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The IceCube Realtime Alert System
IceCube Collaboration, M. G. Aartsen, M. Ackermann +301
Following the detection of high-energy astrophysical neutrinos in 2013, their origin is still unknown. Aiming for the identification of an electromagnetic counterpart of a rapidly…
Search for annihilating dark matter in the Sun with 3 years of IceCube data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +301
We present results from an analysis looking for dark matter annihilation in the Sun with the IceCube neutrino telescope. Gravitationally trapped dark matter in the Sun's core can a…
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…
Very High-Energy Gamma-Ray Follow-Up Program Using Neutrino Triggers from IceCube
IceCube Collaboration, M. G. Aartsen, K. Abraham +537
We describe and report the status of a neutrino-triggered program in IceCube that generates real-time alerts for gamma-ray follow-up observations by atmospheric-Cherenkov telescope…
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…
All-sky search for time-integrated neutrino emission from astrophysical sources with 7 years of IceCube data
IceCube Collaboration, M. G. Aartsen, K. Abraham +306
Since the recent detection of an astrophysical flux of high energy neutrinos, the question of its origin has not yet fully been answered. Much of what is known about this flux come…
First search for dark matter annihilations in the Earth with the IceCube Detector
IceCube Collaboration, M. G. Aartsen, K. Abraham +312
We present the results of the first IceCube search for dark matter annihilation in the center of the Earth. Weakly Interacting Massive Particles (WIMPs), candidates for dark matter…
Observation and Characterization of a Cosmic Muon Neutrino Flux from the Northern Hemisphere using six years of IceCube data
IceCube Collaboration, M. G. Aartsen, K. Abraham +309
The IceCube Collaboration has previously discovered a high-energy astrophysical neutrino flux using neutrino events with interaction vertices contained within the instrumented volu…
Constraints on ultra-high-energy cosmic ray sources from a search for neutrinos above 10 PeV with IceCube
IceCube Collaboration, M. G. Aartsen, K. Abraham +309
We report constraints on the sources of ultra-high-energy cosmic ray (UHECR) above GeV, based on an analysis of seven years of IceCube data. This analysis efficiently sele…
Search for Sources of High Energy Neutrons with Four Years of Data from the IceTop Detector
IceCube Collaboration, M. G. Aartsen, K. Abraham +308
IceTop is an air shower array located on the Antarctic ice sheet at the geographic South Pole. IceTop can detect an astrophysical flux of neutrons from Galactic sources as an exces…
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…