We present a catalog of fundamental stellar properties for∼ 7500 evolved stars, including
stellar radii and masses, determined from the combination of spectroscopic observations …

Metal-poor stars are key to our understanding of the early stages of chemical evolution in the
Universe. New multifilter surveys, such as the Southern Photometric Local Universe Survey …

The stellar stream connected to the Sagittarius (Sgr) dwarf galaxy is the most massive tidal
stream that has been mapped in the Galaxy, and is the dominant contributor to the outer …

We explore the kinematic and chemical properties of the Monoceros stellar overdensity by
combining data from the Two Micron All Sky Survey, Wide-field Infrared Survey Explorer …

We present a chemical and dynamical analysis of the leading arm (LA) and trailing arm (TA)
of the Sagittarius (Sgr) stream, as well as for the Sgr dwarf galaxy core (SC), using red giant …

We present the first detailed chemical-abundance analysis of stars from the dwarf-galaxy
stellar stream Wukong/LMS-1 covering a wide metallicity range (). We find abundance …

The hierarchical model of galaxy formation predicts that the Milky Way halo is populated by
tidal debris of dwarf galaxies and globular clusters. Due to long dynamical times, debris from …

Carbon abundances, especially at low metallicity, reveal the early chemical evolution of a
system, tracing the supernovae (SNe) that contributed and how much of their ejecta made it …

ABSTRACT The Sagittarius dwarf spheroidal (Sgr dSph) galaxy provides one of the most
convincing examples of tidal interaction between satellite galaxies and the Milky Way (MW) …