%0 Journal Article
%T FERMI-LAT observations of the ligo event GW150914
%+ Stanford University
%+ Groupe de Recherche en Physique des Hautes Energies (GRPHE)
%+ Los Alamos National Laboratory (LANL)
%+ Santa Cruz Institute for Particle Physics (SCIPP)
%+ Groupe de Recherche en Economie Théorique et Appliquée (GREThA)
%+ Laboratoire Univers et Particules de Montpellier (LUPM)
%+ Institut de Physique Théorique - UMR CNRS 3681 (IPHT)
%+ Laboratoire Leprince-Ringuet (LLR)
%+ Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112))
%+ Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG)
%+ SLAC National Accelerator Laboratory (SLAC)
%+ UGC-DAE Consortium for Scientific Research
%+ Department of Molecular Medicine
%+ IHU-LIRYC
%+ NASA Goddard Space Flight Center (GSFC)
%+ London School of Hygiene and Tropical Medicine (LSHTM)
%+ Istituto Nazionale di Fisica Nucleare, sezione di Bari (INFN, sezione di Bari)
%+ Istituto Nazionale di Astrofisica (INAF)
%+ École nationale supérieure d'architecture de Nantes (ENSA Nantes)
%+ Unité Scientifique de la Station de Nançay (USN)
%+ Laboratoire de Physique et Chimie de l'Environnement et de l'Espace (LPC2E)
%+ GSFC Astrophysics Science Division
%+ Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
%+ DIEE
%+ Göteborgs Universitet = University of Gothenburg (GU)
%+ China Agricultural University (CAU)
%+ Laboratoire de Météorologie Dynamique (UMR 8539) (LMD)
%+ Hansen Experimental Physics Lab [Stanford] (HEPL)
%+ Institut Pasteur de Montevideo
%+ University of Botswana
%+ Department of Animal and Avian Sciences
%+ Medical Sciences Division
%+ Centre de Recherche Interdisciplinaire sur la Biologie, la Santé la Société, et l’Environnement
%+ Centre Hospitalier Universitaire de Dijon - Hôpital François Mitterrand (CHU Dijon)
%+ Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique (LERMA)
%+ École nationale supérieure d'architecture de Versailles (ENSA-V)
%+ Department of Plant Sciences [Univ California Davis] (Plant - UC Davis)
%+ Sea Mammal Research Unit
%+ Department of Physics [Tokyo]
%+ Naval Research Laboratory (NRL)
%+ Zhejiang University
%+ Laboratoire de Conception Fabrication Commande (LCFC)
%A Ackermann, Markus
%A Ajello, Marco
%A Albert, A.
%A Anderson, B.
%A Arimoto, M.
%A Atwood, William B.
%A Axelsson, Magnus
%A Baldini, Luca
%A Ballet, Jean
%A Barbiellini, Guido
%A Baring, Matthew G.
%A Bastieri, D.
%A Gonzalez, J. Becerra
%A Bellazzini, R.
%A Bissaldi, E.
%A Blandford, R. D.
%A Bloom, E. D.
%A Bonino, R.
%A Bottacini, E.
%A Brandt, T. J.
%A Bregeon, J.
%A Britto, R. J.
%A Bruel, P.
%A Buehler, R.
%A Burnett, T. H.
%A Buson, S.
%A Caliandro, G. A.
%A Cameron, R. A.
%A Caputo, R.
%A Caragiulo, M.
%A Caraveo, P. A.
%A Casandjian, J. M.
%A Cavazzuti, E.
%A Charles, E.
%A Chekhtman, A.
%A Chiang, J.
%A Chiaro, G.
%A Ciprini, S.
%A Cohen-Tanugi, J.
%A Cominsky, L. R.
%A Condon, B.
%A Costanza, F.
%A Cuoco, A.
%A Cutini, S.
%A D’ammando, F.
%A Dumora, D.
%A Palma, F. De
%A Desiante, R.
%A Digel, S. W.
%A Lalla, N. Di
%A Mauro, M. Di
%A Venere, L. Di
%A Domínguez, A.
