Showing 21–40 of 249 results
/ Date/ Name
Dec 25, 2024Quality Assurance and Quality Control of the $26~\text{m}^2$ SiPM production for the DarkSide-20k dark matter experimentJul 24, 2024Chemical tracers of a highly eccentric AGB-main sequence star binaryJul 12, 2024The ALMA-CRISTAL survey: Dust temperature and physical conditions of the interstellar medium in a typical galaxy at z=5.66May 21, 2024V892 Tau: A tidally perturbed circumbinary disc in a triple stellar systemApr 16, 2024Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometryFeb 25, 2024Deep Neural Network Initialization with Sparsity Inducing ActivationsFeb 25, 2024MoodCapture: Depression Detection Using In-the-Wild Smartphone ImagesFeb 8, 2024UNCOVER NIRSpec/PRISM Spectroscopy Unveils Evidence of Early Core Formation in a Massive, Centrally Dusty Quiescent Galaxy at $z_{spec}=3.97$Feb 5, 2024Trillion Parameter AI Serving Infrastructure for Scientific Discovery: A Survey and VisionJan 8, 2024Probing initial distributions of orbital eccentricity and disc misalignment via polar discsDec 25, 2023GenCast: Diffusion-based ensemble forecasting for medium-range weatherDec 1, 2023The Automatic Identification and Tracking of Coronal Flux Ropes -- Part II: New Mathematical Morphology-based Flux Rope Extraction Method and Deflection AnalysisNov 27, 2023The Heavy Metal Survey: Star Formation Constraints and Dynamical Masses of 21 Massive Quiescent Galaxies at $z=1.3-2.3$Jun 30, 2023A VERITAS/Breakthrough Listen Search for Optical TechnosignaturesJun 26, 2023The Automatic Identification and Tracking of Coronal Flux Ropes -- Part I: Footpoints and FluxesJun 13, 2023Strong Interaction Physics at the Luminosity Frontier with 22 GeV Electrons at Jefferson LabJun 13, 2023Observational Signatures of Circumbinary Discs I: KinematicsMay 9, 2023Coronal Heating as Determined by the Solar Flare Frequency Distribution Obtained by Aggregating Case StudiesMay 5, 2023A Race Track Trapped-Ion Quantum ProcessorMay 5, 2023The role of the drag force in the gravitational stability of dusty planet-forming disc -- II. Numerical simulations