Showing 41–60 of 282 results
/ Date/ Name
Jul 14, 2024Supernova Pointing Capabilities of DUNEJun 14, 2024An experimental search for an explanation of the difference between beam and bottle neutron lifetime measurementsApr 24, 2024The Ethics of Advanced AI AssistantsApr 16, 2024Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometryApr 11, 2024A broad linewidth, compact, millimeter-bright molecular emission line source near the Galactic CenterApr 11, 2024Orbital and Atmospheric Characterization of the 1RXS J034231.8+121622 System Using High-Resolution Spectroscopy Confirms That The Companion is a Low-Mass StarMar 27, 2024YAP:Ce scintillator as an absolute ultracold neutron detectorMar 26, 2024Vortex Fiber Nulling for Exoplanet Observations: First Direct Detection of M Dwarf Companions around HIP 21543, HIP 94666, and HIP 50319Mar 5, 2024Performance of a modular ton-scale pixel-readout liquid argon time projection chamberFeb 2, 2024Doping Liquid Argon with Xenon in ProtoDUNE Single-Phase: Effects on Scintillation LightJan 20, 2024Prompt and nonprompt $ψ(2S)$ production in $p$Pb collisions at $\sqrt{s_{NN}}=8.16$ TeVDec 18, 2023Smartpixels: Towards on-sensor inference of charged particle track parameters and uncertaintiesDec 14, 2023Amplitude analysis of the $B^{0}\to K^{*0}μ^+μ^-$ decayDec 5, 2023The DUNE Far Detector Vertical Drift Technology, Technical Design ReportDec 4, 2023Validation of elemental and isotopic abundances in late-M spectral types with the benchmark HIP 55507 AB systemNov 30, 2023Atmospheric metallicity and C/O of HD 189733 b from high-resolution spectroscopyNov 17, 2023A model-independent measurement of the CKM angle $γ$ in partially reconstructed $B^{\pm} \to D^{*} h^{\pm}$ decays with $D \to K_{S}^{0} h^{+}h^{-}$ $(h=π, K)$Nov 9, 2023Neural Network Methods for Radiation Detectors and ImagingOct 26, 2023Ready for O4 II: GRANDMA Observations of Swift GRBs during eight-weeks of Spring 2022Oct 24, 2023A roadmap for the atmospheric characterization of terrestrial exoplanets with JWST