Showing 41–60 of 120 results
/ Date/ Name
Aug 26, 2021Final Targeting Strategy for the SDSS-IV APOGEE-2S SurveyDec 5, 2019The Sixteenth Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS SpectraFeb 17, 2022Quantifying radial migration in the Milky Way: Inefficient over short timescales but essential to the very outer disc beyond ~15 kpcApr 8, 2022The chemical characterisation of halo substructure in the Milky Way based on APOGEEJul 9, 2019The Origin of Elements Across Cosmic Time: Astro2020 Science White PaperSep 4, 2012The Milky Way's circular velocity curve between 4 and 14 kpc from APOGEE dataMar 13, 2014Discovery of Two Rare Rigidly-Rotating Magnetosphere Stars in the APOGEE SurveyOct 6, 2014Bayesian distances and extinctions for giants observed by Kepler and APOGEEJan 29, 2015The Cannon: A data-driven approach to stellar label determinationMar 7, 2015Chemical Cartography with APOGEE: Metallicity Distribution Functions and the Chemical Structure of the Milky Way DiskFeb 17, 2015The APOGEE Spectroscopic Survey of Kepler Planet Hosts: Feasibility, Efficiency, and First ResultsMay 27, 2015IN-SYNC III: The dynamical state of IC 348 - A super-virial velocity dispersion and a puzzling sign of convergenceMay 22, 2015The SDSS-IV in 2014: A Demographic SnapshotApr 17, 2018The APOGEE-2 Survey of the Orion Star Forming Complex: I. Target Selection and Validation with early observationsSep 4, 2024A Comprehensive Study of Open Cluster Chemical Homogeneity using APOGEE and Milky Way Mapper AbundancesNov 11, 2010SDSS-III/APOGEE: Detailed Abundances of Galactic Star ClustersDec 4, 2020SDSS-IV MaNGA: galaxy gas-phase metallicity gradients vary across the mass-size planeJan 9, 2020The Chemical Compositions of Accreted and {\it in situ} Galactic Globular Clusters According to SDSS/APOGEEMay 5, 2014The APOGEE red-clump catalog: Precise distances, velocities, and high-resolution elemental abundances over a large area of the Milky Way's diskSep 16, 2014High-resolution, H band Spectroscopy of Be Stars with SDSS-III/APOGEE: I. New Be Stars, Line Identifications, and Line Profiles