There has been an incredibly large investment in obtaining high-resolution stellar spectra for
determining chemical abundances of stars. This information is crucial to answer …

Understanding the origin of the elements has been a decades-long pursuit, with many open
questions remaining. Old stars found in the Milky Way and its dwarf satellite galaxies can …

To reach a deeper understanding of the origin of elements in the periodic table, we construct
Galactic chemical evolution (GCE) models for all stable elements from C (A= 12) to U (A …

We present the first data release of the SkyMapper Southern Survey, a hemispheric survey
carried out with the SkyMapper Telescope at Siding Spring Observatory in Australia. Here …

Neutron-star mergers were recently confirmed as sites of rapid-neutron-capture (r-process)
nucleosynthesis,–. However, in Galactic chemical evolution models, neutron-star mergers …

The abundances of carbon, oxygen, and iron in late-type stars are important parameters in
exoplanetary and stellar physics, as well as key tracers of stellar populations and Galactic …

We present the Pristine survey, a new narrow-band photometric survey focused on the
metallicity-sensitive Ca H&K lines and conducted in the Northern hemisphere with the wide …

We compare the elemental abundance patterns of∼ 200 extremely metal-poor
(EMP;[Fe/H]<− 3) stars to the supernova yields of metal-free stars, in order to obtain insights …

ABSTRACT Pristine_183. 6849+ 04.8619 (P1836849) is an extremely metal-poor ([Fe/H]=−
3.3±0.1) star on a prograde orbit confined to the Galactic disc. Such stars are rare and may …

Reconstructing the chemical evolution of the Milky Way is crucial for understanding the
formation of stars, planets, and galaxies throughout cosmic time. Different studies associated …