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2012

Search for Galactic PeV Gamma Rays with the IceCube Neutrino Observatory

IceCube collaboration, Aartsen, M. G., Abbasi, R. et al.

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Gamma-ray induced air showers are notable for their lack of muons, compared to hadronic showers.

Hence, air shower arrays with large underground muon detectors can select a sample greatly enriched in photon showers by rejecting showers containing muons.
IceCube is sensitive to muons with energies above ~500 GeV at the surface, which provides an efficient veto system for hadronic air showers with energies above 1 PeV.
One year of data from the 40-string IceCube configuration was used to perform a search for point sources and a Galactic diffuse signal.

Search for Galactic PeV Gamma Rays with the IceCube Neutrino Observatory · Around

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