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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 10.

Upper limits on a possible second intrinsic break ﹩{S}_{{\rm{b}}2}﹩ as a function of ﹩{\rm{\Delta }}{n}_{23}﹩ at 95% confidence level (see text for details). The solid green (dashed blue) line denotes the upper limits derived from the posterior (profile likelihood).

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