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20022026
most citedGaia FGK Benchmark Stars - Metallicity

314 citations · 9.2k across the 198 of their papers we have counts for

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Showing 2014Show all

16 papers · 1 filter

astro-ph.SR2014★ 22 cited

Discovery of true, likely and possible symbiotic stars in the dwarf spheroidal NGC 205

Denise R. Gonçalves, Laura Magrini, Ignacio G. de la Rosa +1

In this paper we discuss the photometric and spectroscopic observations of newly discovered (symbiotic) systems in the dwarf spheroidal galaxy NGC 205. The Gemini Multi-Object Spec…

astro-ph.SR2014★ 61 cited

The Gaia-ESO Survey: CNO abundances in the open clusters Trumpler 20, NGC 4815, and NGC 6705

G. Tautvaišienė, A. Drazdauskas, Š. Mikolaitis +30

Aim of this work is to determine C, N, and O abundances in stars of Galactic open clusters of the Gaia-ESO survey and to compare the observed abundances with those predicted by cur…

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★ 227 cited

Gaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars

R. Smiljanic, A. J. Korn, M. Bergemann +99

The Gaia-ESO Survey is obtaining high-quality spectroscopic data for about 10^5 stars using FLAMES at the VLT. UVES high-resolution spectra are being collected for about 5000 FGK-t…

astro-ph.GA2014★ 129 cited

The Gaia-ESO Survey: the chemical structure of the Galactic discs from the first internal data release

Š. Mikolaitis, V. Hill, A. Recio-Blanco +31

Most high-resolution spectroscopic studies of the Galactic discs were mostly confined to objects in the solar vicinity. Here we aim at enlarging the volume in which individual chem…

astro-ph.GA2014★ 147 cited

The Gaia-ESO Survey: metallicity and kinematic trends in the Milky Way bulge

A. Rojas-Arriagada, A. Recio-Blanco, V. Hill +30

(Abridged) We analyzed the stellar parameters and radial velocities of ~1200 stars in five bulge fields as determined from the Gaia-ESO survey data (iDR1). We use VISTA Variables i…