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20032016
most citedFlavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

197 citations · 1.8k across the 21 of their papers we have counts for

collaborators

21 papers

astro-ph.HE2016★ 31 cited

Lowering IceCube's Energy Threshold for Point Source Searches in the Southern Sky

IceCube Collaboration, M. G. Aartsen, K. Abraham +317

Observation of a point source of astrophysical neutrinos would be a "smoking gun" signature of a cosmic-ray accelerator. While IceCube has recently discovered a diffuse flux of ast…

astro-ph.HE2015★ 197 cited

Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

IceCube Collaboration, M. G. Aartsen, M. Ackermann +300

A diffuse flux of astrophysical neutrinos above has been observed at the IceCube Neutrino Observatory. Here we extend this analysis to probe the astrophysical f…

hep-ex2012★ 193 cited

Multiplicities of charged pions and kaons from semi-inclusive deep-inelastic scattering by the proton and the deuteron

HERMES Collaboration, A. Airapetian, N. Akopov +135

Multiplicities in semi-inclusive deep-inelastic scattering are presented for each charge state of π^\pm and K^\pm mesons. The data were collected by the HERMES experiment at the HE…

hep-ex2012★ 83 cited

Measurement of the Atmospheric flux in IceCube

IceCube Collaboration, M. G. Aartsen, R. Abbasi +274

We report the first measurement of the atmospheric electron neutrino flux in the energy range between approximately 80 GeV and 6 TeV, using data recorded during the first year of o…

hep-ex2012★ 41 cited

Search for exotic resonances decaying into WZ/ZZ in pp collisions at sqrt(s) = 7 TeV

CMS Collaboration

A search for new exotic particles decaying to the VZ final state is performed, where V is either a W or a Z boson decaying into two overlapping jets and the Z decays into a pair of…

astro-ph.HE2012★ 39 cited

Search for Galactic PeV Gamma Rays with the IceCube Neutrino Observatory

IceCube collaboration, M. G. Aartsen, R. Abbasi +274

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…