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Fermi large area telescope observations of blazar 3C 279 occultations by the sun

  • G. Barbiellini
  • , D. Bastieri
  • , K. Bechtol
  • , R. Bellazzini
  • , R. D. Blandford
  • , A. W. Borgland
  • , J. Bregeon
  • , P. Bruel
  • , R. Buehler
  • , S. Buson
  • , G. A. Caliandro
  • , R. A. Cameron
  • , P. A. Caraveo
  • , E. Cavazzuti
  • , C. Cecchi
  • , R. C.G. Chaves
  • , A. Chekhtman
  • , C. C. Cheung
  • , J. Chiang
  • , S. Ciprini
  • R. Claus, J. Cohen-Tanugi, F. D'Ammando, A. De Angelis, C. D. Dermer, S. W. Digel, E. Do Couto E. Silva, P. S. Drell, A. Drlica-Wagner, C. Favuzzi, W. B. Focke, A. Franckowiak, Y. Fukazawa, P. Fusco, F. Gargano, D. Gasparrini, S. Germani, N. Giglietto, P. Giommi, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, I. A. Grenier, J. E. Grove, S. Guiriec, D. Hadasch, M. Hayashida, E. Hays, R. E. Hughes, M. S. Jackson, T. Jogler, J. Knödlseder, M. Kuss, J. Lande, S. Larsson, F. Longo, F. Loparco, M. N. Lovellette, P. Lubrano, M. N. Mazziotta, J. Mehault, P. F. Michelson, T. Mizuno, A. A. Moiseev, C. Monte, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, R. Nemmen, E. Nuss, T. Ohsugi, N. Omodei, M. Orienti, E. Orlando, D. Paneque, J. S. Perkins, F. Piron, G. Pivato, D. Prokhorov, S. Rainò, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, S. Ritz, C. Romoli, M. Sánchez-Conde, D. A. Sanchez, C. Sgrò, E. J. Siskind, G. Spandre, P. Spinelli, H. Takahashi, T. Tanaka, 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
  • INFN Sezione di Trieste
  • University of Trieste
  • INFN
  • University of Padova
  • Stanford Linear Accelerator Center
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • University of Sheffield
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Science and Research Directorate
  • INFN Sezione di Perugia
  • University of Perugia
  • Universite Paris-Saclay
  • George Mason University
  • Naval Research Laboratory
  • National Research Council
  • Max Planck Institute for Astrophysics
  • Laboratoire Univers et Particules de Montpellier
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo
  • INAF-IASF
  • Sezione di Roma
  • Politecnico di Bari
  • INFN Sezione di Bari
  • Hiroshima University
  • INAF Istituto di Radioastronomia
  • NASA Goddard Space Flight Center
  • Kyoto University
  • The Ohio State University
  • KTH Royal Institute of Technology
  • Oskar Klein Centre
  • IRAP/CNRS
  • Stockholm University
  • University of Maryland
  • Max-Planck-Institut für Physik
  • Biochemical and Environmental Engineering
  • Center for Astrophysics | Harvard & Smithsonian
  • University of California at Santa Cruz
  • Medical University of Innsbruck
  • Max-Planck-Institut für Kernphysik
  • NYCB Real-Time Computing Inc.
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • University of Rome “Tor Vergata”

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

14 Citations (Scopus)

Résumé

Observations of occultations of bright γ-ray sources by the Sun may reveal predicted pair halos around blazars and/or new physics, such as, e.g., hypothetical light dark matter particles - axions. We use Fermi Gamma-Ray Space Telescope (Fermi) data to analyze four occultations of blazar 3C 279 by the Sun on October 8 each year from 2008 to 2011. A combined analysis of the observations of these occultations allows a point-like source at the position of 3C 279 to be detected with significance of 3σ, but does not reveal any significant excess over the flux expected from the quiescent Sun. The likelihood ratio test rules out complete transparency of the Sun to the blazar γ-ray emission at a 3σ confidence level.

langue originaleAnglais
Numéro d'article118
journalAstrophysical Journal
Volume784
Numéro de publication2
Les DOIs
étatPublié - 1 avr. 2014

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