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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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7 papers · 1 filter

astro-ph.IM2023★ 1 cited

HRMOS White Paper: Science Motivation

Laura Magrini, Thomas Bensby, Anna Brucalassi +52

The High-Resolution Multi-Object Spectrograph (HRMOS) is a facility instrument that we plan to propose for the Very Large Telescope (VLT) of the European Southern Observatory (ESO)…

astro-ph.IM2020★ 186 cited

Atomic data for the Gaia-ESO Survey

Ulrike Heiter, Karin Lind, Maria Bergemann +27

We describe the atomic and molecular data that were used for the abundance analyses of FGK-type stars carried out within the Gaia-ESO Survey. We present an unprecedented effort to…

astro-ph.IM2019★ 8 cited

4MOST Survey Strategy Plan

G. Guiglion, C. Battistini, C. P. M. Bell +30

The current status of and motivation for the 4MOST Survey Strategy, as developed by the Consortium science team, are presented here. Key elements of the strategy are described, suc…

astro-ph.IM2014★ 38 cited

The AMBRE Project: Parameterisation of FGK-type stars from the ESO:HARPS archived spectra

Marco De Pascale, C. Clare Worley, Patrick de Laverny +3

The AMBRE project is a collaboration between the European Southern Observatory (ESO) and the Observatoire de la Cote d'Azur (OCA). It has been established to determine the stellar…

astro-ph.IM2014★ 41 cited

Empirical classification of VLT/Giraffe stellar spectra in the wavelength range 6440-6810 A in the gamma Vel cluster, and calibration of spectral indices

F. Damiani, L. Prisinzano, G. Micela +23

We study spectral diagnostics available from optical spectra with R=17000 obtained with the VLT/Giraffe HR15n setup, using observations from the Gaia-ESO Survey, on the gamma Vel y…

astro-ph.IM2014★ 93 cited

The Gaia-ESO Survey: processing of the FLAMES-UVES spectra

G. G. Sacco, L. Morbidelli, E. Franciosini +49

The Gaia-ESO Survey is a large public spectroscopic survey that aims to derive radial velocities and fundamental parameters of about 10^5 Milky Way stars in the field and in cluste…