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GeV gamma-ray flux upper limits from clusters of galaxies

  • M. Ackermann
  • , M. Ajello
  • , A. Allafort
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , D. Bastieri
  • , K. Bechtol
  • , R. Bellazzini
  • , R. D. Blandford
  • , P. Blasi
  • , E. D. Bloom
  • , E. Bonamente
  • , A. W. Borgland
  • , A. Bouvier
  • , T. J. Brandt
  • , J. Bregeon
  • , M. Brigida
  • , P. Bruel
  • , R. Buehler
  • S. Buson, G. A. Caliandro, R. A. Cameron, P. A. Caraveo, S. Carrigan, J. M. Casandjian, E. Cavazzuti, C. Cecchi, Çelik, E. Charles, A. Chekhtman, C. C. Cheung, J. Chiang, S. Ciprini, R. Claus, J. Cohen-Tanugi, S. Colafrancesco, L. R. Cominsky, J. Conrad, C. D. Dermer, F. De Palma, E. Do Couto E Silva, P. S. Drell, R. Dubois, D. Dumora, Y. Edmonds, C. Farnier, C. Favuzzi, M. Frailis, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, N. Gehrels, S. Germani, N. Giglietto, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, I. A. Grenier, M. H. Grondin, S. Guiriec, D. Hadasch, A. K. Harding, M. Hayashida, E. Hays, D. Horan, R. E. Hughes, T. E. Jeltema, G. Jóhannesson, A. S. Johnson, T. J. Johnson, W. N. Johnson, T. Kamae, H. Katagiri, J. Kataoka, M. Kerr, J. Knödlseder, M. Kuss, J. Lande, L. Latronico, S. H. Lee, M. Lemoine-Goumard, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, G. M. Madejski, A. Makeev, M. N. Mazziotta, P. F. Michelson, W. Mitthumsiri, T. Mizuno, A. A. Moiseev, C. Monte, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, M. Naumann-Godo, P. L. Nolan, J. P. Norris, E. Nuss, T. Ohsugi, N. Omodei, E. Orlando, J. F. Ormes, M. Ozaki, D. Paneque, J. H. Panetta, M. Pepe, M. Pesce-Rollins, V. Petrosian, C. Pfrommer, F. Piron, T. A. Porter, S. Profumo, S. Rainò, R. Rando, M. Razzano, A. Reimer, O. Reimer, T. Reposeur, J. Ripken, S. Ritz, A. Y. Rodriguez, R. W. Romani, M. Roth, H. F.W. Sadrozinski, A. Sander, P. M. Saz Parkinson, J. D. Scargle, C. Sgrò, E. J. Siskind, P. D. Smith, G. Spandre, P. Spinelli, J. L. Starck, Stawarz, M. S. Strickman, A. W. Strong, D. J. Suson, H. Tajima, H. Takahashi, T. Takahashi, T. Tanaka, J. B. Thayer, J. G. Thayer, L. Tibaldo, O. Tibolla, D. F. Torres, G. Tosti, A. Tramacere, Y. Uchiyama, T. L. Usher, J. Vandenbroucke, V. Vasileiou, N. Vilchez, V. Vitale, A. P. Waite, P. Wang, B. L. Winer, K. S. Wood, Z. Yang, T. Ylinen, M. Ziegler
  • Kavli Institute for Particle Astrophysics and Cosmology
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • Universite Paris-Saclay
  • INFN Sezione di Trieste
  • University of Trieste
  • INFN
  • University of Padova
  • Osservatorio Astrofisico Di Arcetri
  • INFN Sezione di Perugia
  • University of Perugia
  • CNRS
  • The Ohio State University
  • Politecnico di Bari
  • INFN Sezione di Bari
  • Campus UAB
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Science and Research Directorate
  • NASA Goddard Space Flight Center
  • Biochemical and Environmental Engineering
  • Naval Research Laboratory
  • George Mason University
  • National Research Council
  • Laboratoire Univers et Particules de Montpellier
  • Sonoma State University
  • Stockholm University
  • Oskar Klein Centre
  • Royal Swedish Academy of Sciences
  • Université Paris-Sud
  • Univ. Bordeaux
  • and Physics University of Udine
  • INAF-Trieste
  • Hiroshima University
  • INAF Istituto di Radioastronomia
  • Center for Space Plasma and Aeronomic Research
  • Pompeu Fabra University (UPF)
  • University of California at Santa Cruz
  • University of Maryland
  • Waseda University
  • University of Washington
  • INFN Roma Tor Vergata
  • University of Denver
  • Max Planck Institut für Extraterrestrische Physik
  • ISAS/JAXA
  • University of Toronto
  • Medical University of Innsbruck
  • NASA Ames Research Center
  • NYCB Real-Time Computing Inc.
  • Jagiellonian University
  • Purdue University Northwest
  • University of Würzburg
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • University of Geneva
  • University of Rome “Tor Vergata”
  • KTH Royal Institute of Technology
  • University of Kalmar

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

158 Citations (Scopus)

Résumé

The detection of diffuse radio emission associated with clusters of galaxies indicates populations of relativistic leptons infusing the intraclustermedium (ICM). Those electrons and positrons are either injected into and accelerated directly in the ICM, or produced as secondary pairs by cosmic-ray ions scattering on ambient protons. Radiation mechanisms involving the energetic leptons together with the decay of neutral pions produced by hadronic interactions have the potential to produce abundant GeV photons. Here, we report on the search for GeV emission from clusters of galaxies using data collected by the Large Area Telescope on the FermiGamma-ray Space Telescope from 2008 August to 2010 February. Thirty-three galaxy clusters have been selected according to their proximity and high mass, X-ray flux and temperature, and indications of non-thermal activity for this study. We report upper limits on the photon flux in the range 0.2-100GeVtoward a sample of observed clusters (typical values (1-5)×10-9 photon cm-2 s-1) considering both point-like and spatially resolved models for the high-energy emission and discuss how these results constrain the characteristics of energetic leptons and hadrons, and magnetic fields in the ICM. The volume-averaged relativistic-hadron-to-thermal energy density ratio is found to be <5%-10% in several clusters.

langue originaleAnglais
Pages (de - à)L71-L78
journalAstrophysical Journal Letters
Volume717
Numéro de publication1
Les DOIs
étatPublié - 1 juil. 2010

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