Showing 1–20 of 52 results
/ Date/ Name
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 MethodologyNov 28, 2025CECILIA: The Mass-Metallicity Relation of Low-Mass Galaxies at Cosmic NoonSep 22, 2025CECILIA: Gas-Phase Physical Conditions and Multi-Element Chemistry at Cosmic NoonJul 29, 2025CECILIA: Ultra-Deep Rest-Optical Spectra of Faint Galaxies at Cosmic NoonApr 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 13, 2023CECILIA: Direct O, N, S, and Ar Abundances in Q2343-D40, a Galaxy at $z\sim$3Oct 9, 2023Sharing Information Between Machine Tools to Improve Surface Finish ForecastingSep 19, 2023A spectrum of physics-informed Gaussian processes for regression in engineeringAug 25, 2023CECILIA: The Faint Emission Line Spectrum of z~2-3 Star-forming GalaxiesAug 21, 2023HST UV Spectroscopy of the Dwarf Starburst Galaxy Pox 186Sep 8, 2022CHAOS VII: A Large-Scale Direct Abundance Study in M33Sep 8, 2022A Bayesian Method for Material Identification of Composite Plates via Dispersion CurvesAug 4, 2022A First Look at the Abundance Pattern -- O/H, C/O, and Ne/O -- in $z>7$ Galaxies with JWST/NIRSpecJun 30, 2022Physics-informed machine learning for Structural Health Monitoring