Context. Large spectroscopic surveys have in recent years enabled computing three-dimensional interstellar extinction maps thanks to the accurate stellar atmospheric parameters and line-of-sight distances these surveys provide. Interstellar extinction maps are complementary to 3D maps extracted from photometry and allow a more thorough studying...
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May 2015 (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 -
April 2018 (v1)Journal article
International audience
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September 2018 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
July 2021 (v1)Journal article
Aims. We aim to constrain the mixing processes in low-mass stars by investigating the behaviour of the Li surface abundance after the main sequence. We take advantage of the data from the sixth internal data release of Gaia -ESO, IDR 6, and from the Gaia Early Data Release 3, EDR 3s. Methods. We selected a sample of main-sequence, sub-giant,...
Uploaded on: December 3, 2022 -
September 2018 (v1)Journal article
International audience
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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 -
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 -
May 2017 (v1)Journal article
Milky Way open clusters are very diverse in terms of age, chemical composition, and kinematic properties. Intermediate-age and old open clusters are less common, and it is even harder to find them inside the solar Galactocentric radius, due to the high mortality rate and strong extinction inside this region. NGC 6802 is one of the inner disk...
Uploaded on: December 4, 2022 -
September 2019 (v1)Journal article
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Uploaded on: December 3, 2022 -
August 2015 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
May 2014 (v1)Journal article
International audience
Uploaded on: December 4, 2022