The Imprint of the EBL in the Spectra of Blazars Marco Ajello1,2, Anita Reimer3, Rolf Buehler1 on behalf of the Fermi-LAT collaboration 1KIPAC, 2UCB, 3Univ. Innsbruck Ackermann+12, in ScienceExpress Today! 1
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A correlation between 10-500 GeV flux and underdense fraction along the line of sight for VHE-like and Fermi hard sources is found at 2.4σ and 2.6σ, calculated from the Pearson correlation coefficients of r = 0.57 and 0.47, respectively.
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Get PriceThe angular distribution for responds to a significance of about 5.6σ. The recent results on the Franceschini et al. (2008) EBL model was generated by ap- 1ES 0229+200 presented by Vovk et al. (2012) are in agreement plying a scaling relation.
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