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Fermi observations of TeV-Selected active galactic nuclei

  • A. A. Abdo
  • , M. Ackermann
  • , M. Ajello
  • , W. B. Atwood
  • , M. Axelsson
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , M. G. Baring
  • , D. Bastieri
  • , K. Bechtol
  • , R. Bellazzini
  • , B. Berenji
  • , E. D. Bloom
  • , E. Bonamente
  • , A. W. Borgland
  • , J. Bregeon
  • , A. Brez
  • , M. Brigida
  • , P. Bruel
  • T. H. Burnett, G. A. Caliandro, R. A. Cameron, P. A. Caraveo, J. M. Casandjian, E. Cavazzuti, C. Cecchi, Ö Çelik, A. Chekhtman, C. C. Cheung, J. Chiang, S. Ciprini, R. Claus, J. Cohen-Tanugi, L. R. Cominsky, J. Conrad, S. Cutini, A. De Angelis, F. De Palma, G. Di Bernardo, E. Do Couto E Silva, P. S. Drell, A. Drlica-Wagner, R. Dubois, D. Dumora, C. Farnier, C. Favuzzi, S. J. Fegan, J. Finke, W. B. Focke, P. Fortin, L. Foschini, M. Frailis, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, N. Gehrels, S. Germani, G. Giavitto, B. Giebels, N. Giglietto, P. Giommi, F. Giordano, T. Glanzman, G. Godfrey, I. A. Grenier, M. H. Grondin, J. E. Grove, L. Guillemot, S. Guiriec, Y. Hanabata, M. Hayashida, E. Hays, D. Horan, R. E. Hughes, M. S. Jackson, G. Jóhannesson, A. S. Johnson, R. P. Johnson, W. N. Johnson, T. Kamae, H. Katagiri, J. Kataoka, N. Kawai, M. Kerr, J. Knödlseder, M. L. Kocian, M. Kuss, J. Lande, L. Latronico, M. Lemoine-Goumard, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, G. M. Madejski, A. Makeev, M. N. Mazziotta, W. McConville, J. E. McEnery, C. Meurer, P. F. Michelson, W. Mitthumsiri, T. Mizuno, A. A. Moiseev, C. Monte, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, P. L. Nolan, J. P. Norris, E. Nuss, T. Ohsugi, N. Omodei, E. Orlando, J. F. Ormes, M. Ozaki, D. Paneque, J. H. Panetta, D. Parent, V. Pelassa, M. Pepe, M. Pesce-Rollins, F. Piron, T. A. Porter, S. Rainò, R. Rando, M. Razzano, A. Reimer, O. Reimer, T. Reposeur, L. C. Reyes, S. Ritz, L. S. Rochester, A. Y. Rodriguez, M. Roth, F. Ryde, H. F.W. Sadrozinski, D. Sanchez, A. Sander, P. M.Saz Parkinson, J. D. Scargle, T. L. Schalk, A. Sellerholm, C. Sgrò, M. S. Shaw, E. J. Siskind, D. A. Smith, P. D. Smith, G. Spandre, P. Spinelli, M. S. Strickman, D. J. Suson, H. Tajima, H. Takahashi, T. Takahashi, T. Tanaka, Y. Tanaka, J. B. Thayer, J. G. Thayer, D. J. Thompson, L. Tibaldo, D. F. Torres, G. Tosti, A. Tramacere, Y. Uchiyama, T. L. Usher, V. Vasileiou, N. Vilchez, V. Vitale, A. P. Waite, P. Wang, B. L. Winer, K. S. Wood, T. Ylinen, M. Ziegler
  • Space Science Division
  • Naval Research Laboratory
  • National Research Council
  • Stanford Linear Accelerator Center
  • University of California at Santa Cruz
  • Department of Astronomy
  • Stockholm University
  • Oskar Klein Centre
  • 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
  • Sezione di Perugia
  • INFN Sezione di Perugia
  • INFM CRS-SOFT
  • University of Perugia
  • Politecnico di Bari
  • INFN
  • INFN Sezione di Bari
  • Department of Physics
  • University of Washington
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Space Science Data Center
  • Science and Research Directorate
  • NASA Goddard Space Flight Center
  • Center for Research and Exploration in Space Science and Technology (CRESST)
  • Baltimore County
  • Biochemical and Environmental Engineering
  • George Mason University
  • Laboratoire Univers et Particules de Montpellier
  • Sonoma State University
  • Department of Physics
  • KTH Royal Institute of Technology
  • Royal Swedish Academy of Sciences
  • Dipartimento di Fisica
  • and Physics University of Udine
  • Univ. Bordeaux
  • Université Paris-Sud
  • Ip Paris
  • INAF
  • Department of Physical Science
  • Hiroshima University
  • University of Maryland, College Park
  • Istituto Nazionale di Fisica Nucleare
  • University of Alabama in Huntsville
  • Department of Physics
  • The Ohio State University
  • Department of Physics
  • Tokyo Institute of Technology
  • Waseda University
  • Cosmic Radiation Laboratory
  • RIKEN (The Institute of Physical and Chemical Research)
  • CNRS
  • Sezione di Roma
  • Department of Physics and Astronomy
  • University of Denver
  • Max Planck Institut für Extraterrestrische Physik
  • ISAS/JAXA
  • Medical University of Innsbruck
  • University of Chicago
  • University of São Paulo
  • National Aeronautics and Space Administration (NASA)
  • NASA Ames Research Center
  • NYCB Real-Time Computing Inc.
  • Department of Chemistry and Physics
  • Purdue University Northwest
  • Pompeu Fabra University (UPF)
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • Dipartimento di Fisica
  • University of Rome “Tor Vergata”
  • School of Pure and Applied Natural Sciences
  • University of Kalmar

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

140 Citations (Scopus)

Résumé

We report on observations of TeV-selected active galactic nuclei (AGNs) made during the first 5.5 months of observations with the Large Area Telescope (LAT) on-board the Fermi Gamma-ray Space Telescope (Fermi). In total, 96 AGNs were selected for study, each being either (1) a source detected at TeV energies (28 sources) or (2) an object that has been studied with TeV instruments and for which an upper limit has been reported (68 objects). The Fermi observations show clear detections of 38 of these TeV-selected objects, of which 21 are joint GeV-TeV sources, and 29 were not in the third EGRET catalog. For each of the 38 Fermi-detected sources, spectra and light curves are presented. Most can be described with a power law of spectral index harder than 2.0, with a spectral break generally required to accommodate the TeV measurements. Based on an extrapolation of the Fermi spectrum, we identify sources, not previously detected at TeV energies, which are promising targets for TeV instruments. Evidence for systematic evolution of the γ-ray spectrum with redshift is presented and discussed in the context of interaction with the extragalactic background light.

langue originaleAnglais
Pages (de - à)1310-1333
Nombre de pages24
journalAstrophysical Journal
Volume707
Numéro de publication2
Les DOIs
étatPublié - 1 janv. 2009

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