activity
20142025
most citedThe Gaia-ESO Survey: Chromospheric Emission, Accretion Properties, and Rotation in Velorum and Chamaeleon I

102 citations · 286 across the 17 of their papers we have counts for

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Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2025★ 5 cited

Stellar Population Astrophysics (SPA) with the TNG: NLTE atmospheric parameters and abundances of giant stars in 33 Open Clusters

M. Dal Ponte, V. D'Orazi, A. Bragaglia +11

Open clusters serve as important tools for accurately studying the chemical evolution of the Milky Way. By combining precise chemical data from high-resolution spectra with informa…

astro-ph.SR2024★ 7 cited

The Gaia-ESO Survey DR5.1 and Gaia DR3 GSP-Spec: a comparative analysis

M. Van der Swaelmen, C. Viscasillas Vazquez, L. Magrini +10

(abridged) The third data release of Gaia, has provided stellar parameters, metallicity [M/H], [α/Fe], individual abundances, broadening parameter from its RVS spectra for about 5.…

astro-ph.SR2024

Chemical signatures of planet engulfment events in Sun-like stars

Lorenzo Spina

The observational evidence that planetary systems can be very different from each other, suggests that their dynamical histories were very diverse, probably as a result of a strong…

astro-ph.SR2023★ 2 cited

Age Determination of LAMOST Red Giant Branch stars based on the Gradient Boosting Decision Tree method

Hai-Feng Wang, Giovanni Carraro, Xin Li +5

In this study we estimate the stellar ages of LAMOST DR8 Red Giant Branch (RGB) stars based on the Gradient Boosting Decision Tree algorithm (GBDT). We used 2,643 RGB stars extract…

astro-ph.SR2015★ 50 cited

The Gaia-ESO Survey: Discovery of a spatially extended low-mass population in the Vela OB2 association

G. G. Sacco, R. D. Jeffries, S. Randich +28

The nearby (distance~350-400 pc), rich Vela OB2 association, includes Velorum, one of the most massive binaries in the solar neighbourhood and an excellent laboratory for inv…

astro-ph.SR2014★ 102 cited

The Gaia-ESO Survey: Chromospheric Emission, Accretion Properties, and Rotation in Velorum and Chamaeleon I

A. Frasca, K. Biazzo, A. C. Lanzafame +33

We use the fundamental parameters delivered by the GES consortium in the first internal data release to select the members of Vel and Cha I among the UVES and GIRAFFE spectrosc…

astro-ph.SR2014★ 42 cited

The Gaia-ESO Survey: metallicity of the Chamaeleon I star forming region

L. Spina, S. Randich, F. Palla +37

Context. Recent metallicity determinations in young open clusters and star-forming regions suggest that the latter may be characterized by a slightly lower metallicity than the Sun…

astro-ph.SR2014★ 36 cited

The Gaia-ESO Survey: the first abundance determination of the pre-main-sequence cluster Gamma Velorum

L. Spina, S. Randich, F. Palla +36

Knowledge of the abundance distribution of star forming regions and young clusters is critical to investigate a variety of issues, from triggered star formation and chemical enrich…