Showing 21–40 of 102 results
/ Date/ Name
Jun 30, 2025Anchoring Stellar Age Indicators: A Cross-Calibration of [C/N] and Gyrochronology Ages via the Age-Velocity-Dispersion RelationOct 20, 2025Extending the [C/N]-Age Calibration: Using Globular Clusters to Explore Older and Metal-Poor PopulationsDec 3, 2021The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 DataSep 25, 2025A nearly pristine star from the Large Magellanic CloudJul 25, 2018APOGEE Data Releases 13 and 14: Data and AnalysisJan 14, 2019Dynamical heating across the Milky Way disc using APOGEE and $\it{Gaia}$Jul 25, 2023Assessing the Accuracy of TESS Asteroseismology with APOGEEMar 16, 2023A Review of the Mixing Length Theory of Convection in 1D Stellar ModelingJul 6, 2023Asteroseismology with the Roman Galactic Bulge Time-Domain SurveyApr 20, 2023The APO-K2 Catalog. I. 7,673 Red Giants with Fundamental Stellar Parameters from APOGEE DR17 Spectroscopy and K2-GAP AsteroseismologyApr 18, 2022Characterizing Observed Extra Mixing Trends in Red Giants using the Reduced Density Ratio from Thermohaline ModelsOct 3, 2021Stellar multiplicity and stellar rotation: Insights from APOGEENov 30, 2020Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the $\it{TESS}$ Continuous Viewing Zones and beyondMar 19, 2019Astro2020 Science White Paper: Stellar Physics and Galactic Archeology using Asteroseismology in the 2020'sSep 13, 2019Insights from the APOKASC Determination of the Evolutionary State of Red-Giant Stars by consolidation of different methodsJan 31, 2013Precise High-Cadence Time Series of Five Variable Young Stars in Auriga with MOSTMay 12, 2017Asteroseismology and Gaia: Testing Scaling Relations Using 2200 Kepler Stars with TGAS ParallaxesNov 15, 2023SDSS-IV from 2014 to 2016: A Detailed Demographic Comparison over Three YearsApr 7, 2025Rotationally Driven Ultraviolet Emission of Red Giant Stars II. Metallicity, Activity, Binarity and Sub-subgiantsSep 15, 2025TESS Subgiant and Lower Red Giant Asteroseismology in the Continuous Viewing Zones