Showing 101–120 of 522 results
/ Date/ Name
Mar 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 SRG/eROSITA all-sky survey: First X-ray catalogues and data release of the western Galactic hemisphereJan 22, 2024Citizen Science for IceCube: Name that NeutrinoJan 20, 2024Prompt and nonprompt $ψ(2S)$ production in $p$Pb collisions at $\sqrt{s_{NN}}=8.16$ TeVDec 14, 2023Amplitude analysis of the $B^{0}\to K^{*0}μ^+μ^-$ decayDec 6, 2023The Initial Mass Function Based on the Full-sky 20-pc Census of $\sim$3,600 Stars and Brown DwarfsDec 5, 2023The DUNE Far Detector Vertical Drift Technology, Technical Design ReportDec 1, 2023Euclid preparation. XLI. Galaxy power spectrum modelling in real spaceNov 17, 2023A model-independent measurement of the CKM angle $γ$ in partially reconstructed $B^{\pm} \to D^{*} h^{\pm}$ decays with $D \to K_{S}^{0} h^{+}h^{-}$ $(h=π, K)$Oct 24, 2023Euclid preparation. LII. Forecast impact of super-sample covariance on 3x2pt analysis with EuclidOct 14, 2023CWISE J105512.11+544328.3: A Nearby Y Dwarf Spectroscopically Confirmed with Keck/NIRESOct 13, 2023Open X-Embodiment: Robotic Learning Datasets and RT-X ModelsOct 6, 2023Measurement of the CKM angle $γ$ using the $B^{\pm}\rightarrow D^{*} h^{\pm}$ channelsOct 4, 2023Identifying physical structures in our Galaxy with Gaussian Mixture Models: An unsupervised machine learning techniqueOct 2, 2023The SOFIA FEEDBACK Legacy Survey: Rapid molecular cloud dispersal in RCW 79Sep 21, 2023Search for Continuous and Transient Neutrino Emission Associated with IceCube's Highest-Energy Tracks: An 11-Year AnalysisSep 11, 2023Measurement of the CKM angle $γ$ in the $B^0 \to DK^{*0}$ channel using self-conjugate $D \to K_S^0 h^+ h^-$ decaysSep 8, 2023Study of Io's sodium jets with the TRAPPIST telescopesSep 6, 2023Prospects for combined analyses of hadronic emission from $γ$-ray sources in the Milky Way with CTA and KM3NeT