Showing 1–20 of 44 results
/ Date/ Name
Dec 19, 2025Constraining the Prompt Atmospheric Neutrino Flux Combining IceCube's Cascade and Track SamplesOct 16, 2025Measurement of $C\!P$ asymmetry in $D^0 \to K^0_{\rm S} K^0_{\rm S}$ decays with Run 3 dataSep 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 ObservatoryJan 22, 2024Citizen Science for IceCube: Name that NeutrinoJan 20, 2024Prompt and nonprompt $ψ(2S)$ production in $p$Pb collisions at $\sqrt{s_{NN}}=8.16$ TeVDec 14, 2023Amplitude analysis of the $B^{0}\to K^{*0}μ^+μ^-$ decayNov 17, 2023A model-independent measurement of the CKM angle $γ$ in partially reconstructed $B^{\pm} \to D^{*} h^{\pm}$ decays with $D \to K_{S}^{0} h^{+}h^{-}$ $(h=π, K)$Oct 6, 2023Measurement of the CKM angle $γ$ using the $B^{\pm}\rightarrow D^{*} h^{\pm}$ channels