4.7 Article

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

Journal

ASTROPHYSICAL JOURNAL
Volume 892, Issue 2, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.3847/1538-4357/ab791e

Keywords

Active galactic nuclei; Blazars; Gamma-ray sources; Relativistic jets; Quasars; BL Lacertae objects

Funding

  1. DOE [DE- AC02-76SF00515]
  2. National Aeronautics and Space Administration
  3. National Science Foundation
  4. Alfred P. Sloan Foundation
  5. U.S. Department of Energy
  6. Japanese Monbukagakusho
  7. Max Planck Society
  8. Higher Education Funding Council for England
  9. American Museum of Natural History
  10. Astrophysical Institute Potsdam
  11. University of Basel
  12. University of Cambridge
  13. Case Western Reserve University
  14. University of Chicago
  15. Drexel University
  16. Fermilab
  17. Institute for Advanced Study
  18. Japan Participation Group
  19. Johns Hopkins University
  20. Joint Institute for Nuclear Astrophysics
  21. Kavli Institute for Particle Astrophysics and Cosmology
  22. Korean Scientist Group
  23. Chinese Academy of Sciences (LAMOST)
  24. Los Alamos National Laboratory
  25. Max-Planck-Institute for Astronomy (MPIA)
  26. Max-PlanckInstitute for Astrophysics (MPA)
  27. New Mexico State University
  28. Ohio State University
  29. University of Pittsburgh
  30. University of Portsmouth
  31. Princeton University
  32. United States Naval Observatory
  33. University of Washington

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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 . 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, 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 BL Lacs do, confirming previous findings. All AGNs detected by ground-based atmospheric Cerenkov telescopes are also found in the 4LAC.

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