000006547 001__ 6547
000006547 005__ 20240109102415.0
000006547 0247_ $$2DOI$$a10.1051/0004-6361/202345910
000006547 037__ $$aSCART-2024-0004
000006547 100__ $$aHourihane, A.
000006547 245__ $$aThe Gaia-ESO Survey: Homogenisation of stellar parameters and elemental abundances 
000006547 260__ $$c2023
000006547 520__ $$aThe Gaia-ESO Survey is a public spectroscopic survey that targeted ≳105 stars covering all major components of the Milky Way from the end of 2011 to 2018, delivering its final public release in May 2022. Unlike other spectroscopic surveys, Gaia-ESO is the only survey that observed stars across all spectral types with dedicated, specialised analyses: from O (Teff ~ 30 000-52 000 K) all the way to K-M (≳3500 K). The physics throughout these stellar regimes varies significantly, which has previously prohibited any detailed comparisons between stars of significantly different types. In the final data release (internal data release 6) of the Gaia-ESO Survey, we provide the final database containing a large number of products, such as radial velocities, stellar parameters and elemental abundances, rotational velocity, and also, for example, activity and accretion indicators in young stars and membership probability in star clusters for more than 114 000 stars. The spectral analysis is coordinated by a number of working groups (WGs) within the survey, each specialised in one or more of the various stellar samples. Common targets are analysed across WGs to allow for comparisons (and calibrations) amongst instrumental setups and spectral types. Here we describe the procedures employed to ensure all survey results are placed on a common scale in order to arrive at a single set of recommended results for use by all survey collaborators. We also present some general quality and consistency checks performed on the entirety of the survey results. 
000006547 594__ $$aNO
000006547 6531_ $$astars: abundances
000006547 6531_ $$astars: fundamental parameters
000006547 6531_ $$aGalaxy: stellar content
000006547 6531_ $$amethods: data analysis
000006547 6531_ $$amethods: statistical
000006547 6531_ $$atechniques: spectroscopic
000006547 6531_ $$aAstrophysics - Solar and Stellar Astrophysics
000006547 6531_ $$aAstrophysics - Astrophysics of Galaxies 
000006547 700__ $$aFrançois, P.
000006547 700__ $$aWorley, C. C.
000006547 700__ $$aMagrini, L.
000006547 700__ $$aGonneau, A.
000006547 700__ $$aCasey, A. R.
000006547 700__ $$aGilmore, G.
000006547 700__ $$aRandich, S.
000006547 700__ $$aSacco, G. G.
000006547 700__ $$aRecio-Blanco, A.
000006547 700__ $$aKorn, A. J.
000006547 700__ $$aAllende Prieto, C.
000006547 700__ $$aSmiljanic, R.
000006547 700__ $$aBlomme, R.
000006547 700__ $$aBragaglia, A.
000006547 700__ $$aWalton, N. A.
000006547 700__ $$aVan Eck, S.
000006547 700__ $$aBensby, T.
000006547 700__ $$aLanzafame, A.
000006547 700__ $$aFrasca, A.
000006547 700__ $$aFranciosini, E.
000006547 700__ $$aDamiani, F.
000006547 700__ $$aLind, K.
000006547 700__ $$aBergemann, M.
000006547 700__ $$aBonifacio, P.
000006547 700__ $$aHill, V.
000006547 700__ $$aLobel, A.
000006547 700__ $$aMontes, D.
000006547 700__ $$aFeuillet, D. K.
000006547 700__ $$aTautvaišienė, G.
000006547 700__ $$aGuiglion, G.
000006547 700__ $$aTabernero, H. M.
000006547 700__ $$aGonzález Hernández, J. I.
000006547 700__ $$aGebran, M.
000006547 700__ $$aVan der Swaelmen, M.
000006547 700__ $$aMikolaitis, Š.
000006547 700__ $$aDaflon, S.
000006547 700__ $$aMerle, T.
000006547 700__ $$aMorel, T.
000006547 700__ $$aLewis, J. R.
000006547 700__ $$aGonzález Solares, E. A.
000006547 700__ $$aMurphy, D. N. A.
000006547 700__ $$aJeffries, R. D.
000006547 700__ $$aJackson, R. J.
000006547 700__ $$aFeltzing, S.
000006547 700__ $$aPrusti, T.
000006547 700__ $$aCarraro, G.
000006547 700__ $$aBiazzo, K.
000006547 700__ $$aPrisinzano, L.
000006547 700__ $$aJofré, P.
000006547 700__ $$aZaggia, S.
000006547 700__ $$aDrazdauskas, A.
000006547 700__ $$aStonkuté, E.
000006547 700__ $$aMarfil, E.
000006547 700__ $$aJiménez-Esteban, F.
000006547 700__ $$aMahy, L.
000006547 700__ $$aGutiérrez Albarrán, M. L.
000006547 700__ $$aBerlanas, S. R.
000006547 700__ $$aSantos, W.
000006547 700__ $$aMorbidelli, L.
000006547 700__ $$aSpina, L.
000006547 700__ $$aMinkevičiūtė, R.
000006547 773__ $$cA129 (33pp)$$pAstronomy & Astrophysics$$v676$$y2023
000006547 8560_ $$fronny.blomme@ksb-orb.be
000006547 85642 $$ahttps://arxiv.org/abs/2304.07720
000006547 905__ $$apublished in
000006547 980__ $$aREFERD