Cosmological Evolution of Flat-Spectrum Radio Quasars based on the {\it Swift}/BAT 105-month Catalog and Their Contribution to the Cosmic MeV Gamma-ray Background Radiation
arXiv:2005.02648 · doi:10.3847/1538-4357/ab9113
Abstract
We present a new X-ray luminosity function of flat-spectrum radio quasars (FSRQs) utilizing the latest {\it Swift}/BAT 105-month X-ray source catalog. Contrary to previous studies of FSRQs in the X-ray band, using the luminosity-dependent density evolution model, we find that FSRQs show evolutionary peaks at depending on luminosities. Our result is rather consistent with the evolution of FSRQs seen in the radio and GeV bands, although the number density is a factor of 5--10 smaller. We further explore the contribution of FSRQs to the cosmic MeV gamma-ray background radiation. We find that FSRQs can explain only \% of the observed MeV gamma-ray background fluxes around 1 MeV, indicating other populations are required. Future MeV gamma-ray observations will be keys for understanding the origin of the MeV gamma-ray background radiation.
Accepted for ApJ
References in corpus (11)
- The synthesis of the cosmic X-ray background in the Chandra and XMM-Newton era
- The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV
- Toward the Standard Population Synthesis Model of the X-Ray Background: Evolution of X-Ray Luminosity and Absorption Functions of Active Galactic Nuclei Including Compton-Thick Populations
- Radio-Loudness of Active Galactic Nuclei: Observational Facts and Theoretical Implications
- The power of relativistic jets is larger than the luminosity of their accretion disks
- The 5th edition of the Roma-BZCAT. A short presentation
- Cosmic X-ray background and Earth albedo Spectra with Swift/BAT
- The Origin of the Extragalactic Gamma-Ray Background and Implications for Dark-Matter Annihilation
- INTEGRAL observations of the cosmic X-ray background in the 5-100 keV range via occultation by the Earth
- General Physical Properties of CGRaBS Blazars
- The Cosmic MeV Gamma-ray Background and Hard X-ray Spectra of Active Galactic Nuclei: Implications for the Origin of Hot AGN Coronae
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- The diffuse extragalactic gamma-ray background radiation: star-forming galaxies are not the dominant component
- Source identification for the Swift-BAT 150-month hard X-ray catalog using soft X-ray observations
- The Gamma-ray Luminosity Function of Flat-Spectrum Radio Quasars