514 citations · 1.6k across the 8 of their papers we have counts for
8 papers
All-flavor constraints on nonstandard neutrino interactions and generalized matter potential with three years of IceCube DeepCore data
IceCube Collaboration, R. Abbasi, M. Ackermann +370
We report constraints on nonstandard neutrino interactions (NSI) from the observation of atmospheric neutrinos with IceCube, limiting all individual coupling strengths from a singl…
Combined sensitivity to the neutrino mass ordering with JUNO, the IceCube Upgrade, and PINGU
Gen2 Collaboration, M. G. Aartsen, M. Ackermann +440
The ordering of the neutrino mass eigenstates is one of the fundamental open questions in neutrino physics. While current-generation neutrino oscillation experiments are able to pr…
Time-integrated Neutrino Source Searches with 10 years of IceCube Data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +357
This paper presents the results from point-like neutrino source searches using ten years of IceCube data collected between Apr.~6, 2008 and Jul.~10, 2018. We evaluate the significa…
The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part VI: IceCube-Gen2, the Next Generation Neutrino Observatory
Gen2 Collaboration, M. G. Aartsen, M. Ackermann +356
Papers on research & development towards IceCube-Gen2, the next generation neutrino observatory at South Pole, submitted to the 35th International Cosmic Ray Conference (ICRC 2017,…
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…