Weakly interacting neutrinos are ideal astronomical messengers because they travel
through space without deflection by magnetic fields and, essentially, without absorption …

The announcement by the IceCube Collaboration of the observation of 28 cosmic neutrino
candidates has been greeted with a great deal of justified excitement. The data reported so …

The IceCube Neutrino Observatory has established the existence of a high-energy all-sky
neutrino flux of astrophysical origin. This discovery was made using events interacting within …

We report on the first measurement of the astrophysical neutrino flux using particle showers
(cascades) in IceCube data from 2010–2015. Assuming standard oscillations, the …

Abstract The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose
underground liquid scintillator detector, was proposed with the determination of the neutrino …

We report on a measurement of astrophysical tau neutrinos with 9.7 yr of IceCube data.
Using convolutional neural networks trained on images derived from simulated events …

Introduction Neutrino observations are a unique probe of the universe's highest-energy
phenomena: Neutrinos are able to escape from dense astrophysical environments that …

We present a measurement of atmospheric tau neutrino appearance from oscillations with
three years of data from the DeepCore subarray of the IceCube Neutrino Observatory. This …

We consider limits on the local (z= 0) density (n 0) of extragalactic neutrino sources set by
the nondetection of steady high-energy neutrino sources producing≳ 50 TeV muon …

The IceCube Neutrino Observatory was designed primarily to search for high-energy (TeV-
PeV) neutrinos produced in distant astrophysical objects. A search for≳ 100 TeV neutrinos …