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Detection of high-energy gamma-ray emission during the X-ray flaring activity in GRB 100728A

  • A. A. Abdo
  • , M. Ackermann
  • , M. Ajello
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , M. G. Baring
  • , D. Bastieri
  • , K. Bechtol
  • , R. Bellazzini
  • , B. Berenji
  • , P. N. Bhat
  • , E. Bissaldi
  • , R. D. Blandford
  • , E. Bonamente
  • , J. Bonnell
  • , A. W. Borgland
  • , A. Bouvier
  • , J. Bregeon
  • , M. Brigida
  • P. Bruel, R. Buehler, S. Buson, G. A. Caliandro, R. A. Cameron, P. A. Caraveo, J. M. Casandjian, C. Cecchi, E. Charles, A. Chekhtman, J. Chiang, S. Ciprini, R. Claus, V. Connaughton, J. Conrad, S. Cutini, A. De Angelis, F. De Palma, C. D. Dermer, E. Do Couto E Silva, P. S. Drell, R. Dubois, C. Favuzzi, Y. Fukazawa, P. Fusco, F. Gargano, N. Gehrels, S. Germani, N. Giglietto, P. Giommi, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, J. Granot, I. A. Grenier, S. Guiriec, D. Hadasch, Y. Hanabata, R. E. Hughes, G. Jóhannesson, A. S. Johnson, T. Kamae, H. Katagiri, J. Kataoka, M. Kerr, J. Knödlseder, M. Kuss, J. Lande, L. Latronico, S. H. Lee, F. Longo, F. Loparco, B. Lott, P. Lubrano, M. N. Mazziotta, J. E. McEnery, P. Mészros, P. F. Michelson, T. Mizuno, A. A. Moiseev, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, T. Nakamori, M. Naumann-Godo, P. L. Nolan, J. P. Norris, E. Nuss, T. Ohsugi, A. Okumura, N. Omodei, E. Orlando, W. S. Paciesas, V. Pelassa, M. Pesce-Rollins, M. Pierbattista, F. Piron, T. A. Porter, J. L. Racusin, S. Rainò, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, L. C. Reyes, M. Roth, H. F.W. Sadrozinski, C. Sgrò, E. J. Siskind, P. D. Smith, E. Sonbas, G. Spandre, P. Spinelli, M. Stamatikos, M. S. Strickman, H. Takahashi, T. Tanaka, Y. Tanaka, J. G. Thayer, J. B. Thayer, D. F. Torres, G. Tosti, E. Troja, T. Uehara, T. L. Usher, J. Vandenbroucke, V. Vasileiou, G. Vianello, N. Vilchez, V. Vitale, A. Von Kienlin, A. P. Waite, P. Wang, B. L. Winer, K. S. Wood, R. Yamazaki, Z. Yang, M. Ziegler, L. Piro
  • George Mason University
  • Naval Research Laboratory
  • Stanford Linear Accelerator Center
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • Universite Paris-Saclay
  • INFN Sezione di Trieste
  • University of Trieste
  • Rice University
  • INFN
  • University of Padova
  • Center for Space Plasma and Aeronomic Research
  • Medical University of Innsbruck
  • INFN Sezione di Perugia
  • University of Perugia
  • NASA Goddard Space Flight Center
  • University of Maryland
  • University of California at Santa Cruz
  • Politecnico di Bari
  • INFN Sezione di Bari
  • University of São Paulo
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Artep Inc.
  • Stockholm University
  • Oskar Klein Centre
  • Science and Research Directorate
  • and Physics University of Udine
  • Hiroshima University
  • INAF Istituto di Radioastronomia
  • University of Hertfordshire
  • The Ohio State University
  • University of Iceland
  • Waseda University
  • IRAP/CNRS
  • Univ. Bordeaux
  • Pennsylvania State University
  • Sezione di Roma
  • University of Denver
  • Laboratoire Univers et Particules de Montpellier
  • ISAS/JAXA
  • Max Planck Institut für Extraterrestrische Physik
  • University of Chicago
  • University of Washington
  • NYCB Real-Time Computing Inc.
  • Adiyaman University
  • Universities Space Research Association
  • Pompeu Fabra University (UPF)
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • University of Rome “Tor Vergata”
  • Aoyama Gakuin University
  • INAF-IASF

Research output: Contribution to journalArticlepeer-review

44 Citations (Scopus)

Abstract

We present the simultaneous Swift and Fermi observations of the bright GRB 100728A and its afterglow. The early X-ray emission is dominated by a vigorous flaring activity continuing until 1ks after the burst. In the same time interval, high-energy emission is significantly detected by the Fermi/Large Area Telescope. Marginal evidence ofGeV emission is observed up to later times. We discuss the broadband properties of this burst within both the internal and external shock scenarios, with a particular emphasis on the relation between X-ray flares, theGeV emission, and a continued long-duration central engine activity as their power source.

Original languageEnglish
Article numberL27
JournalAstrophysical Journal Letters
Volume734
Issue number2 PART 2
DOIs
Publication statusPublished - 20 Jun 2011

Keywords

  • gamma-ray burst: individual (GRB100728A)
  • radiation mechanisms: non-thermal

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