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 …

The ensemble of chemical element abundance measurements for stars, along with precision
distances and orbit properties, provides high-dimensional data to study the evolution of the …

Gaia is a cornerstone mission in the science programme of the European Space Agency
(ESA). The spacecraft construction was approved in 2006, following a study in which the …

Context. The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to
obtain astrophysical parameters and elemental abundances for 100 000 stars, including …

Multiple codes are available to derive atmospheric parameters and individual chemical
abundances from high-resolution spectra of AFGKM stars. Almost all spectroscopists have …

Though distant and seemingly unreachable, planets outside the Solar System, or
exoplanets, have captivated the imagination of scientists and stargazers alike. With more …

Gaia is a cornerstone mission in the science programme of the EuropeanSpace Agency
(ESA). The spacecraft construction was approved in 2006, following a study in which the …

Accurately measuring stellar parameters is a key goal to increase our understanding of the
observable Universe. However, current methods are limited by many factors, in particular …

Data from the SDSS-IV/Apache Point Observatory Galactic Evolution Experiment (APOGEE-
2) have been released as part of SDSS Data Releases 13 (DR13) and 14 (DR14). These …

The bibliographical compilation of stellar atmospheric parameters (T eff, log g,[Fe/H]) relying
on high-resolution, high signal-to-noise spectroscopy started in the eighties with the so …