activity
20082025
most citedInclination- and dust-corrected galaxy parameters: Bulge-to-disc ratios and size-luminosity relations

325 citations · 4.6k across the 69 of their papers we have counts for

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33 papers · 1 filter

astro-ph.SR2025

Magnesium Isotopic Detection in Cool Stars: Tracing Nucleosynthetic Signatures from MgH Features

Quin Aicken Davies, C. Clare Worley

Magnesium (Mg) isotopic ratios offer valuable insights into stellar nucleosynthesis and Galactic chemical evolution, particularly in distinguishing contributions from supernovae an…

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.SR2023

Gaia FGK Benchmark Stars: fundamental Teff and log g of the third version

Caroline Soubiran, Orlagh Creevey, Nadege Lagarde +8

Context. Large spectroscopic surveys devoted to the study of the Milky Way, including Gaia, use automated pipelines to massively determine the atmospheric parameters of millions of…

astro-ph.SR2022★ 22 cited

The Gaia-ESO Survey: Lithium measurements and new curves of growth

E. Franciosini, S. Randich, P. de Laverny +37

The Gaia-ESO Survey (GES) is a large public spectroscopic survey that was carried out using the multi-object FLAMES spectrograph at the Very Large Telescope. The survey provides ac…

astro-ph.SR2021★ 26 cited

The Gaia-ESO survey: Lithium abundances in open cluster Red Clump stars

L. Magrini, R. Smiljanic, E. Franciosini +25

It has recently been suggested that all giant stars with mass below 2 suffer an episode of surface lithium enrichment between the tip of the red giant branch (RGB) and…

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…