Showing 1–20 of 21 results
/ Date/ Name
Jan 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 MethodologyDec 18, 2025The AURORA Survey: The Mass -- Metallicity and Fundamental Metallicity Relations at $z \sim 2.3$ Based Purely on Direct $T_e$ MetallicitiesDec 14, 2025THRILS -- The High-(Redshift+Ionization) Line Search: Program Description & Redshift CatalogAug 13, 2025The AURORA Survey: High-Redshift Empirical Metallicity Calibrations from Electron Temperature Measurements at z=2-10Apr 3, 2025Detection of Deuterated Hydrocarbon Nanoparticles in the Whirlpool Galaxy, M51May 29, 2024CHAOS VIII: Far-Ultraviolet Spectra of M101 and The Impact of Wolf-Rayet StarsMar 13, 2024CLASSY IX: The Chemical Evolution of the Ne, S, Cl, and Ar ElementsDec 15, 2023The Next Generation Deep Extragalactic Exploratory Public Near-Infrared Slitless Survey Epoch 1 (NGDEEP-NISS1): Extra-Galactic Star-formation and Active Galactic Nuclei at 0.5 < z < 3.6Feb 10, 2023The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) SurveySep 8, 2022CHAOS VII: A Large-Scale Direct Abundance Study in M33Aug 4, 2022A First Look at the Abundance Pattern -- O/H, C/O, and Ne/O -- in $z>7$ Galaxies with JWST/NIRSpecJun 2, 2022CLASSY II: A technical Overview of the COS Legacy Archive Spectroscopic SurveYApr 12, 2022Chiral symmetry restoration at high matter density observed in pionic atomsSep 1, 2021A comprehensive chemical abundance analysis of the extremely metal poor Leoncino Dwarf galaxy (AGC 198691)May 7, 2021CHAOS VI: Direct Abundances in NGC 2403Apr 22, 2020CHAOS V: Recombination Line Carbon Abundances in M101Jan 14, 2020CHAOS IV: Gas-Phase Abundance Trends From The First Four CHAOS Galaxies