Evidence for GeV Pair Halos around Low Redshift Blazars

preprint2015arXivOpen access

Abstract

We report on the results of a search for γγ-ray pair halos with a stacking analysis of low-redshift blazars using data from the Fermi Large Area Telescope. For this analysis we used a number of a-priori selection criteria, including the spatial and spectral properties of the Fermi sources. The angular distribution of ∼\sim 1GeV photons around 24 stacked isolated high-synchrotron-peaked BL Lacs with redshift z<0.5z<0.5 shows an excess over that of point-like sources. A statistical analysis yields a Bayes factor of log10B10>2\mathrm{log}_{10}B_{10}>2, providing evidence in favor of extended emission against the point-source hypothesis, consistent with expectations for pair halos produced in the IGMF with strength BIGMF∼10−17−10−15GB_{\mathrm{IGMF}}\sim 10^{-17}-10^{-15}\mathrm{G}.

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