activity
20142024
most citedThe Gaia-ESO Survey. Mg-Al anti-correlation in iDR4 globular clusters

150 citations · 563 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2024★ 11 cited

Ariel stellar characterisation II. Chemical abundances of carbon, nitrogen, and oxygen for 181 planet-host FGK dwarf stars

R. da Silva, C. Danielski, E. Delgado Mena +12

One of the ultimate goals of the ESA Ariel space mission is to shed light on the formation pathways and evolution of planetary systems in the Solar neighbourhood. Such an endeavour…

astro-ph.EP2020★ 123 cited

A remnant planetary core in the hot-Neptune desert

David J. Armstrong, Théo A. Lopez, Vardan Adibekyan +91

The interiors of giant planets remain poorly understood. Even for the planets in the Solar System, difficulties in observation lead to large uncertainties in the properties of plan…

astro-ph.SR2017★ 150 cited

The Gaia-ESO Survey. Mg-Al anti-correlation in iDR4 globular clusters

E. Pancino, the GES collaboration

We use Gaia-ESO Survey iDR4 data to explore the Mg-Al anti-correlation in globular clusters, that were observed as calibrators, as a demonstration of the quality of Gaia-ESO Survey…

astro-ph.GA2017★ 26 cited

The -ESO Survey: the inner disk intermediate-age open cluster NGC 6802

B. Tang, D. Geisler, E. Friel +43

Milky Way open clusters are very diverse in terms of age, chemical composition, and kinematic properties. Intermediate-age and old open clusters are less common, and it is even har…

astro-ph.SR2016★ 31 cited

The Gaia-ESO Survey: the inner disk, intermediate-age open cluster Trumpler 23

J. C. Overbeek, E. D. Friel, P. Donati +33

Context: Trumpler 23 is a moderately populated, intermediate-age open cluster within the solar circle at a Rgc ~6 kpc. It is in a crowded field very close to the Galactic plane and…

astro-ph.SR2016★ 65 cited

The Gaia-ESO Survey: calibration strategy

E. Pancino, the Gaia-ESO Survey collaboration

The Gaia-ESO survey (GES) is now in its fifth and last year of observations, and has already produced tens of thousands of high-quality spectra of stars in all Milky Way components…