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20042026
most citedThe Gaia-ESO Survey: the Galactic Thick to Thin Disc transition

241 citations · 1.4k across the 23 of their papers we have counts for

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11 papers · 1 filter

astro-ph.SR2024

The Gaia-ESO Survey: Calibrating the lithium-age relation with open clusters and associations. II. Expanded cluster sample and final membership selection

M. L. Gutiérrez Albarrán, D. Montes, H. M. Tabernero +26

The Li abundance observed in pre-main sequence and main sequence late-type stars is strongly age-dependent, but also shows a complex pattern depending on several parameters, such a…

astro-ph.SR2022★ 22 cited

The Gaia-ESO Survey: Lithium measurements and new curves of growth

E. Franciosini, S. Randich, P. de Laverny +37

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 ac…

astro-ph.SR2021★ 26 cited

The Gaia-ESO survey: Lithium abundances in open cluster Red Clump stars

L. Magrini, R. Smiljanic, E. Franciosini +25

It has recently been suggested that all giant stars with mass below 2 suffer an episode of surface lithium enrichment between the tip of the red giant branch (RGB) and…

astro-ph.SR2017★ 150 cited

The Gaia-ESO Survey. Mg-Al anti-correlation in iDR4 globular clusters

E. Pancino, the GES collaboration

We use Gaia-ESO Survey iDR4 data to explore the Mg-Al anti-correlation in globular clusters, that were observed as calibrators, as a demonstration of the quality of Gaia-ESO Survey…

astro-ph.SR2016★ 65 cited

The Gaia-ESO Survey: calibration strategy

E. Pancino, the Gaia-ESO Survey collaboration

The Gaia-ESO survey (GES) is now in its fifth and last year of observations, and has already produced tens of thousands of high-quality spectra of stars in all Milky Way components…

astro-ph.SR2016★ 21 cited

The Gaia-ESO survey: Hydrogen lines in red giants directly trace stellar mass

Maria Bergemann, Aldo Serenelli, Ralph Schoenrich +27

Red giant stars are perhaps the most important type of stars for Galactic and extra-galactic archaeology: they are luminous, occur in all stellar populations, and their surface tem…

astro-ph.SR2016

The Gaia-ESO Survey: Revisiting the Li-rich giant problem

A. R. Casey, G. Ruchti, T. Masseron +48

The discovery of lithium-rich giants contradicts expectations from canonical stellar evolution. Here we report on the serendipitous discovery of 20 Li-rich giants observed during t…

astro-ph.SR2015★ 23 cited

The Gaia-ESO Survey: Detailed Abundances in the Metal-poor Globular Cluster NGC 4372

I. San Roman, C. Muñoz, D. Geisler +28

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…

astro-ph.SR2014★ 73 cited

The Gaia-ESO Survey: the most metal-poor stars in the Galactic bulge

L. Howes, M. Asplund, A. R. Casey +39

We present the first results of the EMBLA survey (Extremely Metal-poor BuLge stars with AAOmega), aimed at finding metal-poor stars in the Milky Way bulge, where the oldest stars s…

astro-ph.SR2014★ 42 cited

The Gaia-ESO Survey: metallicity of the Chamaeleon I star forming region

L. Spina, S. Randich, F. Palla +37

Context. Recent metallicity determinations in young open clusters and star-forming regions suggest that the latter may be characterized by a slightly lower metallicity than the Sun…

astro-ph.SR2009★ 98 cited

The Hamburg/ESO R-process Enhanced Star survey (HERES) IV. Detailed abundance analysis and age dating of the strongly r-process enhanced stars CS 29491-069 and HE 1219-0312

W. Hayek, U. Wiesendahl, N. Christlieb +8

We report on a detailed abundance analysis of two strongly r-process enhanced, very metal-poor stars newly discovered in the HERES project, CS 29491-069 ([Fe/H]=-2.51, [r/Fe]=+1.1)…