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Fermi-LAT observations of the gamma-ray burst GRB 130427A

  • M. Ackermann
  • , M. Ajello
  • , K. Asano
  • , W. B. Atwood
  • , M. Axelsson
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , M. G. Baring
  • , D. Bastieri
  • , K. Bechtol
  • , R. Bellazzini
  • , E. Bissaldi
  • , E. Bonamente
  • , J. Bregeon
  • , M. Brigida
  • , P. Bruel
  • , R. Buehler
  • , J. Michael Burgess
  • , S. Buson
  • G. A. Caliandro, R. A. Cameron, P. A. Caraveo, C. Cecchi, V. Chaplin, E. Charles, A. Chekhtman, C. C. Cheung, J. Chiang, G. Chiaro, S. Ciprini, R. Claus, W. Cleveland, J. Cohen-Tanugi, A. Collazzi, L. R. Cominsky, V. Connaughton, J. Conrad, S. Cutini, F. D'Ammando, A. De Angelis, M. DeKlotz, F. De Palma, C. D. Dermer, R. Desiante, A. Diekmann, L. Di Venere, P. S. Drell, A. Drlica-Wagner, C. Favuzzi, S. J. Fegan, E. C. Ferrara, J. Finke, G. Fitzpatrick, W. B. Focke, A. Franckowiak, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, N. Gehrels, S. Germani, M. Gibby, N. Giglietto, M. Giles, F. Giordano, M. Giroletti, G. Godfrey, J. Granot, I. A. Grenier, J. E. Grove, D. Gruber, S. Guiriec, D. Hadasch, Y. Hanabata, A. K. Harding, M. Hayashida, E. Hays, D. Horan, R. E. Hughes, Y. Inoue, T. Jogler, G. Jóhannesson, W. N. Johnson, T. Kawano, J. Knödlseder, D. Kocevski, M. Kuss, J. Lande, S. Larsson, L. Latronico, F. Longo, F. Loparco, M. N. Lovellette, P. Lubrano, M. Mayer, M. N. Mazziotta, J. E. McEnery, P. F. Michelson, T. Mizuno, A. A. Moiseev, M. E. Monzani, E. Moretti, A. Morselli, I. V. Moskalenko, S. Murgia, R. Nemmen, E. Nuss, M. Ohno, T. Ohsugi, A. Okumura, N. Omodei, M. Orienti, D. Paneque, V. Pelassa, J. S. Perkins, M. Pesce-Rollins, V. Petrosian, F. Piron, G. Pivato, T. A. Porter, J. L. Racusin, S. Rainò, R. Rando, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, S. Ritz, M. Roth, F. Ryde, A. Sartori, P. M. Saz Parkinson, J. D. Scargle, A. Schulz, C. Sgrò, E. J. Siskind, E. Sonbas, G. Spandre, P. Spinelli, H. Tajima, H. Takahashi, J. G. Thayer, J. B. Thayer, D. J. Thompson, L. Tibaldo, M. Tinivella, D. F. Torres, G. Tosti, E. Troja, T. L. Usher, J. Vandenbroucke, V. Vasileiou, G. Vianello, V. Vitale, B. L. Winer, K. S. Wood, R. Yamazaki, G. Younes, H. F. Yu, S. J. Zhu, P. N. Bhat, M. S. Briggs, D. Byrne, S. Foley, A. Goldstein, P. Jenke, R. M. Kippen, C. Kouveliotou, S. McBreen, C. Meegan, W. S. Paciesas, R. Preece, A. Rau, D. Tierney, A. J. Van Der Horst, A. Von Kienlin, C. Wilson-Hodge, S. Xiong, G. Cusumano, V. La Parola, J. R. Cummings
  • c/o DESY
  • University of California, Space Sciences Laboratory
  • University of Tokyo
  • University of California at Santa Cruz
  • Stockholm University
  • Oskar Klein Centre
  • KTH Royal Institute of Technology
  • University of Pisa
  • Université Paris-Diderot
  • INFN Sezione di Trieste
  • University of Trieste
  • Rice University
  • INFN
  • University of Padova
  • Stanford University
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • INFN Sezione di Perugia
  • University of Perugia
  • Politecnico di Bari
  • INFN Sezione di Bari
  • Center for Space Plasma and Aeronomic Research
  • University of Sheffield
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • George Mason University
  • Naval Research Laboratory
  • Science and Research Directorate
  • Osservatorio Astronomico di Roma
  • Universities Space Research Association
  • Laboratoire Univers et Particules de Montpellier
  • NASA Postdoctoral Program Fellow
  • Sonoma State University
  • Royal Swedish Academy of Sciences
  • INAF Istituto di Radioastronomia
  • and Physics University of Udine
  • Stellar Solutions Inc.
  • Jacobs Technology Inc.
  • NASA Goddard Space Flight Center
  • University College Dublin
  • Hiroshima University
  • The Open University of Israel
  • Max Planck Institut für Extraterrestrische Physik
  • Department of Astronomy, Graduate School of Science, Kyoto University
  • The Ohio State University
  • University of Iceland
  • IRAP/CNRS
  • Université Paul Sabatier
  • INFN Sezione di Torino
  • University of Maryland
  • INFN Roma Tor Vergata
  • Nagoya University
  • Max-Planck-Institut für Physik
  • Biochemical and Environmental Engineering
  • University of Johannesburg
  • University of Innsbruck
  • University of Washington
  • NASA Ames Research Center
  • NYCB Real-Time Computing Inc.
  • Adiyaman University
  • Pompeu Fabra University (UPF)
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • University of Rome “Tor Vergata”
  • Aoyama Gakuin University
  • NASA Marshall Space Flight Center
  • MST-8, Los Alamos National Laboratory
  • University of Amsterdam
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
  • Biochemical and Environmental Engineering

Research output: Contribution to journalArticlepeer-review

Abstract

The observations of the exceptionally bright gamma-ray burst (GRB) 130427A by the Large Area Telescope aboard the Fermi Gamma-ray Space Telescope provide constraints on the nature of these unique astrophysical sources. GRB 130427A had the largest fluence, highest-energy photon (95 GeV), longest γ-ray duration (20 hours), and one of the largest isotropic energy releases ever observed from a GRB. Temporal and spectral analyses of GRB 130427A challenge the widely accepted model that the nonthermal high-energy emission in the afterglow phase of GRBs is synchrotron emission radiated by electrons accelerated at an external shock.

Original languageEnglish
Pages (from-to)42-47
Number of pages6
JournalScience
Volume343
Issue number6166
DOIs
Publication statusPublished - 1 Jan 2014

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