The Astrophysical Journal · 2020 · 359 citations · 125 references
Natural SciencesAstronomyPhysicsAstrophysicsGamma-ray AstronomyRadio AstronomyExtragalactic Gamma-ray AstronomyExtragalactic Radio AstronomyGalactic Gamma-ray AstronomyGamma-ray TelescopesGround-based Gamma-ray ObservatoriesSpace-based Gamma-ray ObservatoriesActive Galactic Nuclei ContributionActive Galactic Nuclei VariabilityActive Galactic Nucleus ContributionExtragalactic Source CatalogsGamma-ray Source CatalogsGamma-ray VariabilityHigh-latitude Gamma-ray EmissionSpace-based Gamma-ray Telescopes
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 objects located at high Galactic latitudes ( ). 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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