000006051 001__ 6051
000006051 005__ 20230113160015.0
000006051 0247_ $$2DOI$$a10.1051/0004-6361/202243134
000006051 037__ $$aSCART-2023-0012
000006051 100__ $$aGilmore, G.
000006051 245__ $$aThe Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products
000006051 260__ $$c2022
000006051 520__ $$aContext. The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to obtain astrophysical parameters and elemental abundances for 100 000 stars, including large representative samples of the stellar populations in the Galaxy, and a well-defined sample of 60 (plus 20 archive) open clusters. We provide internally consistent results calibrated on benchmark stars and star clusters, extending across a very wide range of abundances and ages. This provides a legacy data set of intrinsic value, and equally a large wide-ranging dataset that is of value for the homogenisation of other and future stellar surveys and Gaia's astrophysical parameters. Aims. This article provides an overview of the survey methodology, the scientific aims, and the implementation, including a description of the data processing for the GIRAFFE spectra. A companion paper introduces the survey results. Methods. Gaia-ESO aspires to quantify both random and systematic contributions to measurement uncertainties. Thus, all available spectroscopic analysis techniques are utilised, each spectrum being analysed by up to several different analysis pipelines, with considerable effort being made to homogenise and calibrate the resulting parameters. We describe here the sequence of activities up to delivery of processed data products to the ESO Science Archive Facility for open use. Results. The Gaia-ESO Survey obtained 202 000 spectra of 115 000 stars using 340 allocated VLT nights between December 2011 and January 2018 from GIRAFFE and UVES. Conclusions. The full consistently reduced final data set of spectra was released through the ESO Science Archive Facility in late 2020, with the full astrophysical parameters sets following in 2022. A companion article reviews the survey implementation, scientific highlights, the open cluster survey, and data products.
000006051 536__ $$aGaia PRODEX/$$cGaia PRODEX/$$fGaia PRODEX
000006051 594__ $$aNO
000006051 6531_ $$aGalaxy: stellar content
000006051 6531_ $$aGalaxy: kinematics and dynamics
000006051 6531_ $$astars: abundances
000006051 6531_ $$amethods: observational
000006051 6531_ $$atechniques: spectroscopic
000006051 6531_ $$asurveys
000006051 700__ $$aRandich, S.
000006051 700__ $$aWorley, C. C.
000006051 700__ $$aHourihane, A.
000006051 700__ $$aGonneau, A.
000006051 700__ $$aSacco, G. G.
000006051 700__ $$aLewis, J. R.
000006051 700__ $$aMagrini, L.
000006051 700__ $$aFrançois, P.
000006051 700__ $$aJeffries, R. D.
000006051 700__ $$aKoposov, S. E.
000006051 700__ $$aBragaglia, A.
000006051 700__ $$aAlfaro, E. J.
000006051 700__ $$aAllende Prieto, C.
000006051 700__ $$aBlomme, R.
000006051 700__ $$aKorn, A. J.
000006051 700__ $$aLanzafame, A. C.
000006051 700__ $$aPancino, E.
000006051 700__ $$aRecio-Blanco, A.
000006051 700__ $$aSmiljanic, R.
000006051 700__ $$aVan Eck, S.
000006051 700__ $$aZwitter, T.
000006051 700__ $$aBensby, T.
000006051 700__ $$aFlaccomio, E.
000006051 700__ $$aIrwin, M. J.
000006051 700__ $$aFranciosini, E.
000006051 700__ $$aMorbidelli, L.
000006051 700__ $$aDamiani, F.
000006051 700__ $$aBonito, R.
000006051 700__ $$aFriel, E. D.
000006051 700__ $$aVink, J. S.
000006051 700__ $$aPrisinzano, L.
000006051 700__ $$aAbbas, U.
000006051 700__ $$aHatzidimitriou, D.
000006051 700__ $$aHeld, E. V.
000006051 700__ $$aJordi, C.
000006051 700__ $$aPaunzen, E.
000006051 700__ $$aSpagna, A.
000006051 700__ $$aJackson, R. J.
000006051 700__ $$aMaíz Apellániz, J.
000006051 700__ $$aAsplund, M.
000006051 700__ $$aBonifacio, P.
000006051 700__ $$aFeltzing, S.
000006051 700__ $$aBinney, J.
000006051 700__ $$aDrew, J.
000006051 700__ $$aFerguson, A. M. N.
000006051 700__ $$aMicela, G.
000006051 700__ $$aNegueruela, I.
000006051 700__ $$aPrusti, T.
000006051 700__ $$aRix, H. -W.
000006051 700__ $$aVallenari, A.
000006051 700__ $$aBergemann, M.
000006051 700__ $$aCasey, A. R.
000006051 700__ $$ade Laverny, P.
000006051 700__ $$aFrasca, A.
000006051 700__ $$aHill, V.
000006051 700__ $$aLind, K.
000006051 700__ $$aSbordone, L.
000006051 700__ $$aSousa, S. G.
000006051 700__ $$aAdibekyan, V.
000006051 700__ $$aCaffau, E.
000006051 700__ $$aDaflon, S.
000006051 700__ $$aFeuillet, D. K.
000006051 700__ $$aGebran, M.
000006051 700__ $$aGonzalez Hernandez, J. I.
000006051 700__ $$aGuiglion, G.
000006051 700__ $$aHerrero, A.
