Resolving the Extragalactic $\gamma$-ray Background above 50 GeV with Fermi-LAT

Abstract

The Fermi Large Area Telescope (LAT) Collaboration has recently released a catalog of 360 sources detected above 50 GeV (2FHL). This catalog was obtained using 80 months of data re-processed with Pass 8, the newest event-level analysis, which significantly improves the acceptance and angular resolution of the instrument. Most of the 2FHL sources at high Galactic latitude are blazars. Using detailed Monte Carlo simulations, we measure, for the first time, the source count distribution, $dN/dS$, of extragalactic $\gamma$-ray sources at $E>50$ GeV and find that it is compatible with a Euclidean distribution down to the lowest measured source flux in the 2FHL ($\sim 8\times 10^{-12}$ ph cm${}^{-2}$ s${}^{-1}$). We employ a one-point photon fluctuation analysis to constrain the behavior of $dN/dS$ below the source detection threshold. Overall the source count distribution is constrained over three decades in flux and found compatible with a broken power law with a break flux, $S_b$, in the range $[8\times 10^{-12},1.5\times 10^{-11}]$ ph cm${}^{-2}$ s${}^{-1}$ and power-law indices below and above the break of ${\alpha }_2\in [1.60,1.75]$ and ${\alpha }_1=2.49\pm 0.12$ respectively. Integration of $dN/dS$ shows that point sources account for at least $86_{-14}^{+16}\%$ of the total extragalactic $\gamma$-ray background. The simple form of the derived source count distribution is consistent with a single population (i.e. blazars) dominating the source counts to the minimum flux explored by this analysis. We estimate the density of sources detectable in blind surveys that will be performed in the coming years by the Cherenkov Telescope Array.

Submitted to PRL; 7 pages and 5 figures; corresponding authors: Mattia Di Mauro and Marco Ajello

References in corpus (9)

• 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
• The Spectrum and Morphology of the Fermi Bubbles
• The Origin of the Extragalactic Gamma-Ray Background and Implications for Dark-Matter Annihilation
• Composition of the Fermi-LAT isotropic gamma-ray background intensity: Emission from extragalactic point sources and dark matter annihilations
• Joint anisotropy and source count constraints on the contribution of blazars to the diffuse gamma-ray background
• Statistics of Cosmological Black Hole Jet Sources: Blazar Predictions for GLAST
• A simplified view of blazars: contribution to the X-ray and gamma-ray cosmic backgrounds
• Fermi-LAT gamma-ray anisotropy and intensity explained by unresolved Radio-Loud Active Galactic Nuclei

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