International audience
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February 2018 (v1)Journal articleUploaded on: December 4, 2022
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July 2017 (v1)Journal article
Aims: We present the first extensive spectroscopic study of the global population in star clusters Trumpler 16, Trumpler 14, and Collinder 232 in the Carina nebula, using data from the Gaia-ESO Survey, down to solar-mass stars. Methods: In addition to the standard homogeneous survey data reduction, a special processing was applied here because...
Uploaded on: December 4, 2022 -
July 2016 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
September 2018 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
January 1, 2018 (v1)Journal article
The typical methodology for comparing simulated galaxies with observational surveys is usually to apply a spatial selection to the simulation to mimic the region of interest covered by a comparable observational survey sample. In this work, we compare this approach with a more sophisticated post-processing in which the observational...
Uploaded on: December 4, 2022 -
2022 (v1)Journal article
Context. The Gaia-ESO Survey (GES) is a large public spectroscopic survey that was carried out using the multi-object FLAMES spectrograph at the Very Large Telescope. The survey provides accurate radial velocities, stellar parameters, and elemental abundances for ~115 000 stars in all Milky Way components. Aims: In this paper, we describe the...
Uploaded on: April 20, 2023