Title: Unveiling the Gamma-Ray Source Count Distribution Below the Fermi Detection Limit with Photon Statistics

Abstract

The source-count distribution as a function of their flux, dN/dS, is one of the main quantities characterizing gamma-ray source populations. In this paper, we employ statistical properties of the Fermi Large Area Telescope (LAT) photon counts map to measure the composition of the extragalactic gamma-ray sky at high latitudes (|b| greater-than or slanted equal to 30°) between 1 and 10 GeV. We present a new method, generalizing the use of standard pixel-count statistics, to decompose the total observed gamma-ray emission into (a) point-source contributions, (b) the Galactic foreground contribution, and (c) a truly diffuse isotropic background contribution. Using the 6 yr Fermi-LAT data set (P7REP), we show that the dN/dS distribution in the regime of so far undetected point sources can be consistently described with a power law with an index between 1.9 and 2.0. We measure dN/dS down to an integral flux of ~2 x 10^-11cm^-2s^-1, improving beyond the 3FGL catalog detection limit by about one order of magnitude. The overall dN/dS distribution is consistent with a broken power law, with a break at 2.1^+1.0_-1.3 x 10^-8cm^-2s^-1. The power-law index n₁ = 3.1^+0.7_-0.5 for bright sources above the break hardens to n₂ = 1.97 ± 0.03 for fainter sourcesmore » below the break. A possible second break of the dN/dS distribution is constrained to be at fluxes below 6.4 x 10^-11cm^-2s^-1 at 95% confidence level. Finally, the high-latitude gamma-ray sky between 1 and 10 GeV is shown to be composed of ~25% point sources, ~69.3% diffuse Galactic foreground emission, and ~6% isotropic diffuse background.« less

Authors:

Zechlin, Hannes-S.  ^[1];

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• Search DOE PAGES for ORCID "0000-0001-5032-7704"

Cuoco, Alessandro ^[2]; Donato, Fiorenza  ^[1];

• Search DOE PAGES for author "Donato, Fiorenza"
• Search DOE PAGES for ORCID "0000-0002-9526-5612"

Fornengo, Nicolao  ^[1];

• Search DOE PAGES for author "Fornengo, Nicolao"
• Search DOE PAGES for ORCID "0000-0002-3074-3118"

Vittino, Andrea ^[3]

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+ Show Author Affiliations

1. Univ. of Turin (Italy). Dept. of Physics; National Inst. for Nuclear Physics (INFN), Turin (Italy)
2. National Inst. for Nuclear Physics (INFN), Turin (Italy); RWTH Aachen Univ. (Germany). Inst. for Theoretical Particle Physics and Cosmology (TTK)
3. Technical Univ. of Munich, Garching (Germany). Physics Dept.

Publication Date:

Tue Jul 26 00:00:00 EDT 2016

Research Org.:

National Inst. for Nuclear Physics (INFN), Turin (Italy); Univ. of Turin (Italy); Technical Univ. of Munich, Garching (Germany)

Sponsoring Org.:

USDOE; Ministry of Education, University and Research (MIUR) (Italy); National Inst. for Nuclear Physics (INFN) (Italy); Univ. of Turin (Italy); Compagnia di San Paolo (Italy); German-Israeli Foundation for Scientific Research and Development (GIF) (Israel)

Contributing Org.:

Fermi-LAT Collaboration; RWTH Aachen Univ. (Germany)

OSTI Identifier:

1355703

Grant/Contract Number:  

2012CPPYP7

Resource Type:

Accepted Manuscript

Journal Name:

The Astrophysical Journal. Supplement Series (Online)

Additional Journal Information:

Journal Name: The Astrophysical Journal. Supplement Series (Online); Journal Volume: 225; Journal Issue: 2; Journal ID: ISSN 1538-4365

Publisher:

American Astronomical Society/IOP

Country of Publication:

United States

Language:

English

Subject:

79 ASTRONOMY AND ASTROPHYSICS; diffuse background; gamma-rays; statistical methods