The Gaia mission has provided an invaluable wealth of astrometric data for more than a
billion stars in our Galaxy. The synergy between Gaia astrometry, photometry, and …

We combine spectroscopic, photometric, and astrometric information from APOGEE data
release 17 and Gaia early data release 3 to perform a self-consistent characterization of …

Carbon-enhanced metal-poor (CEMP) stars are a unique resource for Galactic archaeology
because they probe the properties of the First Stars, early chemical evolution, and binary …

We construct a sample of 644 carbon-enhanced metal-poor (CEMP) stars with abundance
analyses based on moderate-to high-resolution spectroscopic studies. Dynamical …

We use the 17th data release of the second phase of the Apache Point Observatory Galactic
Evolution Experiment (APOGEE-2) to provide a homogenous census of N-rich red giant …

The r-process-enhanced (RPE) stars provide fossil records of the assembly history of the
Milky Way (MW) and the nucleosynthesis of the heaviest elements. Observations by the R …

We present precise photometric estimates of stellar parameters, including effective
temperature, metallicity, luminosity classification, distance, and stellar age, for nearly 26 …

We employ a sample of 135 873 RR Lyrae stars (RRLs) with precise photometric-metallicity
and distance estimates from the newly calibrated P–ϕ31–R 21–[Fe/H] and Gaia G band P–R …

We combine the power of two stream-searching tools, STREAMFINDER and StarGO applied
to the Gaia EDR3 data, to detect stellar debris belonging to the Cetus stream system that …

Orbital characteristics based on Gaia Early Data Release 3 astrometric parameters are
analyzed for∼ 1700 r-process-enhanced (RPE;[Eu/Fe]>+ 0.3) metal-poor stars ([Fe/H]≤ …