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The IceCube Neutrino Observatory: Instrumentation and Online Systems
IceCube Collaboration, M. G. Aartsen, M. Ackermann +350
The IceCube Neutrino Observatory is a cubic-kilometer-scale high-energy neutrino detector built into the ice at the South Pole. Construction of IceCube, the largest neutrino detect…
The contribution of Fermi-2LAC blazars to the diffuse TeV-PeV neutrino flux
IceCube Collaboration, M. G. Aartsen, K. Abraham +319
The recent discovery of a diffuse cosmic neutrino flux extending up to PeV energies raises the question of which astrophysical sources generate this signal. One class of extragalac…
PINGU: A Vision for Neutrino and Particle Physics at the South Pole
Gen2 Collaboration
The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on t…
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…
All-flavour Search for Neutrinos from Dark Matter Annihilations in the Milky Way with IceCube/DeepCore
IceCube collaboration, M. G. Aartsen, K. Abraham +319
We present the first IceCube search for a signal of dark matter annihilations in the Milky Way using all-flavour neutrino-induced particle cascades. The analysis focuses on the Dee…
Anisotropy in Cosmic-Ray Arrival Directions in the Southern Hemisphere with Six Years of Data from the IceCube Detector
IceCube Collaboration, M. G. Aartsen, K. Abraham +314
The IceCube Neutrino Observatory has accumulated a total of 318 billion cosmic-ray induced muon events between May 2009 and May 2015. This data set was used for a detailed analysis…