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THE THIRD CATALOG OF ACTIVE GALACTIC NUCLEI DETECTED BY THE FERMI LARGE AREA TELESCOPE

  • M. Ackermann
  • , M. Ajello
  • , W. B. Atwood
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , D. Bastieri
  • , J. Becerra Gonzalez
  • , R. Bellazzini
  • , E. Bissaldi
  • , R. D. Blandford
  • , E. D. Bloom
  • , R. Bonino
  • , E. Bottacini
  • , T. J. Brandt
  • , J. Bregeon
  • , R. J. Britto
  • , P. Bruel
  • , R. Buehler
  • , S. Buson
  • G. A. Caliandro, R. A. Cameron, M. Caragiulo, P. A. Caraveo, B. Carpenter, J. M. Casandjian, E. Cavazzuti, C. Cecchi, E. Charles, A. Chekhtman, C. C. Cheung, J. Chiang, G. Chiaro, S. Ciprini, R. Claus, J. Cohen-Tanugi, L. R. Cominsky, J. Conrad, S. Cutini, R. D'Abrusco, F. D'Ammando, A. De Angelis, R. Desiante, S. W. Digel, L. Di Venere, P. S. Drell, C. Favuzzi, S. J. Fegan, E. C. Ferrara, J. Finke, W. B. Focke, A. Franckowiak, L. Fuhrmann, Y. Fukazawa, A. K. Furniss, P. Fusco, F. Gargano, D. Gasparrini, N. Giglietto, P. Giommi, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, I. A. Grenier, J. E. Grove, S. Guiriec, J. W. Hewitt, A. B. Hill, D. Horan, R. Itoh, G. Jóhannesson, A. S. Johnson, W. N. Johnson, J. Kataoka, T. Kawano, F. Krauss, M. Kuss, G. La Mura, S. Larsson, L. Latronico, C. Leto, J. Li, L. Li, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, G. M. Madejski, M. Mayer, M. N. Mazziotta, J. E. McEnery, P. F. Michelson, T. Mizuno, A. A. Moiseev, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, E. Nuss, M. Ohno, T. Ohsugi, R. Ojha, N. Omodei, M. Orienti, E. Orlando, A. Paggi, D. Paneque, J. S. Perkins, M. Pesce-Rollins, F. Piron, G. Pivato, T. A. Porter, S. Rainò, R. Rando, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, R. W. Romani, D. Salvetti, M. Schaal, F. K. Schinzel, A. Schulz, C. Sgrò, E. J. Siskind, K. V. Sokolovsky, F. Spada, G. Spandre, P. Spinelli, L. Stawarz, D. J. Suson, H. Takahashi, T. Takahashi, Y. Tanaka, J. G. Thayer, J. B. Thayer, L. Tibaldo, D. F. Torres, E. Torresi, G. Tosti, E. Troja, Y. Uchiyama, G. Vianello, B. L. Winer, K. S. Wood, S. Zimmer
  • c/o DESY
  • Clemson University
  • University of California at Santa Cruz
  • University of Pisa
  • Universite Paris-Saclay
  • INFN Sezione di Trieste
  • University of Trieste
  • INFN
  • University of Padova
  • NASA Goddard Space Flight Center
  • University of Maryland
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • INFN Sezione di Bari
  • Kavli Institute for Particle Astrophysics and Cosmology
  • INFN Sezione di Torino
  • University of Turin
  • Laboratoire Univers et Particules de Montpellier
  • University of Johannesburg
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Catholic University of America
  • Science and Research Directorate
  • INFN Sezione di Perugia
  • University of Perugia
  • George Mason University
  • Naval Research Laboratory
  • Osservatorio Astronomico di Roma
  • Sonoma State University
  • Stockholm University
  • Oskar Klein Centre
  • Royal Swedish Academy of Sciences
  • Center for Astrophysics | Harvard & Smithsonian
  • INAF Istituto di Radioastronomia
  • University of Bologna
  • and Physics University of Udine
  • Politecnico di Bari
  • Max-Planck-Institut für Radioastronomie
  • Hiroshima University
  • Biochemical and Environmental Engineering
  • University of Southampton
  • University of Iceland
  • Waseda University
  • Dr. Remeis-Sternwarte Bamberg
  • Medical University of Innsbruck
  • ASI Science Data Center
  • University of Sheffield
  • KTH Royal Institute of Technology
  • Univ. Bordeaux
  • Sezione di Roma
  • Long Beach VA and University of California
  • Max-Planck-Institut für Physik
  • National Research Council
  • University of New Mexico
  • NYCB Real-Time Computing Inc.
  • P.N. Lebedev Physical Institute of the Russian Academy of Sciences
  • ISAS/JAXA
  • Jagiellonian University
  • Purdue University Northwest
  • Pompeu Fabra University (UPF)
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Bologna
  • The Ohio State University

Research output: Contribution to journalArticlepeer-review

Abstract

The third catalog of active galactic nuclei (AGNs) detected by the Fermi-LAT (3LAC) is presented. It is based on the third Fermi-LAT catalog (3FGL) of sources detected between 100 MeV and 300 GeV with a Test Statistic greater than 25, between 2008 August 4 and 2012 July 31. The 3LAC includes 1591 AGNs located at high Galactic latitudes (), a 71% increase over the second catalog based on 2 years of data. There are 28 duplicate associations, thus 1563 of the 2192 high-latitude gamma-ray sources of the 3FGL catalog are AGNs. Most of them (98%) are blazars. About half of the newly detected blazars are of unknown type, i.e., they lack spectroscopic information of sufficient quality to determine the strength of their emission lines. Based on their gamma-ray spectral properties, these sources are evenly split between flat-spectrum radio quasars (FSRQs) and BL Lacs. The most abundant detected BL Lacs are of the high-synchrotron-peaked (HSP) type. About 50% of the BL Lacs have no measured redshifts. A few new rare outliers (HSP-FSRQs and high-luminosity HSP BL Lacs) are reported. The general properties of the 3LAC sample confirm previous findings from earlier catalogs. The fraction of 3LAC blazars in the total population of blazars listed in BZCAT remains non-negligible even at the faint ends of the BZCAT-blazar radio, optical, and X-ray flux distributions, which hints that even the faintest known blazars could eventually shine in gamma-rays at LAT-detection levels. The energy-flux distributions of the different blazar populations are in good agreement with extrapolation from earlier catalogs.

Original languageEnglish
Article number14
JournalAstrophysical Journal
Volume810
Issue number1
DOIs
Publication statusPublished - 1 Sept 2015

Keywords

  • BL Lacertae objects: general
  • galaxies: active
  • galaxies: jets
  • gamma rays: galaxies

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