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20142023
most citedThe Gaia-ESO Survey: the Galactic Thick to Thin Disc transition

241 citations · 1.6k across the 18 of their papers we have counts for

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12 papers · 1 filter

astro-ph.SR202376 cited

The Gaia-ESO Survey: Empirical estimates of stellar ages from lithium equivalent widths (EAGLES)

R. D. Jeffries, R. J. Jackson, Nicholas J. Wright +17

We present an empirical model of age-dependent photospheric lithium depletion, calibrated using a large, homogeneously-analysed sample of 6200 stars in 52 open clusters, with ages…

astro-ph.SR202313 cited

Gaia-ESO Survey: massive stars in the Carina Nebula. A new census of OB stars

S. R. Berlanas, J. Maíz Apellániz, A. Herrero +16

The Gaia-ESO survey sample of massive OB stars in the Carina Nebula consists of 234 stars. The addition of brighter sources from the Galactic O-Star Spectroscopic Survey and additi…

astro-ph.SR2022133 cited

The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products

G. Gilmore, S. Randich, C. C. Worley +165

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

astro-ph.SR202211 cited

The Gaia-ESO survey: A spectroscopic study of the young open cluster NGC 3293

T. Morel, A. Blazère, T. Semaan +24

We present a spectroscopic analysis of the GIRAFFE and UVES data collected by the Gaia-ESO survey for the young open cluster NGC 3293. Archive spectra from the same instruments obt…

astro-ph.SR202132 cited

Gaia-ESO Survey: Role of magnetic activity and starspots on pre-main sequence lithium evolution

E. Franciosini, E. Tognelli, S. Degl'Innocenti +24

Pre-main sequence models with inflated radii are needed to simultaneously reproduce the colour-magnitude diagram and the lithium depletion pattern in young open clusters. We tested…

astro-ph.SR201673 cited

The Gaia-ESO Survey: Lithium depletion in the Gamma Velorum cluster and inflated radii in low-mass pre-main-sequence stars

R. D. Jeffries, R. J. Jackson, E. Franciosini +25

We show that non-magnetic models for the evolution of pre-main-sequence (PMS) stars *cannot* simultaneously describe the colour-magnitude diagram (CMD) and the pattern of lithium d…