Showing 161–180 of 8,707 results
/ Date/ Name
Feb 6, 2026Non-spherical BUFFALOs: a weak lensing view of the Frontier Field clusters and associated systematicsFeb 6, 2026Prediction-based inference for integrated diffusions with high-frequency dataFeb 6, 2026First results from the E302 efficiency$\unicode{x2013}$instability experiment at the FACET-II facilityFeb 6, 2026The Walkaway Star HP Tau/G2: Evidence for a Stellar MergerFeb 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 4, 2026From Evaluation to Design: Using Potential Energy Surface Smoothness Metrics to Guide Machine Learning Interatomic Potential ArchitecturesFeb 3, 2026The Tarantula massive binary monitoring VII. The nature of the eccentric O+BH binary candidate VFTS 812Feb 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 1, 2026PersistBench: When Should Long-Term Memories Be Forgotten by LLMs?Jan 29, 2026The LBT $Y_{\rm p}$ Project V: Cosmological Implications of a New Determination of Primordial $^4$HeJan 29, 2026The LBT Y$_\mathrm{p}$ Project IV: A New Value of the Primordial Helium AbundanceJan 29, 2026The LBT $Y_{\rm p}$ Project III: LUCI Spectra of Metal-Poor NebulaeJan 29, 2026The LBT $Y_{\rm p}$ Project II: MODS Spectra, Physical Conditions, and Oxygen Abundances in Local Metal-Poor NebulaeJan 29, 2026The LBT $Y_{\rm p}$ Project I: An Improved Determination of the Primordial Helium Abundance -- Project Description, Sample Selection, Observations, and MethodologyJan 29, 2026The Little Blue and Red Dots Rosetta Stones: Non-Gaussian broad lines, hot dust, and X-ray weaknessJan 28, 202627 years of Spaceborne IR Astronomy: An ISO, Spitzer, WISE and NEOWISE Survey for Large-Amplitude Variability in Young Stellar ObjectsJan 28, 2026It's More Complicated Than You Think: A Forward Model to Infer the Recent Star Formation History, Bursty or Not, of Galaxy PopulationsJan 28, 2026Trigger Optimization and Event Classification for Dark Matter Searches in the CYGNO Experiment Using Machine Learning