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UNVEILING THE GAMMA-RAY SOURCE COUNT DISTRIBUTION BELOW THE FERMI DETECTION LIMIT WITH PHOTON STATISTICS

  • Authors: Hannes-S. Zechlin, Alessandro Cuoco, Fiorenza Donato, Nicolao Fornengo, and Andrea Vittino

2016 The Astrophysical Journal Supplement Series 225 18.

  • Provider: AAS Journals

Caption: Figure 7.

Differential source-count distribution ﹩{dN}/{dS}﹩ (left column) and integral source-count distribution ﹩N(\gt S)﹩ (right column) as obtained from the 6 yr Fermi-LAT data using the hybrid approach. The ﹩{dN}/{dS}﹩ distribution has been parameterized with an MBPL with one, two, and three free breaks (from top to bottom), together with a node at the faint end of the distribution. The use of line styles and colors resembles Figure 5.

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