activity
20032026
most citedGaia-ESO Survey: The analysis of high-resolution UVES spectra of FGK-type stars

227 citations · 4.3k across the 103 of their papers we have counts for

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Showing 2021Show all

8 papers · 1 filter

astro-ph.SR2021★ 43 cited

The Gaia-ESO Survey: Target selection of open cluster stars

A. Bragaglia, E. Alfaro, E. Flaccomio +36

The Gaia-ESO Survey (GES) is a public, high-resolution spectroscopic survey with FLAMES@VLT. GES targeted in particular a large sample of open clusters (OCs) of all ages. The diffe…

astro-ph.SR2021★ 32 cited

Gaia-ESO Survey: Role of magnetic activity and starspots on pre-main sequence lithium evolution

E. Franciosini, E. Tognelli, S. Degl'Innocenti +24

Pre-main sequence models with inflated radii are needed to simultaneously reproduce the colour-magnitude diagram and the lithium depletion pattern in young open clusters. We tested…

astro-ph.SR2021★ 59 cited

The Gaia-ESO Survey: Membership probabilities for stars in 63 open and 7 globular clusters from 3D kinematics

R. J. Jackson, R. D. Jeffries, N. J. Wright +26

Spectroscopy from the final internal data release of the Gaia-ESO Survey (GES) has been combined with Gaia EDR3 to assign membership probabilities to targets observed towards 63 Ga…

astro-ph.EP2021★ 68 cited

The PLATO field selection process I. Identification and content of the long-pointing fields

V. Nascimbeni, G. Piotto, A. Börner +26

PLATO (PLAnetary Transits and Oscillations of stars) is an ESA M-class satellite planned for launch by end 2026 and dedicated to the wide-field search of transiting planets around…

astro-ph.EP2021★ 77 cited

The all-sky PLATO input catalogue

M. Montalto, G. Piotto, P. M. Marrese +29

Context. The ESA PLAnetary Transits and Oscillations of stars (PLATO) mission will search for terrestrial planets in the habitable zone of solar-type stars. Because of telemetry li…

astro-ph.SR2021★ 54 cited

The Gaia-ESO survey: Mixing processes in low-mass stars traced by lithium abundance in cluster and field stars

L. Magrini, N. Lagarde, C. Charbonnel +42

We aim to constrain the mixing processes in low-mass stars by investigating the behaviour of the Li surface abundance after the main sequence. We take advantage of the data from th…