The Gaia-ESO survey (GES) is now in its fifth and last year of observations and has produced tens of thousands of high-quality spectra of stars in all Milky Way...
The Gaia-ESO survey: Discovery of a spatially extended low-mass population in the Vela OB2 association
The nearby (distance ~ 350-400 pc), rich Vela OB2 association, includes γ2 Velorum, one of the most massive binaries in the solar neighbourhood and an excellent...
The Gaia-ESO Survey: Empirical determination of the precision of stellar radial velocities and projected rotation velocities
Context. The Gaia-ESO Survey (GES) is a large public spectroscopic survey at the European Southern Observatory Very Large Telescope. Aims: A key aim is to...
The Gaia-ESO Survey: Homogenisation of stellar parameters and elemental abundances
The Gaia-ESO Survey is a public spectroscopic survey that targeted ≳10 5 stars covering all major components of the Milky Way from the end of 2011 to 2018...
The Gaia-ESO Survey: impact of extra mixing on C and N abundances of giant stars
Context. The Gaia-ESO Public Spectroscopic Survey using FLAMES at the VLT has obtained high-resolution UVES spectra for a large number of giant stars, allowing...
The Gaia-ESO Survey: Kinematics of seven Galactic globular clusters
The Gaia-ESO survey is a large public spectroscopic survey aimed at investigating the origin and formation history of our Galaxy by collecting spectroscopy of...
The Gaia-ESO Survey: Low-α element stars in the Galactic bulge
We take advantage of the Gaia-ESO Survey iDR4 bulge data to search for abundance anomalies that could shed light on the composite nature of the Milky Way bulge...
The Gaia-ESO Survey: Metallicity of the Chamaeleon I star-forming region
Context. Recent metallicity determinations in young open clusters and star-forming regions suggest that the latter may be characterized by a slightly lower...