International audience
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2012 (v1)Journal articleUploaded on: December 3, 2022
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April 2017 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
2018 (v1)Publication
Updated stellar parameters of the Gaia FGK benchmark stars (GBS). (1 data file).
Uploaded on: December 4, 2022 -
2024 (v1)Journal article
Context. The third data release of Gaia, has provided stellar parameters, metallicity [M/H], [α/Fe], individual abundances, broadening parameter from its Radial Velocity Spectrograph (RVS) spectra for about 5.6 million objects thanks to the GSP-Spec module, implemented in the Gaia pipeline. The catalogue also publishes the radial velocity of 33...
Uploaded on: January 13, 2025 -
May 2015 (v1)Journal article
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...
Uploaded on: December 4, 2022 -
June 20, 2016 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
2018 (v1)Journal article
Context. There have been conflicting results with respect to the extent that radial migration has played in the evolution of the Galaxy. Additionally, observations of the solar neighborhood have shown evidence of a merger in the past history of the Milky Way that drives enhanced radial migration. Aims. We attempt to determine the relative...
Uploaded on: December 4, 2022 -
July 2015 (v1)Journal article
We present the abundance analysis for a sample of 7 red giant branch stars in the metal-poor globular cluster NGC 4372 based on UVES spectra acquired as part of the Gaia-ESO Survey. This is the first extensive study of this cluster from high-resolution spectroscopy. We derive abundances of O, Na, Mg, Al, Si, Ca, Sc, Ti, Fe, Cr, Ni, Y, Ba, and...
Uploaded on: December 4, 2022 -
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