activity
20032026
most cited4MOST: Project overview and information for the First Call for Proposals

311 citations · 6.6k across the 137 of their papers we have counts for

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Showing 2018Show all

6 papers · 1 filter

astro-ph.SR2018★ 20 cited

Systematic investigation of chemical abundances derived using IR spectra obtained with GIANO

E. Caffau, P. Bonifacio, E. Oliva +10

Detailed chemical abundances of Galactic stars are needed in order to improve our knowledge of the formation and evolution of our galaxy, the Milky Way. We took advantage of the GI…

astro-ph.SR2018★ 30 cited

Debris disks with multiple absorption features in metallic lines: circumstellar or interstellar origin?

D. Iglesias, A. Bayo, J. Olofsson +8

Debris disks are second generation dusty disks thought to be devoid of gas. However, this idea has been challenged in the last years by gas detections in some systems. We compiled…

astro-ph.GA2018★ 54 cited

The Gaia-ESO Survey: the origin and evolution of s-process elements

L. Magrini, L. Spina, S. Randich +45

Several works have found an increase of the abundances of the s-process neutron-capture elements in the youngest Galactic stellar populations, giving important constraints to stell…

astro-ph.SR2018★ 42 cited

The Gaia-ESO Survey: properties of newly discovered Li-rich giants

R. Smiljanic, E. Franciosini, A. Bragaglia +41

We report 20 new lithium-rich giants discovered within the Gaia-ESO Survey, including the first Li-rich giant with evolutionary stage confirmed by CoRoT data. Atmospheric parameter…

astro-ph.SR2018★ 66 cited

The Gaia-ESO survey: impact of extra-mixing on C- and N-abundances of giant stars

N. Lagarde, C. Reylé, A. C. Robin +30

The GES survey using FLAMES at the VLT has obtained high-resolution UVES spectra for a large number of giant stars, allowing a determination of the abundances of the key chemical e…

astro-ph.SR2018★ 17 cited

Investigation of a sample of carbon-enhanced metal-poor stars observed with FORS and GMOS

E. Caffau, A. J. Gallagher, P. Bonifacio +5

Carbon-enhanced metal-poor (CEMP) stars represent a sizeable fraction of all known metal-poor stars in the Galaxy. Their formation and composition remains a significant topic of in…