Showing 1–20 of 44 results
/ Date/ Name
Apr 9, 2026Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing StrategiesAug 26, 2025Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array ObservatoryMar 7, 2024Dark Matter Line Searches with the Cherenkov Telescope ArrayJan 22, 2024Citizen Science for IceCube: Name that NeutrinoSep 21, 2023Search for Continuous and Transient Neutrino Emission Associated with IceCube's Highest-Energy Tracks: An 11-Year AnalysisJul 24, 2023The IceCube-Gen2 Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC2023)Jul 10, 2023Observation of high-energy neutrinos from the Galactic planeMar 23, 2023Search for neutrino lines from dark matter annihilation and decay with IceCubeDec 13, 2022A Search for Coincident Neutrino Emission from Fast Radio Bursts with Seven Years of IceCube Cascade EventsNov 18, 2022Evidence for neutrino emission from the nearby active galaxy NGC 1068Jul 11, 2022Search for Astrophysical Neutrinos from 1FLE Blazars with IceCubeMay 25, 2022Searches for Connections between Dark Matter and High-Energy Neutrinos with IceCubeMay 23, 2022Searches for Neutrinos from Gamma-Ray Bursts using the IceCube Neutrino ObservatoryJan 18, 2022Search for Spatial Correlations of Neutrinos with Ultra-High-Energy Cosmic RaysNov 18, 2021Search for GeV-scale Dark Matter Annihilation in the Sun with IceCube DeepCoreJul 14, 2021The IceCube-Gen2 Collaboration -- Contributions to the 37th International Cosmic Ray Conference (ICRC2021)Jul 14, 2021The IceCube Collaboration -- Contributions to the 37th International Cosmic Ray Conference (ICRC2021)Jul 7, 2021Search for High-Energy Neutrinos from Ultra-Luminous Infrared Galaxies with IceCubeMar 31, 2021A muon-track reconstruction exploiting stochastic losses for large-scale Cherenkov detectorsJun 29, 2020Measurements of the Time-Dependent Cosmic-Ray Sun Shadow with Seven Years of IceCube Data -- Comparison with the Solar Cycle and Magnetic Field Models