Showing 41–60 of 317 results
/ Date/ Name
Jul 1, 2024Measurement of the integrated luminosity of data samples collected during 2019-2022 by the Belle II experimentJun 18, 2024The giant outburst of EXO 2030+375 II: Broadband spectroscopy and evolutionMay 31, 2024The giant outburst of EXO 2030+375 I: Spectral and pulse profile evolutionMay 30, 2024Search for the decay $B^{0}\toγγ$ using Belle and Belle II dataMay 12, 2024Search for lepton-flavor-violating $τ^- \to μ^-μ^+μ^-$ decays at Belle IIApr 19, 2024Determination of the CKM angle $φ_{3}$ from a combination of Belle and Belle II resultsMar 19, 2024QUBIQ: Uncertainty Quantification for Biomedical Image Segmentation ChallengeFeb 13, 2024The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy ClustersJan 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 20, 2023Search for the $e^+e^-\toη_{b}(1S)ω$ and $e^+e^-\toχ_{b0}(1P)ω$ processes at $\sqrt{s}=10.745\,\mathrm{GeV}$Dec 14, 2023Amplitude analysis of the $B^{0}\to K^{*0}μ^+μ^-$ decayDec 14, 2023EWOCS-I: The catalog of X-ray sources in Westerlund 1 from the Extended Westerlund 1 and 2 Open Clusters SurveyNov 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 13, 2023First Measurement of $R(X_{τ/\ell})$ as an Inclusive Test of the $b \to c τν$ AnomalyOct 11, 2023Chasing Gravitational Waves with the Cherenkov Telescope ArrayOct 6, 2023Measurement of the CKM angle $γ$ using the $B^{\pm}\rightarrow D^{*} h^{\pm}$ channelsSep 23, 2023Inclusive e$^+$e$^-$ production in collisions of pions with protons and nuclei in the second resonance region of baryonsSep 21, 2023Search for Continuous and Transient Neutrino Emission Associated with IceCube's Highest-Energy Tracks: An 11-Year Analysis