Showing 1–20 of 325 results
/ Date/ Name
Apr 22, 2026Direct construction of scalar quantum fields by L{é}vy fields -- nontrivial exact Wightman fields in a wider field with a relaxed Gårding-Wightman Axioms-Apr 20, 2026Proposing Topic Models and Evaluation Frameworks for Analyzing Associations with External Outcomes: An Application to Leadership Analysis Using Large-Scale Corporate Review DataApr 20, 2026The General Antiparticle Spectrometer (GAPS) Antarctic Balloon PayloadMar 25, 2026A Fast, Hot Wind from a Nuclear StarburstDec 25, 2025Phylogenetics in a warm place: computational aspects of the Tropical GrassmannianDec 19, 2025Constraining the Prompt Atmospheric Neutrino Flux Combining IceCube's Cascade and Track SamplesDec 6, 2025A XRISM/Resolve view of the dynamics in the hot gaseous atmosphere of M87Nov 24, 2025Limits on GeV-scale WIMP Annihilation in Dwarf Spheroidals with IceCube DeepCoreNov 11, 2025Search for Dark Particles in $K^0_L \to γX$ at the KOTO ExperimentNov 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 28, 2025XRISM constraints on unidentified X-ray emission lines, including the 3.5 keV line, in the stacked spectrum of ten galaxy clustersOct 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 DataSep 29, 2025High-Precision Temperature Estimation Based on Magnetic Nanoparticles Dominated by Brownian Relaxation under Combined AC and DC Magnetic FieldsSep 18, 2025Stratified wind from a super-Eddington X-ray binary is slower than expectedAug 20, 2025Identification and Denoising of Radio Signals from Cosmic-Ray Air Showers using Convolutional Neural NetworksAug 7, 2025XRISM/Resolve View of Abell 2319: Turbulence, Sloshing, and ICM DynamicsAug 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 PeV