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The first catalog of active galactic nuclei detected by the Fermi large area telescope

  • A. A. Abdo
  • , M. Ackermann
  • , M. Ajello
  • , A. Allafort
  • , E. Antolini
  • , W. B. Atwood
  • , M. Axelsson
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , D. Bastieri
  • , B. M. Baughman
  • , K. Bechtol
  • , R. Bellazzini
  • , B. Berenji
  • , R. D. Blandford
  • , E. D. Bloom
  • , J. R. Bogart
  • , E. Bonamente
  • , A. W. Borgland
  • A. Bouvier, J. Bregeon, A. Brez, M. Brigida, P. Bruel, R. Buehler, T. H. Burnett, S. Buson, G. A. Caliandro, R. A. Cameron, A. Cannon, P. A. Caraveo, S. Carrigan, J. M. Casandjian, E. Cavazzuti, C. Cecchi, Ö Çelik, A. Celotti, E. Charles, A. Chekhtman, A. W. Chen, C. C. Cheung, J. Chiang, S. Ciprini, R. Claus, J. Cohen-Tanugi, J. Conrad, L. Costamante, G. Cotter, S. Cutini, V. D'Elia, C. D. Dermer, A. De Angelis, F. De Palma, A. De Rosa, S. W. Digel, E. Do Couto E Silva, P. S. Drell, R. Dubois, D. Dumora, L. Escande, C. Farnier, C. Favuzzi, S. J. Fegan, E. C. Ferrara, W. B. Focke, P. Fortin, M. Frailis, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, N. Gehrels, S. Germani, B. Giebels, N. Giglietto, P. Giommi, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, P. Grandi, I. A. Grenier, M. H. Grondin, J. E. Grove, S. Guiriec, D. Hadasch, A. K. Harding, M. Hayashida, E. Hays, S. E. Healey, A. B. Hill, D. Horan, R. E. Hughes, G. Iafrate, R. Itoh, G. Jóhannesson, A. S. Johnson, R. P. Johnson, T. J. Johnson, W. N. Johnson, T. Kamae, H. Katagiri, J. Kataoka, N. Kawai, M. Kerr, J. Knödlseder, M. Kuss, J. Lande, L. Latronico, C. Lavalley, M. Lemoine-Goumard, M. Llena Garde, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, G. M. Madejski, A. Makeev, G. Malaguti, E. Massaro, M. N. Mazziotta, W. McConville, J. E. McEnery, S. McGlynn, 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, M. Ohno, 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, S. Piranomonte, F. Piron, T. A. Porter, S. Rainò, R. Rando, M. Razzano, A. Reimer, O. Reimer, T. Reposeur, J. Ripken, S. Ritz, A. Y. Rodriguez, R. W. Romani, M. Roth, F. Ryde, H. F.W. Sadrozinski, D. Sanchez, A. Sander, P. M. Saz Parkinson, J. D. Scargle, C. Sgrò, M. S. Shaw, E. J. Siskind, P. D. Smith, G. Spandre, P. Spinelli, J. L. Starck, L. Stawarz, M. S. Strickman, D. J. Suson, H. Tajima, H. Takahashi, T. Takahashi, T. Tanaka, G. B. Taylor, J. B. Thayer, J. G. Thayer, D. J. Thompson, L. Tibaldo, D. F. Torres, G. Tosti, A. Tramacere, P. Ubertini, Y. Uchiyama, T. L. Usher, V. Vasileiou, N. Vilchez, M. Villata, V. Vitale, A. P. Waite, E. Wallace, P. Wang, B. L. Winer, K. S. Wood, Z. Yang, T. Ylinen, M. Ziegler
  • Naval Research Laboratory
  • National Research Council
  • Stanford University
  • INFN Sezione di Perugia
  • University of Perugia
  • University of California at Santa Cruz
  • Stockholm University
  • Oskar Klein Centre
  • Universite Paris-Saclay
  • INFN Sezione di Trieste
  • University of Trieste
  • INFN
  • University of Padova
  • The Ohio State University
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • Politecnico di Bari
  • INFN Sezione di Bari
  • University of Washington
  • University of São Paulo
  • NASA Goddard Space Flight Center
  • University College Dublin
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Science and Research Directorate
  • Biochemical and Environmental Engineering
  • International School of Advanced Studies
  • George Mason University
  • Laboratoire Univers et Particules de Montpellier
  • University of Oxford
  • Sezione di Roma
  • INAF-IASF
  • Université Paris-Sud
  • Univ. Bordeaux
  • Hiroshima University
  • Pennsylvania State University
  • University of Maryland
  • INAF Istituto di Radioastronomia
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna
  • Center for Space Plasma and Aeronomic Research
  • Pompeu Fabra University (UPF)
  • LTHE (UMR 5564 CNRS/IRD/Université de Grenoble)
  • INAF-Trieste
  • Waseda University
  • Tokyo Institute of Technology
  • RIKEN (The Institute of Physical and Chemical Research)
  • CNRS
  • University of Rome
  • KTH Royal Institute of Technology
  • University of Denver
  • ISAS/JAXA
  • Max Planck Institut für Extraterrestrische Physik
  • Osservatorio Astronomico di Roma
  • Medical University of Innsbruck
  • NASA Ames Research Center
  • NYCB Real-Time Computing Inc.
  • Jagiellonian University
  • Purdue University Northwest
  • University of New Mexico
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • University of Geneva
  • Osservatorio Astronomico di Torino
  • University of Rome “Tor Vergata”
  • University of Kalmar

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

We present the first catalog of active galactic nuclei (AGNs) detected by the Large Area Telescope (LAT), corresponding to 11 months of data collected in scientific operation mode. The First LAT AGN Catalog (1LAC) includes 671 γ-ray sources located at high Galactic latitudes (|b|>10°) that are detected with a test statistic greater than 25 and associated statistically with AGNs. Some LAT sources are associated with multiple AGNs, and consequently, the catalog includes 709 AGNs, comprising 300 BL Lacertae objects, 296 flat-spectrum radio quasars, 41 AGNs of other types, and 72 AGNs of unknown type. We also classify the blazars based on their spectral energy distributions as archival radio, optical, and X-ray data permit. In addition to the formal 1LAC sample, we provide AGN associations for 51 low-latitude LAT sources and AGN "affiliations" (unquantified counterpart candidates) for 104 high-latitude LAT sources without AGN associations. The overlap of the 1LAC with existing γ-ray AGN catalogs (LBAS, EGRET, AGILE, Swift, INTEGRAL, TeVCat) is briefly discussed. Various properties - such as γ-ray fluxes and photon power-law spectral indices, redshifts, γ-ray luminosities, variability, and archival radio luminosities - and their correlations are presented and discussed for the different blazar classes. We compare the 1LAC results with predictions regarding the γ-ray AGN populations, and we comment on the power of the sample to address the question of the blazar sequence.

langue originaleAnglais
Pages (de - à)429-457
Nombre de pages29
journalAstrophysical Journal
Volume715
Numéro de publication1
Les DOIs
étatPublié - 1 janv. 2010

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