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Title: Statistical measurement of the gamma-ray source-count distribution as a function of energy

Statistical properties of photon count maps have recently been proven as a new tool to study the composition of the gamma-ray sky with high precision. Here, we employ the 1-point probability distribution function of six years of Fermi-LAT data to measure the source-count distribution dN/dS and the diffuse components of the high-latitude gamma-ray sky as a function of energy. To that aim, we analyze the gamma-ray emission in five adjacent energy bands between 1 and 171 GeV. It is demonstrated that the source-count distribution as a function of flux is compatible with a broken power law up to energies of ~50 GeV. Furthermore, the index below the break is between 1.95 and 2.0. For higher energies, a simple power-law fits the data, with an index of $${2.2}_{-0.3}^{+0.7}$$ in the energy band between 50 and 171 GeV. Upper limits on further possible breaks as well as the angular power of unresolved sources are derived. We find that point-source populations probed by this method can explain $${83}_{-13}^{+7}$$% ($${81}_{-19}^{+52}$$%) of the extragalactic gamma-ray background between 1.04 and 1.99 GeV (50 and 171 GeV). Our method has excellent capabilities for constraining the gamma-ray luminosity function and the spectra of unresolved blazars.
Authors:
ORCiD logo [1] ;  [2] ; ORCiD logo [1] ; ORCiD logo [1] ; ORCiD logo [1]
  1. Univ. of Torino (Italy). Dept. of Physics; National Inst. of Nuclear Physics, Torino (Italy)
  2. National Inst. of Nuclear Physics, Torino (Italy); RWTH Aachen Univ. (Germany). Inst. for Theoretical Particle Physics and Cosmology (TTK)
Publication Date:
Grant/Contract Number:
AC02-76SF00515
Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal. Letters
Additional Journal Information:
Journal Volume: 826; Journal Issue: 2; Journal ID: ISSN 2041-8213
Publisher:
Institute of Physics (IOP)
Research Org:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Org:
USDOE
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; gamma rays: diffuse background; gamma rays: general; methods: statistical
OSTI Identifier:
1355707

Zechlin, Hannes-S., Cuoco, Alessandro, Donato, Fiorenza, Fornengo, Nicolao, and Regis, Marco. Statistical measurement of the gamma-ray source-count distribution as a function of energy. United States: N. p., Web. doi:10.3847/2041-8205/826/2/L31.
Zechlin, Hannes-S., Cuoco, Alessandro, Donato, Fiorenza, Fornengo, Nicolao, & Regis, Marco. Statistical measurement of the gamma-ray source-count distribution as a function of energy. United States. doi:10.3847/2041-8205/826/2/L31.
Zechlin, Hannes-S., Cuoco, Alessandro, Donato, Fiorenza, Fornengo, Nicolao, and Regis, Marco. 2016. "Statistical measurement of the gamma-ray source-count distribution as a function of energy". United States. doi:10.3847/2041-8205/826/2/L31. https://www.osti.gov/servlets/purl/1355707.
@article{osti_1355707,
title = {Statistical measurement of the gamma-ray source-count distribution as a function of energy},
author = {Zechlin, Hannes-S. and Cuoco, Alessandro and Donato, Fiorenza and Fornengo, Nicolao and Regis, Marco},
abstractNote = {Statistical properties of photon count maps have recently been proven as a new tool to study the composition of the gamma-ray sky with high precision. Here, we employ the 1-point probability distribution function of six years of Fermi-LAT data to measure the source-count distribution dN/dS and the diffuse components of the high-latitude gamma-ray sky as a function of energy. To that aim, we analyze the gamma-ray emission in five adjacent energy bands between 1 and 171 GeV. It is demonstrated that the source-count distribution as a function of flux is compatible with a broken power law up to energies of ~50 GeV. Furthermore, the index below the break is between 1.95 and 2.0. For higher energies, a simple power-law fits the data, with an index of ${2.2}_{-0.3}^{+0.7}$ in the energy band between 50 and 171 GeV. Upper limits on further possible breaks as well as the angular power of unresolved sources are derived. We find that point-source populations probed by this method can explain ${83}_{-13}^{+7}$% (${81}_{-19}^{+52}$%) of the extragalactic gamma-ray background between 1.04 and 1.99 GeV (50 and 171 GeV). Our method has excellent capabilities for constraining the gamma-ray luminosity function and the spectra of unresolved blazars.},
doi = {10.3847/2041-8205/826/2/L31},
journal = {The Astrophysical Journal. Letters},
number = 2,
volume = 826,
place = {United States},
year = {2016},
month = {7}
}