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Multiwavelength observations of GRB 110731A: GeV emission from onset to afterglow

  • M. Ackermann
  • , M. Ajello
  • , K. Asano
  • , L. Baldini
  • , G. Barbiellini
  • , M. G. Baring
  • , D. Bastieri
  • , R. Bellazzini
  • , R. D. Blandford
  • , E. Bonamente
  • , A. W. Borgland
  • , E. Bottacini
  • , J. Bregeon
  • , M. Brigida
  • , P. Bruel
  • , R. Buehler
  • , S. Buson
  • , G. A. Caliandro
  • , R. A. Cameron
  • , P. A. Caraveo
  • C. Cecchi, E. Charles, R. C.G. Chaves, A. Chekhtman, J. Chiang, S. Ciprini, R. Claus, J. Cohen-Tanugi, J. Conrad, S. Cutini, F. D'Ammando, A. De Angelis, F. De Palma, C. D. Dermer, E. Do Couto E Silva, P. S. Drell, A. Drlica-Wagner, C. Favuzzi, S. J. Fegan, W. B. Focke, A. Franckowiak, Y. Fukazawa, P. Fusco, F. Gargano, D. Gasparrini, N. Gehrels, N. Giglietto, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, J. Granot, J. Greiner, I. A. Grenier, J. E. Grove, S. Guiriec, D. Hadasch, Y. Hanabata, M. Hayashida, E. Hays, R. E. Hughes, M. S. Jackson, T. Jogler, G. Jóhannesson, A. S. Johnson, J. Knödlseder, D. Kocevski, M. Kuss, J. Lande, S. Larsson, L. Latronico, F. Longo, F. Loparco, M. N. Lovellette, P. Lubrano, M. N. Mazziotta, J. E. McEnery, J. Mehault, P. Mészáros, P. F. Michelson, W. Mitthumsiri, T. Mizuno, C. Monte, M. E. Monzani, E. Moretti, A. Morselli, I. V. Moskalenko, S. Murgia, M. Naumann-Godo, J. P. Norris, E. Nuss, T. Nymark, M. Ohno, T. Ohsugi, N. Omodei, M. Orienti, E. Orlando, D. Paneque, J. S. Perkins, M. Pesce-Rollins, F. Piron, G. Pivato, J. L. Racusin, S. Rainò, R. Rando, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, C. Romoli, M. Roth, F. Ryde, D. A. Sanchez, C. Sgrò, E. J. Siskind, E. Sonbas, P. Spinelli, M. Stamatikos, H. Takahashi, T. Tanaka, J. G. Thayer, J. B. Thayer, L. Tibaldo, M. Tinivella, G. Tosti, E. Troja, T. L. Usher, J. Vandenbroucke, V. Vasileiou, G. Vianello, V. Vitale, A. P. Waite, B. L. Winer, K. S. Wood, Z. Yang, D. Gruber, P. N. Bhat, E. Bissaldi, M. S. Briggs, J. M. Burgess, V. Connaughton, S. Foley, R. M. Kippen, C. Kouveliotou, S. McBreen, S. McGlynn, W. S. Paciesas, V. Pelassa, R. Preece, A. Rau, A. J. Van Der Horst, A. Von Kienlin, D. A. Kann, R. Filgas, S. Klose, T. Krühler, A. Fukui, T. Sako, P. J. Tristram, S. R. Oates, T. N. Ukwatta, O. Littlejohns
  • c/o DESY
  • Stanford University
  • Interactive Research Center of Science
  • Tokyo Institute of Technology
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • INFN Gruppo Collegato di Udine
  • INFN Sezione di Trieste
  • Dipartimento di Fisica
  • University of Trieste
  • Department of Physics and Astronomy
  • Rice University
  • INFN
  • Dipartimento di Fisica e Astronomia G. Galilei
  • University of Padova
  • Sezione di Perugia
  • INFN Sezione di Perugia
  • INFM CRS-SOFT
  • University of Perugia
  • Politecnico di Bari
  • INFN
  • INFN Sezione di Bari
  • University of Sheffield
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Laboratoire AIM
  • Universite Paris-Saclay
  • Center for Earth Observing and Space Research
  • George Mason University
  • Naval Research Laboratory
  • ASI Science Data Center
  • Laboratoire Univers et Particules de Montpellier
  • Department of Physics
  • Stockholm University
  • Oskar Klein Centre
  • Science and Research Directorate
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
  • INAF-IASF
  • Dipartimento di Fisica
  • and Physics University of Udine
  • Space Science Division
  • Department of Physical Science
  • Hiroshima University
  • NASA Goddard Space Flight Center
  • INAF Istituto di Radioastronomia
  • Centre for Astrophysics Research
  • University of Hertfordshire
  • Max Planck Institut für Extraterrestrische Physik
  • Center for Space Plasma and Aeronomic Research
  • Department of Astronomy
  • Kyoto University
  • Department of Physics
  • The Ohio State University
  • KTH Royal Institute of Technology
  • University of Iceland
  • IRAP/CNRS
  • Department of Astronomy
  • Sezione di Torino
  • INFN Sezione di Torino
  • University of Maryland
  • Department of Astronomy and Astrophysics
  • Pennsylvania State University
  • Hiroshima Astrophysical Science Center
  • Sezione di Roma
  • Department of Physics
  • Boise State University
  • ISAS/JAXA
  • Max-Planck-Institut für Physik
  • Department of Physics
  • Biochemical and Environmental Engineering
  • Center for Research and Exploration in Space Science and Technology (CRESST)
  • Center for Astrophysics | Harvard & Smithsonian
  • University of California at Santa Cruz
  • Medical University of Innsbruck
  • Department of Physics
  • University of Washington
  • Max-Planck-Institut für Kernphysik
  • NYCB Real-Time Computing Inc.
  • Faculty of Arts and Sciences
  • Adiyaman University
  • Universities Space Research Association
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • Dipartimento di Fisica
  • University of Rome “Tor Vergata”
  • School of Physics
  • University College Dublin
  • MST-8, Los Alamos National Laboratory
  • NASA Marshall Space Flight Center
  • Technical University of Munich
  • Thüringer Landessternwarte Tautenburg
  • Institute of Experimental and Applied Physics Czech Technical University in Prague
  • Niels Bohr Institutet
  • National Astronomical Observatory
  • Solar-Terrestrial Environment Laboratory
  • Nagoya University
  • Victoria University of Wellington
  • UCL Mullard Space Science Laboratory
  • Department of Physics and Astronomy
  • Michigan State University
  • University of Leicester

