Showing 41–60 of 98 results
/ Date/ Name
Feb 15, 2023Searching for TeV Dark Matter in Irregular dwarf galaxies with HAWC ObservatoryDec 13, 2022Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCoreDec 6, 2024Observation of Cosmic-Ray Anisotropy in the Southern Hemisphere with 12 yr of Data Collected by the IceCube Neutrino ObservatoryNov 2, 2025Search for GeV-scale Dark Matter from the Galactic Center with IceCube-DeepCoreJun 24, 2025Measurement of the mean number of muons with energies above 500 GeV in air showers detected with the IceCube Neutrino ObservatoryJul 29, 2025Improved measurements of the TeV-PeV extragalactic neutrino spectrum from joint analyses of IceCube tracks and cascadesSep 8, 2023HAWC Study of Very-High-Energy $γ$-ray Spectrum of HAWC J1844-034Feb 27, 2023Detailed Analysis of the TeV γ-Ray Sources 3HWC J1928+178, 3HWC J1930+188, and the New Source HAWC J1932+192Dec 18, 2025Prompt Searches for Very-High-Energy γ-Ray Counterparts to IceCube Astrophysical Neutrino AlertsNov 25, 2022Searches for Neutrinos from LHAASO ultra-high-energy γ-ray sources using the IceCube Neutrino ObservatoryOct 10, 2022Constraints on populations of neutrino sources from searches in the directions of IceCube neutrino alertsApr 24, 2023Measurement of Atmospheric Neutrino Mixing with Improved IceCube DeepCore Calibration and Data ProcessingApr 3, 2023IceCat-1: the IceCube Event Catalog of Alert TracksMar 8, 2023Observation of Seasonal Variations of the Flux of High-Energy Atmospheric Neutrinos with IceCubeMar 28, 2023A Search for IceCube sub-TeV Neutrinos Correlated with Gravitational-Wave Events Detected By LIGO/VirgoMar 4, 2024Improved modeling of in-ice particle showers for IceCube event reconstructionApr 30, 2024Acceptance Tests of more than 10 000 Photomultiplier Tubes for the multi-PMT Digital Optical Modules of the IceCube UpgradeJun 11, 2024IceCube Search for Neutrino Emission from X-ray Bright Seyfert GalaxiesJul 1, 2024Probing the connection between IceCube neutrinos and MOJAVE AGNJul 15, 2024Testing the Molecular Cloud Paradigm for Ultra-High-Energy Gamma Ray Emission from the Direction of SNR G106.3+2.7