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TANAMI Blazars in the IceCube PeV Neutrino Fields

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arxiv 1406.0645 v2 pith:SIATRSBI submitted 2014-06-03 astro-ph.HE hep-exhep-ph

TANAMI Blazars in the IceCube PeV Neutrino Fields

classification astro-ph.HE hep-exhep-ph
keywords eventsneutrinoatmosphericbackgroundblazarsicecubetanamiaccelerated
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The IceCube Collaboration has announced the discovery of a neutrino flux in excess of the atmospheric background. Due to the steeply falling atmospheric background spectrum, events at PeV energies are most likely of extraterrestrial origin. We present the multiwavelength properties of the six radio brightest blazars positionally coincident with these events using contemporaneous data of the TANAMI blazar sample, including high-resolution images and spectral energy distributions. Assuming the X-ray to {\gamma}-ray emission originates in the photoproduction of pions by accelerated protons, the integrated predicted neutrino luminosity of these sources is large enough to explain the two detected PeV events.

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