Showing 1–20 of 66 results
/ Date/ Name
Apr 11, 2026Full-polarization millimeter wavelength variability of Sagittarius A* during the 2018 EHT campaignJan 19, 2026Locating the missing large-scale emission in the jet of M87* with short EHT baselinesDec 2, 2025Probing jet base emission of M87* with the 2021 Event Horizon Telescope observationsOct 16, 2025Measurement of $C\!P$ asymmetry in $D^0 \to K^0_{\rm S} K^0_{\rm S}$ decays with Run 3 dataSep 30, 2025The twin red giant branch system BD+20 5391 A case study of low-mass double-core evolutionMay 23, 2025Source Separation of Small Classical Ensembles: Challenges and OpportunitiesMay 15, 2025Origin of the ring ellipticity in the black hole images of M87*Mar 31, 2025Quantum Information meets High-Energy Physics: Input to the update of the European Strategy for Particle PhysicsJan 9, 2025A multi-frequency study of sub-parsec jets with the Event Horizon TelescopeOct 9, 2024First Very Long Baseline Interferometry Detections at 870μmSep 8, 2024The first Cadenza challenges: using machine learning competitions to improve music for listeners with a hearing lossApr 12, 2024Absolute dimensions of solar-type eclipsing binaries. NY Hya: A test for magnetic stellar evolution modelsMar 22, 2024A 500 pc volume-limited sample of hot subluminous stars I. Space density, scale height, and population propertiesFeb 1, 2024Ordered magnetic fields around the 3C 84 central black holeJan 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 JWST Early Release Science Program for Direct Observations of Exoplanetary Systems V: Do Self-Consistent Atmospheric Models Represent JWST Spectra? A Showcase With VHS 1256 bDec 6, 2023The Initial Mass Function Based on the Full-sky 20-pc Census of $\sim$3,600 Stars and Brown DwarfsNov 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 5, 2023MELCHIORS: The Mercator Library of High Resolution Stellar Spectroscopy