activity
20002022
most citedThe Gaia-ESO Public Spectroscopic Survey: Implementation, data products, open cluster survey, science, and legacy

188 citations · 253 across the 9 of their papers we have counts for

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8 papers · 1 filter

astro-ph2008

New high resolution synthetic stellar libraries for the Gaia Mission

R. Sordo, A. Vallenari, J. C. Bouret +12

High resolution synthetic stellar libraries are of fundamental importance for the preparation of the Gaia Mission. We present new sets of spectral stellar libraries covering two sp…

astro-ph2005

The Carina dSph galaxy: where is the edge?

G. Bono, M. Monelli, A. R. Walker +13

Recent cosmological N-body simulations suggest that current empirical estimates of tidal radii in dSphs might be underestimated by at least one order of magnitude. To constrain the…

astro-ph2005

Spectroscopic Survey of the Galaxy with Gaia II. The expected science yield from the Radial Velocity Spectrometer

M. I. Wilkinson, A. Vallenari, C. Turon +21

The Gaia mission is designed as a Galaxy explorer, and will measure simultaneously, in a survey mode, the five or six phase space parameters of all stars brighter than 20th magnitu…

astro-ph2004

Spectroscopic survey of the Galaxy with Gaia I. Design and performance of the Radial Velocity Spectrometer

D. Katz, U. Munari, M. Cropper +22

The definition and optimisation studies for the Gaia satellite spectrograph, the Radial Velocity Spectrometer (RVS), converged in late 2002 with the adoption of the instrument base…

astro-ph2004

The angular size of dwarf stars and subgiants - Surface brightness relations calibrated by interferometry

P. Kervella, F. Thevenin, E. Di Folco +1

The availability of a number of new interferometric measurements of Main Sequence and subgiant stars makes it possible to calibrate the surface brightness relations of these stars…

astro-ph2003

Modeling of Alpha Cen and Procyon using VLTI observations

P. Kervella, F. Thevenin, P. Morel +4

We present a novel approach to model the nearby stars Alpha Cen A & B and Procyon A using asteroseismic and interferometric constraints. Using the VINCI instrument installed at the…