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The Fourth Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope

  • M. Ajello
  • , R. Angioni
  • , M. Axelsson
  • , J. Ballet
  • , G. Barbiellini
  • , D. Bastieri
  • , J. Becerra Gonzalez
  • , R. Bellazzini
  • , E. Bissaldi
  • , E. D. Bloom
  • , R. Bonino
  • , E. Bottacini
  • , P. Bruel
  • , S. Buson
  • , F. Cafardo
  • , R. A. Cameron
  • , E. Cavazzuti
  • , S. Chen
  • , C. C. Cheung
  • , S. Ciprini
  • D. Costantin, S. Cutini, F. D'Ammando, P. De La Torre Luque, R. De Menezes, F. De Palma, A. Desai, N. Di Lalla, L. Di Venere, A. Domínguez, F. Fana Dirirsa, E. C. Ferrara, J. Finke, A. Franckowiak, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, S. Garrappa, D. Gasparrini, N. Giglietto, F. Giordano, M. Giroletti, D. Green, I. A. Grenier, S. Guiriec, S. Harita, E. Hays, D. Horan, R. Itoh, G. Jóhannesson, M. Kovac'Evic', F. Krauss, M. Kreter, M. Kuss, S. Larsson, C. Leto, J. Li, I. Liodakis, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, G. M. Madejski, S. Maldera, A. Manfreda, G. Martí-Devesa, F. Massaro, M. N. Mazziotta, I. Mereu, M. Meyer, G. Migliori, N. Mirabal, T. Mizuno, M. E. Monzani, A. Morselli, I. V. Moskalenko, M. Negro, R. Nemmen, E. Nuss, L. S. Ojha, R. Ojha, N. Omodei, M. Orienti, E. Orlando, J. F. Ormes, V. S. Paliya, Z. Pei, H. Peña-Herazo, M. Persic, M. Pesce-Rollins, L. Petrov, F. Piron, H. Poon, G. Principe, S. Rainò, R. Rando, B. Rani, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, F. K. Schinzel, D. Serini, C. Sgrò, E. J. Siskind, G. Spandre, P. Spinelli, D. J. Suson, Y. Tachibana, D. J. Thompson, D. F. Torres, E. Torresi, E. Troja, J. Valverde, P. Van Zyl, M. Yassine
  • Clemson University
  • Italian Space Agency
  • National Institute for Nuclear Physics
  • Stockholm University
  • KTH Royal Institute of Technology
  • Université Paris Diderot
  • University of Trieste
  • University of Padua
  • Instituto de Astrofísica de Canarias
  • Polytechnic University of Bari
  • SLAC National Accelerator Laboratory
  • University of Turin
  • Laboratoire Leprince-Ringuet
  • University of Würzburg
  • Universidade de São Paulo
  • Naval Research Laboratory
  • National Institute for Astrophysics
  • Complutense University
  • University of Johannesburg
  • NASA Goddard Space Flight Center
  • German Electron Synchrotron
  • Hiroshima University
  • Friedrich-Alexander University Erlangen-Nürnberg
  • Max Planck Institute for Physics (Werner Heisenberg Institute)
  • George Washington University
  • Tokyo Institute of Technology
  • Bisei Astronomical Observatory
  • University of Iceland
  • Pennsylvania State University
  • North West University
  • Oskar Klein Centre
  • Dalarna University
  • Université de Bordeaux
  • University of Pisa
  • University of Innsbruck
  • Istituto Nazionale di Astrofisica-Osservatorio Astrofisico di Torino
  • University of Perugia
  • University of Bologna
  • University of Maryland Baltimore County
  • Université Montpellier 2
  • University of Denver
  • Instituto Nacional de Astrofisica Optica y Electronica
  • Osservatorio Astronomico di Trieste
  • Korea Astronomy and Space Science Institute
  • National Science Foundation
  • University of New Mexico
  • NYCB Real-Time Computing Inc.
  • Purdue University Northwest
  • Autonomous University of Barcelona
  • ICREA
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • University of Maryland
  • National Research Foundation
  • University of the Witwatersrand
  • Square Kilometre Array

Research output: Contribution to journalArticlepeer-review

320 Citations (Scopus)

Abstract

The fourth catalog of active galactic nuclei (AGNs) detected by the Fermi Gamma-ray Space Telescope Large Area Telescope (4LAC) between 2008 August 4 and 2016 August 2 contains 2863 objects located at high Galactic latitudes (|b| > 10°). It includes 85% more sources than the previous 3LAC catalog based on 4 yr of data. AGNs represent at least 79% of the high-latitude sources in the fourth Fermi-Large Area Telescope Source Catalog (4FGL), which covers the energy range from 50 MeV to 1 TeV. In addition, 344 gamma-ray AGNs are found at low Galactic latitudes. Most of the 4LAC AGNs are blazars (98%), while the remainder are other types of AGNs. The blazar population consists of 24% Flat Spectrum Radio Quasars (FSRQs), 38% BL Lac-type objects, and 38% blazar candidates of unknown types (BCUs). On average, FSRQs display softer spectra and stronger variability in the gamma-ray band than BLQLacs do, confirming previous findings. All AGNs detected by ground-based atmospheric Cerenkov telescopes are also found in the 4LAC.

Original languageEnglish
Article number105
JournalAstrophysical Journal
Volume892
Issue number2
DOIs
Publication statusPublished - 1 Apr 2020

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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