activity
20122017
most citedFlavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

197 citations · 929 across the 12 of their papers we have counts for

collaborators

12 papers

hep-ex2017190 cited

Measurement of the multi-TeV neutrino cross section with IceCube using Earth absorption

IceCube Collaboration, M. G. Aartsen, M. Ackermann +314

Neutrinos interact only very weakly, so they are extremely penetrating. However, the theoretical neutrino-nucleon interaction cross section rises with energy such that, at energies…

astro-ph.HE2017

The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part III: Cosmic Rays

IceCube Collaboration, M. G. Aartsen, M. Ackermann +312

Papers on cosmic-ray measurements submitted to the 35th International Cosmic Ray Conference (ICRC 2017, Busan, South Korea) by the IceCube Collaboration

astro-ph.HE2017147 cited

Constraints on Galactic Neutrino Emission with Seven Years of IceCube Data

IceCube Collaboration, M. G. Aartsen, M. Ackermann +309

The origins of high-energy astrophysical neutrinos remain a mystery despite extensive searches for their sources. We present constraints from seven years of IceCube Neutrino Observ…

astro-ph.HE201631 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.HE2015197 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-ex201283 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…