Skip to main navigation Skip to search Skip to main content

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
  • German Electron Synchrotron
  • Stanford University
  • Tokyo Institute of Technology
  • National Institute for Nuclear Physics
  • University of Trieste
  • Rice University
  • University of Padua
  • University of Perugia
  • Polytechnic University of Bari
  • Laboratoire Leprince-Ringuet
  • CSIC
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • CEA-IRFU/CNRS/Université Paris Diderot
  • George Mason University
  • Naval Research Laboratory
  • ASI Science Data Center
  • Université Montpellier 2
  • Stockholm University
  • Oskar Klein Centre
  • Italian Space Agency
  • National Institute for Astrophysics
  • University of Udine
  • Hiroshima University
  • NASA Goddard Space Flight Center
  • University of Hertfordshire
  • Max Planck Institute for Extraterrestrial Physics
  • University of Alabama in Huntsville
  • Kyoto University
  • Ohio State University
  • KTH Royal Institute of Technology
  • University of Iceland
  • IRAP
  • University of Maryland
  • Pennsylvania State University
  • Boise State University
  • JAXA Institute of Space and Astronautical Science
  • Max Planck Institute for Physics (Werner Heisenberg Institute)
  • University of Maryland Baltimore County
  • Harvard & Smithsonian
  • University of California at Santa Cruz
  • Innsbruck Medical University
  • University of Washington
  • Max Planck Institute for Nuclear Physics
  • NYCB Real-Time Computing Inc.
  • Adiyaman University
  • Universities Space Research Association
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • University of Rome Tor Vergata
  • University College Dublin
  • Los Alamos National Laboratory
  • NASA Marshall Space Flight Center
  • Technical University of Munich
  • Karl Schwarzschild Observatory
  • Czech Technical University in Prague
  • University of Copenhagen
  • National Institutes of Natural Sciences - National Astronomical Observatory of Japan
  • Nagoya University
  • Victoria University of Wellington
  • University College London
  • Michigan State University
  • University of Leicester

Research output: Contribution to journalArticlepeer-review

89 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
Externally publishedYes

Keywords

  • gamma-ray burst: individual (GRB110731A)

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'Multiwavelength observations of GRB 110731A: GeV emission from onset to afterglow'. Together they form a unique fingerprint.

Cite this