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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
  • Space Science Division
  • Naval Research Laboratory
  • Kavli Institute for Particle Astrophysics and Cosmology
  • Stanford Linear Accelerator Center
  • Oskar Klein Centre
  • Department of Astronomy
  • Stockholm University
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • Universite Paris-Saclay
  • INFN Gruppo Collegato di Udine
  • INFN Sezione di Trieste
  • Dipartimento di Fisica
  • University of Trieste
  • INFN
  • Dipartimento di Fisica G. Galilei
  • University of Padova
  • Department of Physics
  • The Ohio State University
  • Sezione di Perugia
  • INFN Sezione di Perugia
  • INFM CRS-SOFT
  • University of Perugia
  • Politecnico di Bari
  • INFN
  • INFN Sezione di Bari
  • Université Paris-Sud
  • Department of Physics
  • University of Washington
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Space Science Data Center
  • Science and Research Directorate
  • George Mason University
  • NASA Goddard Space Flight Center
  • Laboratoire Univers et Particules de Montpellier
  • Max Planck Institut für Extraterrestrische Physik
  • Sonoma State University
  • KTH Royal Institute of Technology
  • Department of Physics
  • Dipartimento di Fisica
  • and Physics University of Udine
  • UMR 5797
  • Univ. Bordeaux
  • INAF
  • Max-Planck-Institut für Radioastronomie
  • Department of Physical Science
  • Hiroshima University
  • University of Maryland, College Park
  • Laboratoire Leprince-Ringuet
  • INAF Istituto di Radioastronomia
  • University of Alabama in Huntsville
  • University of California at Santa Cruz
  • Department of Astronomy and Astrophysics
  • University of California, Santa Cruz
  • Dr. Remeis-Sternwarte Bamberg
  • Center for Research and Exploration in Space Science and Technology (CRESST)
  • Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
  • Universities Space Research Association
  • Waseda University
  • Centre national de la recherche scientifique
  • University of Rome
  • Sezione di Roma
  • Department of Physics and Astronomy
  • University of Denver
  • ISAS/JAXA
  • University of Chicago
  • University of São Paulo
  • National Aeronautics and Space Administration (NASA)
  • NASA Ames Research Center
  • Department of Chemistry and Physics
  • Purdue University Northwest
  • University of New Mexico
  • Pompeu Fabra University (UPF)
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • Osservatorio Astronomico di Torino
  • Dipartimento di Fisica
  • University of Rome “Tor Vergata”
  • School of Pure and Applied Natural Sciences
  • University of Kalmar

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

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