytechnique
  • University of Washington
  • University of Maryland Baltimore County
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • Polytechnic University of Bari
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • Italian Space Agency
  • George Mason University
  • Naval Research Laboratory
  • Sonoma State University
  • Centre d'Etudes Nucléaires Bordeaux-Gradingnan (CENBG)
  • Osservatorio Astronomico Roma
  • National Institute for Astrophysics
  • University of Bologna
  • Pegaso Telematic University
  • University of Udine
  • Hiroshima University
  • Friedrich-Alexander University Erlangen-Nürnberg
  • Pontificia Universidad Católica de Chile
  • Open University of Israel
  • Université d'Orléans
  • CNRS
  • Innsbruck Medical University
  • University of North Florida
  • University of Southampton
  • University of Iceland
  • The University of Tokyo
  • CSIC
  • Max Planck Institute for Physics (Werner Heisenberg Institute)
  • University of California at Irvine
  • University of Denver
  • The University of Hong Kong
  • NYCB Real-Time Computing Inc.
  • Purdue University Northwest
  • Nagoya University
  • Max Planck Institute for Nuclear Physics
  • ICREA
  • Department of Physics
  • University of Nova Gorica

Research output: Contribution to journalArticlepeer-review

47 Citations (Scopus)

Abstract

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.

Original languageEnglish
Article numberL2
JournalAstrophysical Journal Letters
Volume823
Issue number1
DOIs
Publication statusPublished - 20 May 2016

Keywords

  • gamma-ray burst: general
  • gamma-rays: general
  • gravitational waves
  • methods: observational

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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