Showing 61–80 of 355 results
/ Date/ Name
Jul 16, 2024Calibration and simulation of ionization signal and electronics noise in the ICARUS liquid argon time projection chamberJul 14, 2024Supernova Pointing Capabilities of DUNEJun 13, 2024Probing the polarized emission from SMC X-1: the brightest X-ray pulsar observed by IXPEJun 8, 2024The PLATO MissionMay 24, 2024Searches for new physics below twice the electron mass with GERDAMay 13, 2024JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noonApr 16, 2024First double-differential cross section measurement of neutral-current $π^0$ production in neutrino-argon scattering in the MicroBooNE detectorApr 16, 2024Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometryApr 11, 2024Birds of a Feather: Resolving Stellar Mass Assembly With JWST/NIRCam in a Pair of Kindred $z \sim 2$ Dusty Star-forming Galaxies Lensed by the PLCK G165.7+67.0 ClusterMar 27, 2024JWST Photometric Time-Delay and Magnification Measurements for the Triply-Imaged Type Ia "Supernova H0pe" at z = 1.78Mar 5, 2024Performance of a modular ton-scale pixel-readout liquid argon time projection chamberFeb 29, 2024The ArgusSpec Prototype: Autonomous Spectroscopic Follow-up of Flares Detected by Large Array TelescopesFeb 29, 2024Inclusive cross section measurements in final states with and without protons for charged-current $ν_μ$-Ar scattering in MicroBooNEFeb 13, 2024The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy ClustersFeb 2, 2024Doping Liquid Argon with Xenon in ProtoDUNE Single-Phase: Effects on Scintillation LightJan 29, 2024MIRI MRS Observations of Beta Pictoris I. The Inner Dust, the Planet, and the GasJan 20, 2024Prompt and nonprompt $ψ(2S)$ production in $p$Pb collisions at $\sqrt{s_{NN}}=8.16$ TeVJan 10, 2024TREASUREHUNT: Transients and Variability Discovered with HST in the JWST North Ecliptic Pole Time Domain FieldDec 18, 2023JWST's PEARLS: 119 multiply imaged galaxies behind MACS0416, lensing properties of caustic crossing galaxies, and the relation between halo mass and number of globular clusters at $z=0.4$Dec 14, 2023Amplitude analysis of the $B^{0}\to K^{*0}μ^+μ^-$ decay