Showing 1–20 of 134 results
/ Date/ Name
Dec 19, 2025Constraining the Prompt Atmospheric Neutrino Flux Combining IceCube's Cascade and Track SamplesNov 24, 2025Limits on GeV-scale WIMP Annihilation in Dwarf Spheroidals with IceCube DeepCoreNov 2, 2025Search for GeV-scale Dark Matter from the Galactic Center with IceCube-DeepCoreOct 28, 2025Characterization of the Three-Flavor Composition of Cosmic Neutrinos with IceCubeOct 15, 2025Evidence for Neutrino Emission from X-Ray-bright Active Galactic Nuclei with IceCubeSep 30, 2025Limiting the Parameter Space for Unstable eV-scale Neutrinos Using IceCube DataAug 20, 2025Identification and Denoising of Radio Signals from Cosmic-Ray Air Showers using Convolutional Neural NetworksAug 5, 2025The LED calibration systems for the mDOM and D-Egg sensor modules of the IceCube UpgradeJul 29, 2025Evidence for a Spectral Break or Curvature in the Spectrum of Astrophysical Neutrinos from 5 TeV--10 PeVJul 11, 2025The IceCube Collaboration -- Contributions to the 39th International Cosmic Ray Conference (ICRC2025)Jul 11, 2025Search for High-Energy Neutrinos From the Sun Using Ten Years of IceCube DataJul 9, 2025All-sky neutrino point-source search with IceCube combined track and cascade dataFeb 25, 2025Seasonal Variations of the Atmospheric Muon Neutrino Spectrum measured with IceCubeFeb 18, 2025Measurement of the inelasticity distribution of neutrino-nucleon interactions for $\mathbf{80~GeV<E_ν<560~GeV}$ with IceCube DeepCoreFeb 13, 2025Search for Heavy Neutral Leptons with IceCube DeepCoreJan 27, 2025Time-Integrated Southern-Sky Neutrino Source Searches with 10 Years of IceCube Starting-Track Events at Energies Down to 1 TeVJan 16, 2025Search for neutrino doublets and triplets using 11.4 years of IceCube dataDec 6, 2024Observation of Cosmic-Ray Anisotropy in the Southern Hemisphere with 12 yr of Data Collected by the IceCube Neutrino ObservatoryOct 2, 2024Limits on the Low-Energy Electron Antineutrino Flux from the Brightest GRB of All TimeSep 29, 2024Search for proton decay via $p\rightarrow{e^+η}$ and $p\rightarrow{μ^+η}$ with a 0.37 Mton-year exposure of Super-Kamiokande