activity
20152025
most cited4MOST: Project overview and information for the First Call for Proposals

311 citations · 2k across the 34 of their papers we have counts for

collaborators
Showing 2017Show all

15 papers · 1 filter

astro-ph.GA2017★ 35 cited

The Gaia-ESO Survey: Churning through the Milky Way

M. R. Hayden, A. Recio-Blanco, P. de Laverny +29

We attempt to determine the relative fraction of stars that have undergone significant radial migration by studying the orbital properties of metal-rich ([Fe/H]) stars within…

astro-ph.GA2017

The Gaia -ESO Survey: Lithium enrichment histories of the Galactic thick and thin disc

Xiaoting. Fu, D. Romano, A. Bragaglia +32

Lithium abundance in most of the warm metal-poor main sequence stars shows a constant plateau (A(Li)~2.2 dex) and then the upper envelope of the lithium vs. metallicity distributio…

astro-ph.SR2017★ 2 cited

Gaia FGK benchmark stars: a bridge between spectroscopic surveys

Paula Jofre, Ulrike Heiter, Sven Buder

The Gaia benchmark stars (GBS) are very bright stars of different late spectral types, luminosities and metallicities. They are well-known in the Galactic archaeology community bec…

astro-ph.SR2017★ 98 cited

Binary stars in the Galactic thick disc

Robert G. Izzard, Holly Preece, Paula Jofre +3

The combination of asteroseismologically-measured masses with abundances from detailed analyses of stellar atmospheres challenges our fundamental knowledge of stars and our ability…

astro-ph.SR2017★ 55 cited

The Gaia-ESO Survey and CSI 2264: Substructures, disks, and sequential star formation in the young open cluster NGC 2264

L. Venuti, L. Prisinzano, G. G. Sacco +21

We explore the structure and star formation history of the open cluster NGC 2264 (~3 Myr). We combined spectroscopic data from the Gaia-ESO Survey (GES) with multi-wavelength photo…

astro-ph.GA2017★ 11 cited

The Gaia-ESO Survey: Matching Chemo-Dynamical Simulations to Observations of the Milky Way

B. B. Thompson, C. G. Few, M. Bergemann +39

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 covere…