activity
20152021
most citedFlavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

197 citations · 807 across the 15 of their papers we have counts for

collaborators
Showing 2018Show all

11 papers · 1 filter

astro-ph.HE2018

High-Energy Cosmic Rays from Radio Galaxies

Björn Eichmann

A detailed investigation of radio galaxies has recently stressed these sources as the possible origin of the cosmic rays observed above . Here, the relevance of this…

astro-ph.HE20181 cited

Summing up Ultra-High-Energy Cosmic Rays from Radio Galaxies

Björn Eichmann

Radio galaxies are intensively discussed as the sources of cosmic rays observed above about 3 EeV, called ultra-high-energy cosmic rays (UHECRs). Here, the key issues from a recent…

astro-ph.HE2018

Search for Multi-messenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during its first Observing Run, ANTARES and IceCube

ANTARES, IceCube, LIGO +1589

Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-th…

hep-ph2018

Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data

IceCube Collaboration, M. G. Aartsen, M. Ackermann +325

The IceCube Collaboration has observed a high-energy astrophysical neutrino flux and recently found evidence for neutrino emission from the blazar TXS 0506+056. These results open…

astro-ph.HE2018

Detection of the Temporal Variation of the Sun's Cosmic Ray Shadow with the IceCube Detector

IceCube Collaboration, M. G. Aartsen, M. Ackermann +326

We report on the observation of a deficit in the cosmic ray flux from the directions of the Moon and Sun with five years of data taken by the IceCube Neutrino Observatory. Between…

hep-ex2018

Measurements using the inelasticity distribution of multi-TeV neutrino interactions in IceCube

IceCube Collaboration, M. G. Aartsen, M. Ackermann +330

Inelasticity--the fraction of a neutrino's energy transferred to hadrons--is a quantity of interest in the study of astrophysical and atmospheric neutrino interactions at multi-TeV…