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Fermi observations of high-energy gamma-ray emission from GRB 090217A

  • 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
  • , A. W. Borgland
  • , A. Bouvier
  • , J. Bregeon
  • , A. Brez
  • , M. S. Briggs
  • , M. Brigida
  • P. Bruel, R. Buehler, S. Buson, G. A. Caliandro, R. A. Cameron, P. A. Caraveo, S. Carrigan, J. M. Casandjian, C. Cecchi, Ö Çelik, E. Charles, A. Chekhtman, J. Chiang, S. Ciprini, R. Claus, J. Cohen-Tanugi, V. Connaughton, J. Conrad, S. Cutini, C. D. Dermer, A. De Angelis, F. De Palma, S. W. Digel, E. Do Couto E Silva, P. S. Drell, R. Dubois, C. Favuzzi, S. J. Fegan, E. C. Ferrara, M. Frailis, Y. Fukazawa, P. Fusco, F. Gargano, D. Gasparrini, N. Gehrels, S. Germani, N. Giglietto, P. Giommi, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, J. Granot, I. A. Grenier, J. E. Grove, L. Guillemot, S. Guiriec, D. Hadasch, E. Hays, D. Horan, R. E. Hughes, G. Jóhannesson, A. S. Johnson, W. N. Johnson, T. Kamae, H. Katagiri, R. M. Kippen, J. Knödlseder, D. Kocevski, M. Kuss, J. Lande, L. Latronico, S. H. Lee, M. Llena Garde, F. Longo, F. Loparco, M. N. Lovellette, P. Lubrano, A. Makeev, M. N. Mazziotta, S. McBreen, J. E. McEnery, S. McGlynn, C. Meegan, J. Mehault, P. Mészros, P. F. Michelson, T. Mizuno, A. A. Moiseev, C. Monte, M. E. Monzani, E. Moretti, A. Morselli, I. V. Moskalenko, S. Murgia, H. Nakajima, T. Nakamori, M. Naumann-Godo, P. L. Nolan, J. P. Norris, E. Nuss, M. Ohno, T. Ohsugi, A. Okumura, N. Omodei, E. Orlando, J. F. Ormes, M. Ozaki, W. S. Paciesas, D. Paneque, J. H. Panetta, D. Parent, V. Pelassa, M. Pepe, M. Pesce-Rollins, V. Petrosian, F. Piron, T. A. Porter, R. Preece, J. L. Racusin, S. Rainò, R. Rando, A. Rau, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, J. Ripken, M. Roth, F. Ryde, H. F.W. Sadrozinski, A. Sander, J. D. Scargle, T. L. Schalk, C. Sgrò, E. J. Siskind, P. D. Smith, G. Spandre, P. Spinelli, M. Stamatikos, M. S. Strickman, D. J. Suson, H. Tajima, H. Takahashi, T. Tanaka, J. B. Thayer, J. G. Thayer, L. Tibaldo, D. F. Torres, G. Tosti, A. Tramacere, T. Uehara, T. L. Usher, J. Vandenbroucke, A. J. Van Der Horst, V. Vasileiou, N. Vilchez, V. Vitale, A. Von Kienlin, A. P. Waite, P. Wang, C. Wilson-Hodge, B. L. Winer, K. S. Wood, X. F. Wu, R. Yamazaki, Z. Yang, T. Ylinen, M. Ziegler
  • Stanford University
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • Laboratoire AIM
  • Universite Paris-Saclay
  • 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 G. Galilei
  • University of Padova
  • Center for Space Plasma and Aeronomic Research
  • Max Planck Institut für Extraterrestrische Physik
  • Sezione di Perugia
  • INFN Sezione di Perugia
  • INFM CRS-SOFT
  • University of Perugia
  • Politecnico di Bari
  • INFN
  • INFN Sezione di Bari
  • University of São Paulo
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • NASA Goddard Space Flight Center
  • Center for Research and Exploration in Space Science and Technology (CRESST)
  • Department of Physics
  • Biochemical and Environmental Engineering
  • Space Science Division
  • Naval Research Laboratory
  • George Mason University
  • Laboratoire Univers et Particules de Montpellier
  • Department of Physics
  • Stockholm University
  • Oskar Klein Centre
  • Space Science Data Center
  • Science and Research Directorate
  • Dipartimento di Fisica
  • and Physics University of Udine
  • INAF-Trieste
  • Department of Physical Science
  • Hiroshima University
  • INAF Istituto di Radioastronomia
  • Centre for Astrophysics Research
  • University of Hertfordshire
  • Max-Planck-Institut für Radioastronomie
  • Université Paris-Sud
  • Univ. Bordeaux
  • Pompeu Fabra University (UPF)
  • Department of Physics
  • The Ohio State University
  • MST-8, Los Alamos National Laboratory
  • Centre national de la recherche scientifique
  • University College Dublin
  • University of Maryland
  • KTH Royal Institute of Technology
  • Universities Space Research Association
  • Department of Astronomy and Astrophysics
  • Pennsylvania State University
  • Sezione di Roma
  • Department of Physics
  • Tokyo Institute of Technology
  • Research Institute for Science and Engineering
  • Waseda University
  • Department of Physics and Astronomy
  • University of Denver
  • ISAS/JAXA
  • Hiroshima Astrophysical Science Center
  • National Research Council
  • Medical University of Innsbruck
  • Department of Physics
  • University of Washington
  • University of California at Santa Cruz
  • National Aeronautics and Space Administration (NASA)
  • NASA Ames Research Center
  • NYCB Real-Time Computing Inc.
  • Department of Chemistry and Physics
  • Purdue University Northwest
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • University of Geneva
  • NASA Marshall Space Flight Center
  • Dipartimento di Fisica
  • University of Rome “Tor Vergata”
  • Joint Center for Particle Nuclear Physics and Cosmology (J-CPNPC)
  • Purple Mountain Observatory Chinese Academy of Sciences
  • Aoyama Gakuin University
  • School of Pure and Applied Natural Sciences
  • University of Kalmar

Research output: Contribution to journalArticlepeer-review

32 Citations (Scopus)

Abstract

The Fermi observatory is advancing our knowledge of gamma-ray bursts (GRBs) through pioneering observations at high energies, covering more than seven decades in energy with the two on-board detectors, the Large Area Telescope (LAT) and the Gamma-ray Burst Monitor (GBM). Here, we report on the observation of the long GRB 090217A which triggered the GBM and has been detected by the LAT with a significance greater than 9σ. We present the GBM and LAT observations and on-ground analyses, including the time-resolved spectra and the study of the temporal profile from 8 keV up to 1 GeV. All spectra are well reproduced by a Band model. We compare these observations to the first two LAT-detected, long bursts GRB 080825C and GRB 080916C. These bursts were found to have time-dependent spectra and exhibited a delayed onset of the high-energy emission, which are not observed in the case of GRB 090217A. We discuss some theoretical implications for the high-energy emission of GRBs.

Original languageEnglish
Pages (from-to)L127-L132
JournalAstrophysical Journal Letters
Volume717
Issue number2 PART 2
DOIs
Publication statusPublished - 1 Jan 2010

Keywords

  • gamma-ray burst: individual (GRB090217A)

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