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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 2.

Average distribution function ﹩\rho (f)﹩ of the fractional photon flux f from a point source in a given pixel. The solid and dashed red lines depict the distribution function for the effective detector PSF for two different pixel sizes: a HEALPix grid with resolution parameter ﹩\kappa =6﹩ (solid) and ﹩\kappa =7﹩ (dashed); see Section 3 for details. The dot-dotted blue line depicts the ﹩\kappa =6﹩ distribution function for a Gaussian PSF with a 68% containment radius resembling the one of the actual effective PSF. The average distributions have been derived from Monte Carlo simulations of ﹩5\times {10}^{4}﹩ fiducial point sources at random positions on the sky. The numerical resolution is ﹩{\rm{\Delta }}f=0.01.﹩

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