%A Drell, P. S.
%A Dubois, R.
%A Favuzzi, C.
%A Fegan, S. J.
%A Ferrara, E. C.
%A Franckowiak, A.
%A Fukazawa, Y.
%A Funk, S.
%A Fusco, P.
%A Gargano, F.
%A Gasparrini, D.
%A Gehrels, N.
%A Giglietto, N.
%A Giomi, M.
%A Giommi, P.
%A Giordano, F.
%A Giroletti, M.
%A Glanzman, T.
%A Godfrey, G.
%A Gomez-Vargas, G. A.
%A Granot, J.
%A Green, D.
%A Grenier, I. A.
%A Grondin, M.-H.
%A Grove, J. E.
%A Guillemot, Lucas
%A Guiriec, S.
%A Hadasch, D.
%A Harding, A. K.
%A Hays, E.
%A Hewitt, J. W.
%A Hill, A. B.
%A Horan, D.
%A Jogler, T.
%A Jóhannesson, G.
%A Kamae, T.
%A Kensei, S.
%A Kocevski, D.
%A Kuss, M.
%A Mura, G. La
%A Larsson, S.
%A Latronico, L.
%A Lemoine-Goumard, M.
%A Li, J.
%A Li, L.
%A Longo, F.
%A Loparco, F.
%A Lovellette, M. N.
%A Lubrano, P.
%A Madejski, G. M.
%A Magill, J.
%A Maldera, S.
%A Manfreda, A.
%A Marelli, M.
%A Mayer, M.
%A Mazziotta, M. N.
%A Mcenery, J. E.
%A Meyer, M.
%A Michelson, P. F.
%A Mirabal, N.
%A Mizuno, T.
%A Moiseev, A. A.
%A Monzani, M. E.
%A Moretti, E.
%A Morselli, A.
%A Moskalenko, I. V.
%A Murgia, S.
%A Negro, M.
%A Nuss, E.
%A Ohsugi, T.
%A Omodei, N.
%A Orienti, M.
%A Orlando, E.
%A Ormes, J. F.
%A Paneque, D.
%A Perkins, J. S.
%A Pesce-Rollins, M.
%A Piron, F.
%A Pivato, G.
%A Porter, T. A.
%A Racusin, J. L.
%A Rainò, S.
%A Rando, R.
%A Razzaque, S.
%A Reimer, A.
%A Reimer, O.
%A Reposeur, T.
%A Ritz, S.
%A Rochester, L. S.
%A Romani, R. W.
%A Parkinson, P. M. Saz
%A Sgrò, C.
%A Simone, D.
%A Siskind, E. J.
%A Smith, D. A.
%A Spada, F.
%A Spandre, G.
%A Spinelli, P.
%A Suson, D. J.
%A Tajima, H.
%A Thayer, J. G.
%A Thayer, J. B.
%A Thompson, D. J.
%A Tibaldo, L.
%A Torres, D. F.
%A Troja, E.
%A Uchiyama, Y.
%A Venters, T. M.
%A Vianello, G.
%A Wood, K. S.
%A Wood, M.
%A Zaharijas, G.
%A Zhu, S.
%A Zimmer, S.
%< avec comité de lecture
%@ 2041-8205
%J The Astrophysical journal letters
%I Bristol : IOP Publishing
%V 823
%N 1
%P L2
%8 2016-05
%D 2016
%Z 1602.04488
%R 10.3847/2041-8205/823/1/L2
%K ravitational waves
%K methods: observational
%K gamma rays: general
%Z Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
%Z Sciences of the Universe [physics]Journal articles
%X The Fermi Large Area Telescope (LAT) has an instantaneous field of view (FoV) covering $\sim 1/5$ 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.
%G English
%2 https://insu.hal.science/insu-01362128/document
%2 https://insu.hal.science/insu-01362128/file/Ackermann_2016_ApJL_823_L2.pdf
%L insu-01362128
%U https://insu.hal.science/insu-01362128
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