Showing 181–200 of 10,192 results
/ Date/ Name
Feb 10, 2026Investigating the Nested Structure of the Outflow from the Low Luminosity Protostar IRAS 16253-2429 using JWST and ALMAFeb 6, 2026Non-spherical BUFFALOs: a weak lensing view of the Frontier Field clusters and associated systematicsFeb 6, 2026First results from the E302 efficiency$\unicode{x2013}$instability experiment at the FACET-II facilityFeb 6, 2026The Non-Eruptive Reconfiguration of a Quiescent Filament After a Nearby Active Region EmergenceFeb 6, 2026The Walkaway Star HP Tau/G2: Evidence for a Stellar MergerFeb 5, 2026Venting and Outgassing Simulations of Pressurized Lunar Modules: Contamination of the Lunar EnvironmentFeb 5, 2026The JWST EXCELS survey: The ages and abundances of $3<z<5$ massive quiescent galaxies show that downsizing was already in place by $z\simeq4$Feb 5, 2026Early growth of massive black holes in dynamical dark energy models with negative cosmological constantFeb 4, 2026From Evaluation to Design: Using Potential Energy Surface Smoothness Metrics to Guide Machine Learning Interatomic Potential ArchitecturesFeb 3, 2026Production of GEM-like structures for cryogenic applications, using laser-cutting techniquesFeb 3, 2026A surprisingly large asymmetric ejection from Mira AFeb 2, 2026Mitigating half-wave plate systematics at the map-making level: calibration requirements for LiteBIRDFeb 2, 2026PRISMS. UNCOVER-26185, a metal-poor SFG at z=10.05 with no evidence for a X-ray-luminous AGNFeb 2, 2026PRISMS. U37126, a very blue, ISM-naked starburst at z=10.255 with nearly 100% Lyman continuum escape fractionFeb 2, 2026A whole-planet model of the Earth without life for terrestrial exoplanet studiesFeb 2, 2026Noble gases Neon and argon: a role for the chemical patterns of multiple populations in globular clusters?Jan 30, 2026DimABSA: Building Multilingual and Multidomain Datasets for Dimensional Aspect-Based Sentiment AnalysisJan 29, 2026Fast, dust-poor outflows in the local candidate dual AGN MCG-03-34-64 observed with VLT/ERISJan 29, 2026The Little Blue and Red Dots Rosetta Stones: Non-Gaussian broad lines, hot dust, and X-ray weaknessJan 28, 2026Performance of the Particle-Identification Silicon-Telescope Array Coupled with the VAMOS++ Magnetic Spectrometer