Research output: Contribution to journal › Article › peer-review

92 Citations (Scopus)

Abstract

We report on the multiwavelength observations of the bright, long gamma-ray burst GRB 110731A, by the Fermi and Swift observatories, and by the MOA and GROND optical telescopes. The analysis of the prompt phase reveals that GRB 110731A shares many features with bright Large Area Telescope bursts observed by Fermi during the first three years on-orbit: a light curve with short time variability across the whole energy range during the prompt phase, delayed onset of the emission above 100 MeV, extra power-law component and temporally extended high-energy emission. In addition, this is the first GRB for which simultaneous GeV, X-ray, and optical data are available over multiple epochs beginning just after the trigger time and extending for more than 800 s, allowing temporal and spectral analysis in different epochs that favor emission from the forward shock in a wind-type medium. The observed temporally extended GeV emission is most likely part of the high-energy end of the afterglow emission. Both the single-zone pair transparency constraint for the prompt signal and the spectral and temporal analysis of the forward-shock afterglow emission independently lead to an estimate of the bulk Lorentz factor of the jet Γ ∼ 500-550.

Original languageEnglish
Article number71
JournalAstrophysical Journal
Volume763
Issue number2
DOIs
Publication statusPublished - 1 Feb 2013

Keywords

  • gamma-ray burst: individual (GRB110731A)

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