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Unresolved Unidentified Source Contribution to the Gamma‐Ray Background

  • Authors: V. Pavlidou, J. M. Siegal-Gaskins, B. D. Fields, A. V. Olinto, and C. Brown

Pavlidou et al. 2008 The Astrophysical Journal 677 27.

  • Provider: AAS Journals

Caption: Fig. 5.

Likelihood contours for the intrinsic spectral index distribution parameters of sample 1 (solid line). The maximum likelihood parameters are denoted by cross signs. The square and triangle symbols denote the locations of the maximum likelihood parameters for samples 2 and 3, respectively. As a comparison, the likelihood contours for the sample of confidently identified blazars (as in Mattox et al. 2001) are overplotted with the dashed lines.

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