Showing 1–20 of 45 results
/ Date/ Name
Nov 4, 2016Chemical trends in the Galactic Halo with APOGEE dataApr 25, 2019Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18Feb 14, 2024Chronology of our Galaxy from Gaia Colour-Magnitude Diagram-fitting (ChronoGal). I. The formation and evolution of the thin disk from the Gaia Catalogue of Nearby StarsMar 21, 2025Chronology of our Galaxy from Gaia CMD-fitting (ChronoGal): the early formation of the Milky Way disk and the impact of Gaia-Sausage-EnceladusAug 31, 2020Cool stars in the Galactic Center as seen by APOGEE: M giants, AGB stars and supergiant stars/candidatesJul 25, 2020The Milky Way bar and bulge revealed by APOGEE DR16 and Gaia EDR3Mar 30, 2018Chemo-kinematics of the Milky Way from the SDSS-III MARVELS SurveyDec 3, 2015Physical properties of star clusters in the outer LMC as observed by the Dark Energy SurveyJul 9, 2024Transferring spectroscopic stellar labels to 217 million Gaia DR3 XP stars with SHBoostFeb 12, 2026Abundances in 78 metal-rich bulge spheroid stars from APOGEEJul 28, 2020How Many Components? Quantifying the Complexity of the Metallicity Distribution in the Milky Way Bulge with APOGEEJun 8, 2023Beyond Gaia DR3: Tracing the [$α$/M]-[M/H] bimodality from the inner to the outer Milky Way disc with Gaia-RVS and convolutional neural networksApr 27, 2020The RAdial Velocity Experiment (RAVE): Parameterisation of RAVE spectra based on convolutional neural networksOct 17, 2024Abundances of iron-peak elements in 58 bulge spheroid stars from APOGEEJul 15, 2025Abundances of P, S, and K in 58 bulge spheroid stars from APOGEEMar 4, 2019Kinematics with Gaia DR2: The Force of a DwarfNov 28, 2022The Pristine Inner Galaxy Survey (PIGS) VI: Different vertical distributions between two DIBs at 442.8 nm and 862.1 nmJul 21, 2023Exploring the short-term variability of H$α$ and H$β$ emissions in a sample of M dwarfsAug 13, 2022Abundance analysis of APOGEE spectra for 58 metal-poor stars from the bulge spheroidFeb 14, 2023Parameters for > 300 million Gaia stars: Bayesian inference vs. machine learning