Showing 21–40 of 234 results
/ Date/ Name
Feb 10, 2025Neutrino Interaction Vertex Reconstruction in DUNE with Pandora Deep LearningDec 3, 2024History and Habitability of the LP 890-9 Planetary SystemOct 15, 2024SCExAO/CHARIS Near-Infrared Scattered-Light Imaging and Integral Field Spectropolarimetry of the AB Aurigae Protoplanetary SystemSep 26, 2024The track-length extension fitting algorithm for energy measurement of interacting particles in liquid argon TPCs and its performance with ProtoDUNE-SP dataAug 28, 2024The Remarkable X-ray Spectra and Variability of the Ultraluminous Weak-Line Quasar SDSS J1521+5202Aug 22, 2024DUNE Phase II: Scientific Opportunities, Detector Concepts, Technological SolutionsAug 1, 2024First Measurement of the Total Inelastic Cross-Section of Positively-Charged Kaons on Argon at Energies Between 5.0 and 7.5 GeVJul 25, 2024The DAMIC-M Low Background ChamberJul 14, 2024Supernova Pointing Capabilities of DUNEMar 15, 2024Measurement of the 1-jettiness event shape observable in deep-inelastic electron-proton scattering at HERAMar 13, 2024Observation and differential cross section measurement of neutral current DIS events with an empty hemisphere in the Breit frameMar 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 30, 2024The eROSITA Final Equatorial Depth Survey (eFEDS): the hard X-ray selected sampleDec 5, 2023The DUNE Far Detector Vertical Drift Technology, Technical Design ReportNov 28, 2023Redshifted iron emission and absorption lines in the Chandra X-ray spectrum of Centaurus ANov 8, 2023The High Energy X-ray Probe (HEX-P): Bringing the Cosmic X-ray Background into FocusOct 11, 2023The Slicer Combined with Array of Lenslets for Exoplanet Spectroscopy (SCALES): driving science cases and expected outcomesAug 21, 2023Synergies between interstellar dust and heliospheric science with an Interstellar ProbeMar 29, 2023Impact of cross-section uncertainties on supernova neutrino spectral parameter fitting in the Deep Underground Neutrino Experiment