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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Showing astro-ph.GAShow all

28 papers · 1 filter

astro-ph.GA2024★ 2 cited

The accreted Galaxy: An overview of TESS metal-poor accreted stars candidates

Danielle de Brito Silva, Paula Jofré, Clare Worley +2

The Milky Way is a mosaic of stars from different origins. In particular, metal-poor accreted star candidates offer a unique opportunity to better understand the accretion history…

astro-ph.GA2023★ 1 cited

The Gaia-ESO Survey: 3D dynamics of young groups and clusters from GES and Gaia EDR3

Nicholas J. Wright, R. D. Jeffries, R. J. Jackson +9

We present the first large-scale 3D kinematic study of ~2000 spectroscopically-confirmed young stars (<20 Myr) in 18 star clusters and OB associations (hereafter groups) from the c…

astro-ph.GA2021★ 55 cited

The Gaia-ESO Survey: Galactic evolution of lithium from iDR6

D. Romano, L. Magrini, S. Randich +31

We exploit the unique characteristics of a sample of open clusters (OCs) and field stars for which high-precision 7Li abundances and stellar parameters are homogeneously derived by…

astro-ph.GA2020★ 88 cited

The Gaia-ESO survey: the non-universality of the age-chemical-clocks-metallicity relations in the Galactic disc

G. Casali, L. Spina, L. Magrini +36

In the era of large spectroscopic surveys, massive databases of high-quality spectra provide tools to outline a new picture of our Galaxy. In this framework, an important piece of…

astro-ph.GA2017★ 97 cited

The AMBRE project: The thick thin disk and thin thick disk of the Milky Way

M. Hayden, A. Recio-Blanco, P. de Laverny +2

We analyze 494 main sequence turnoff and subgiant stars from the AMBRE:HARPS survey. These stars have accurate astrometric information from \textit{Gaia}/DR1, providing reliable ag…

astro-ph.GA2017★ 35 cited

The Gaia-ESO Survey: Churning through the Milky Way

M. R. Hayden, A. Recio-Blanco, P. de Laverny +29

We attempt to determine the relative fraction of stars that have undergone significant radial migration by studying the orbital properties of metal-rich ([Fe/H]) stars within…