Showing 1–20 of 31 results
/ Date/ Name
Jun 2, 2025Science Prospects for the Southern Wide-field Gamma-ray Observatory: SWGOJul 10, 2023Observation of high-energy neutrinos from the Galactic planeNov 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 ModelsMay 26, 2020Searching for eV-scale sterile neutrinos with eight years of atmospheric neutrinos at the IceCube neutrino telescopeApr 6, 2020IceCube Search for Neutrinos Coincident with Compact Binary Mergers from LIGO-Virgo's First Gravitational-Wave Transient CatalogMar 26, 2020IceCube Search for High-Energy Neutrino Emission from TeV Pulsar Wind NebulaeJan 6, 2020A search for IceCube events in the direction of ANITA neutrino candidatesNov 6, 2019Neutrino astronomy with the next generation IceCube Neutrino ObservatoryOct 15, 2019Design and Performance of the first IceAct Demonstrator at the South PoleSep 4, 2019Efficient propagation of systematic uncertainties from calibration to analysis with the SnowStorm method in IceCube