output
19952026
most citedThe Gaia mission

7.1k citations

Showing 2014 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2014★ 11 cited

The Gaia-ESO Survey: α-abundances of metal-poor stars

R. Jackson-Jones, P. Jofré, K. Hawkins +21

We performed a detailed study of the ratio of low-α to high-α stars in the Galactic halo as observed by the Gaia-ESO Survey. Using a sample of 381 metal-poor stars from the second…

astro-ph.GA2014★ 18 cited

Dwarf Irregular Galaxy Leo A. Suprime-Cam Wide-Field Stellar Photometry

R. Stonkutė, N. Arimoto, T. Hasegawa +3

We have surveyed a complete extent of Leo A - an apparently isolated gas-rich low-mass dwarf irregular galaxy in the Local Group. The , , and passband CCD images (typical…

astro-ph.GA2014

Structural Parameters of Star Clusters: Stochastic Effects

D. Narbutis, R. Stonkutė, P. de Meulenaer +2

Stochasticity of bright stars introduces uncertainty and bias into derived structural parameters of star clusters. We have simulated a grid of cluster -band images, observed wit…

astro-ph.GA2014★ 2 cited

Deriving structural parameters of semi-resolved star clusters. FitClust: a program for crowded fields

D. Narbutis, D. Semionov, R. Stonkutė +4

Context. An automatic tool to derive structural parameters of semi-resolved star clusters located in crowded stellar fields in nearby galaxies is needed for homogeneous processing…

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★ 204 cited

The Gaia-ESO Survey: radial metallicity gradients and age-metallicity relation of stars in the Milky Way disk

M. Bergemann, G. Ruchti, A. Serenelli +42

We study the relationship between age, metallicity, and alpha-enhancement of FGK stars in the Galactic disk. The results are based upon the analysis of high-resolution UVES spectra…