000006051 700__ $$aLobel, A.
000006051 700__ $$aMerle, T.
000006051 700__ $$aMikolaitis, Š.
000006051 700__ $$aMontes, D.
000006051 700__ $$aMorel, T.
000006051 700__ $$aRuchti, G.
000006051 700__ $$aSoubiran, C.
000006051 700__ $$aTabernero, H. M.
000006051 700__ $$aTautvaišienė, G.
000006051 700__ $$aTraven, G.
000006051 700__ $$aValentini, M.
000006051 700__ $$aVan der Swaelmen, M.
000006051 700__ $$aVillanova, S.
000006051 700__ $$aViscasillas Vázquez, C.
000006051 700__ $$aBayo, A.
000006051 700__ $$aBiazzo, K.
000006051 700__ $$aCarraro, G.
000006051 700__ $$aEdvardsson, B.
000006051 700__ $$aHeiter, U.
000006051 700__ $$aJofré, P.
000006051 700__ $$aMarconi, G.
000006051 700__ $$aMartayan, C.
000006051 700__ $$aMasseron, T.
000006051 700__ $$aMonaco, L.
000006051 700__ $$aWalton, N. A.
000006051 700__ $$aZaggia, S.
000006051 700__ $$aAguirre Børsen-Koch, V.
000006051 700__ $$aAlves, J.
000006051 700__ $$aBalaguer-Nunez, L.
000006051 700__ $$aBarklem, P. S.
000006051 700__ $$aBarrado, D.
000006051 700__ $$aBellazzini, M.
000006051 700__ $$aBerlanas, S. R.
000006051 700__ $$aBinks, A. S.
000006051 700__ $$aBressan, A.
000006051 700__ $$aCapuzzo-Dolcetta, R.
000006051 700__ $$aCasagrande, L.
000006051 700__ $$aCasamiquela, L.
000006051 700__ $$aCollins, R. S.
000006051 700__ $$aD'Orazi, V.
000006051 700__ $$aDantas, M. L. L.
000006051 700__ $$aDebattista, V. P.
000006051 700__ $$aDelgado-Mena, E.
000006051 700__ $$aDi Marcantonio, P.
000006051 700__ $$aDrazdauskas, A.
000006051 700__ $$aEvans, N. W.
000006051 700__ $$aFamaey, B.
000006051 700__ $$aFranchini, M.
000006051 700__ $$aFrémat, Y.
000006051 700__ $$aFu, X.
000006051 700__ $$aGeisler, D.
000006051 700__ $$aGerhard, O.
000006051 700__ $$aGonzález Solares, E. A.
000006051 700__ $$aGrebel, E. K.
000006051 700__ $$aGutiérrez Albarrán, M. L.
000006051 700__ $$aJiménez-Esteban, F.
000006051 700__ $$aJönsson, H.
000006051 700__ $$aKhachaturyants, T.
000006051 700__ $$aKordopatis, G.
000006051 700__ $$aKos, J.
000006051 700__ $$aLagarde, N.
000006051 700__ $$aLudwig, H. -G.
000006051 700__ $$aMahy, L.
000006051 700__ $$aMapelli, M.
000006051 700__ $$aMarfil, E.
000006051 700__ $$aMartell, S. L.
000006051 700__ $$aMessina, S.
000006051 700__ $$aMiglio, A.
000006051 700__ $$aMinchev, I.
000006051 700__ $$aMoitinho, A.
000006051 700__ $$aMontalban, J.
000006051 700__ $$aMonteiro, M. J. P. F. G.
000006051 700__ $$aMorossi, C.
000006051 700__ $$aMowlavi, N.
000006051 700__ $$aMucciarelli, A.
000006051 700__ $$aMurphy, D. N. A.
000006051 700__ $$aNardetto, N.
000006051 700__ $$aOrtolani, S.
000006051 700__ $$aPaletou, F.
000006051 700__ $$aPalouš, J.
000006051 700__ $$aPickering, J. C.
000006051 700__ $$aQuirrenbach, A.
000006051 700__ $$aRe Fiorentin, P.
000006051 700__ $$aRead, J. I.
000006051 700__ $$aRomano, D.
000006051 700__ $$aRyde, N.
000006051 700__ $$aSanna, N.
000006051 700__ $$aSantos, W.
000006051 700__ $$aSeabroke, G. M.
000006051 700__ $$aSpina, L.
000006051 700__ $$aSteinmetz, M.
000006051 700__ $$aStonkuté, E.
000006051 700__ $$aSutorius, E.
000006051 700__ $$aThévenin, F.
000006051 700__ $$aTosi, M.
000006051 700__ $$aTsantaki, M.
000006051 700__ $$aWright, N.
000006051 700__ $$aWyse, R. F. G.
000006051 700__ $$aZoccali, M.
000006051 700__ $$aZorec, J.
000006051 700__ $$aZucker, D. B.
000006051 773__ $$cA120 (36pp)$$pAstronomy & Astrophysics$$v666
000006051 8560_ $$fronny.blomme@observatoire.be
000006051 85642 $$ahttps://www.aanda.org/articles/aa/full_html/2022/10/aa43134-22/aa43134-22.html
000006051 85642 $$ahttps://ui.adsabs.harvard.edu/abs/2022A%26A...666A.120G/abstract
000006051 905__ $$apublished in
000006051 980__ $$aREFERD