We report on the results of a search for γ-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 ∼ 1GeV photons around 24 stacked isolated high-synchrotron-peaked BL Lacs with redshift z < 0.5 shows an excess over that of point-like sources. A statistical analysis yields a Bayes factor of log 10 B10 > 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 −15 G. PACS numbers: 95.85.Pw, 98.58.Ay, 98.54.Cm,
INTRODUCTIONThe magnetic fields that are observed in galaxies and galaxy clusters are believed to result from the dynamo amplification of weak magnetic field seeds, whose origin remains a mystery. Intergalactic magnetic fields (IGMFs), deep in the voids between galaxies, provide the most accurate image of the weak primordial seed fields and could be linked to the early stages in the evolution of the universe (see e.g.[1] for a recent review). Among the several methods used to study cosmological magnetic fields (see e.g. [2] for a recent review), the observation (or nondetection) of cascade emission from blazars can potentially measure very weak IGMFs. A number of blazars have been observed to emit both very-high-energy (VHE, > 100 GeV) γ-rays with ground-based γ-ray instruments and high-energy (HE, MeV/GeV) γ-rays with the Fermi Gamma-ray Space Telescope [3,4]. Most of the detected TeV γ-rays are from the nearest sources since such high energy γ-rays cannot propagate over long distances in intergalactic space due to interactions with the extragalactic background light (EBL). Of course, some higherredshift sources still have detectable TeV emission (e.g. blazar PKS1424+240, which has redshift lower limit of z > 0.6 [5]), but with highly absorbed spectra consistent with theoretical calculations of the attenuation by the EBL. [6][7][8][9][10]. These interactions of TeV γ-rays with the EBL produce electron-positron pairs that subsequently are cooled by inverse Compton (IC) interactions with the Cosmic Microwave Background (CMB), ultimately leading to GeV γ-ray emission from these pair cascades. Since magnetic fields deflect the electron-positron pairs changing the angular distribution of cascade emission, searches for extended GeV emission around blazars can provide an avenue for constraining the IGMF.Due to the low GeV γ-ray flux from extragalactic sources, it is difficult to examine the angular extent of the photon events from a single blazar or even to assess the joint likelihood for detailed fits to a set of individual sources where individual source parameters are taken to be completely independent. To overcome this limitation, stacking sources has been used to make such statistical analysis feasible. Despite early hints at a signal in the stacking analysis of 1...