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Bright active galactic nuclei source list from the first three months of the Fermi large area telescope all-sky survey

  • A. A. Abdo
  • , M. Ackermann
  • , M. Ajello
  • , W. B. Atwood
  • , M. Axelsson
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , D. Bastieri
  • , B. M. Baughman
  • , K. Bechtol
  • , R. Bellazzini
  • , R. D. Blandford
  • , E. D. Bloom
  • , E. Bonamente
  • , A. W. Borgland
  • , A. Bouvier
  • , 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, E. Charles, A. Chekhtman, A. W. Chen, C. C. Cheung, J. Chiang, S. Ciprini, R. Claus, J. Cohen-Tanugi, S. Colafrancesco, W. Collmar, L. R. Cominsky, J. Conrad, L. Costamante, S. Cutini, C. D. Dermer, A. De Angelis, F. De Palma, S. W. Digel, E. Do Couto e Silva, P. S. Drell, R. Dubois, D. Dumora, C. Farnier, C. Favuzzi, S. J. Fegan, E. C. Ferrara, J. Finke, W. B. Focke, L. Foschini, M. Frailis, L. Fuhrmann, 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, I. A. Grenier, M. H. Grondin, J. E. Grove, L. Guillemot, S. Guiriec, Y. Hanabata, A. K. Harding, R. C. Hartman, M. Hayashida, E. Hays, S. E. Healey, D. Horan, R. E. Hughes, G. Jóhannesson, A. S. Johnson, R. P. Johnson, T. J. Johnson, W. N. Johnson, M. Kadler, T. Kamae, H. Katagiri, J. Kataoka, M. Kerr, J. Knödlseder, M. L. Kocian, F. Kuehn, 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, E. Massaro, M. N. Mazziotta, W. McConville, J. E. McEnery, S. McGlynn, C. Meurer, P. F. Michelson, W. Mitthumsiri, T. Mizuno, A. A. Moiseev, C. Monte, M. E. Monzani, E. Moretti, 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, S. Razzaque, A. Reimer, O. Reimer, T. Reposeur, L. C. Reyes, S. Ritz, L. S. Rochester, A. Y. Rodriguez, R. W. Romani, 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, D. A. Smith, P. D. Smith, G. Spandre, P. Spinelli, J. L. Starck, 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, Y. Uchiyama, T. L. Usher, N. Vilchez, M. Villata, V. Vitale, A. P. Waite, B. L. Winer, K. S. Wood, T. Ylinen, M. Ziegler
  • Naval Research Laboratory
  • Kavli Institute for Particle Astrophysics and Cosmology
  • SLAC National Accelerator Laboratory
  • Oskar Klein Centre
  • Stockholm University
  • National Institute for Nuclear Physics
  • CEA-IRFU/CNRS/Université Paris Diderot
  • University of Trieste
  • University of Padua
  • Ohio State University
  • University of Perugia
  • Polytechnic University of Bari
  • IN2P3 - Institut National de Physique Nucléaire et de Physique Des Particules
  • University of Washington
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • Italian Space Agency
  • George Mason University
  • NASA Goddard Space Flight Center
  • Université Montpellier 2
  • Max Planck Institute for Extraterrestrial Physics
  • Sonoma State University
  • KTH Royal Institute of Technology
  • University of Udine
  • Centre d'Etudes Nucléaires Bordeaux-Gradingnan (CENBG)
  • Université de Bordeaux
  • Osservatorio Astronomico di Brera
  • Max Planck Institute for Radio Astronomy
  • Hiroshima University
  • University of Maryland, College Park
  • National Institute for Astrophysics
  • University of Alabama in Huntsville
  • University of California at Santa Cruz
  • Dr. Remeis-Sternwarte Bamberg
  • Friedrich-Alexander University Erlangen-Nürnberg
  • Universities Space Research Association
  • Waseda University
  • CNRS
  • University of Rome La Sapienza
  • University of Denver
  • JAXA Institute of Space and Astronautical Science
  • The University of Chicago
  • Autonomous University of Barcelona
  • NASA Ames Research Center
  • Purdue University Northwest
  • University of New Mexico
  • ICREA
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • Osservatorio Astronomico di Torino
  • University of Rome Tor Vergata
  • Linnaeus University

Research output: Contribution to journalArticlepeer-review

394 Citations (Scopus)

Abstract

The first three months of sky-survey operation with the Large Area Telescope (LAT) onboard the Fermi Gamma-Ray Space Telescope reveal 132 bright sources at |b| > 10° with test statistic greater than 100 (corresponding to about 10σ). Two methods, based on the CGRaBS, CRATES, and BZCat catalogs, indicate high-confidence associations of 106 of these sources with known active galactic nuclei (AGNs). This sample is referred to as the LAT Bright AGN Sample (LBAS). It contains two radio galaxies, namely, Centaurus A and NGC 1275, and 104 blazars consisting of 58 flat spectrum radio quasars (FSRQs), 42 BL Lac objects, and 4 blazars with unknown classification. Four new blazars were discovered on the basis of the LAT detections. Remarkably, the LBAS includes 10 high-energy-peaked BL Lacs (HBLs), sources which were previously difficult to detect in the GeV range. Another 10 lower-confidence associations are found. Only 33 of the sources, plus two at |b| < 10°, were previously detected with Energetic Gamma-Ray Experiment Telescope(EGRET), probably due to variability. The analysis of the γ-ray properties of the LBAS sources reveals that the average GeV spectra of BL Lac objects are significantly harder than the spectra of FSRQs. No significant correlation between radio and peak γ-ray fluxes is observed. Blazar log N-log S distributions and luminosity functions are constructed to investigate the evolution of the different blazar classes, with positive evolution indicated for FSRQs but none for BL Lacs. The contribution of LAT blazars to the total extragalactic γ-ray intensity is estimated.

Original languageEnglish
Pages (from-to)597-622
Number of pages26
JournalAstrophysical Journal
Volume700
Issue number1
DOIs
Publication statusPublished - 20 Jul 2009
Externally publishedYes

Keywords

  • BL lacertae objects: General
  • Galaxies: Active
  • Galaxies: Jets
  • Gamma rays: Observations Online-only material: Color figures

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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