Jofre, P.P.Jofre0000-0003-0788-5879Heiter, U.U.Heiter0000-0003-4486-6802Soubiran, C.C.Soubiran0000-0003-0014-519XBlanco-Cuaresma, S.S.Blanco-Cuaresma0000-0003-4979-0659Masseron, T.T.MasseronNordlander, T.T.NordlanderChemin, L.L.CheminWorley, C. C.C. C.Worleyvan Eck, S.S.van EckHourihane, A.A.HourihaneGilmore, G.G.GilmoreAdibekyan, V.V.AdibekyanBergemann, M.M.BergemannCantat-Gaudin, T.T.Cantat-GaudinDelgado-Mena, E.E.Delgado-MenaGonzalez Hernandez, J. I.J. I.Gonzalez HernandezGuiglion, G.G.GuiglionLardo, C.C.Lardode Laverny, P.P.de LavernyLind, K.K.LindMAGRINI, LAURALAURAMAGRINIMikolaitis, S.S.MikolaitisMontes, D.D.MontesPANCINO, ELENAELENAPANCINORecio-Blanco, A.A.Recio-BlancoSORDO, ROSANNAROSANNASORDOSousa, S.S.SousaTabernero, H. M.H. M.TaberneroVALLENARI, AntonellaAntonellaVALLENARI2020-03-042020-03-042015http://hdl.handle.net/20.500.12386/23121As in our previous work on the subject, we built a library of high- resolution spectra of the GBS, using our own observations on the NARVAL spectrograph at Pic du Midi in addition to archived data. <P />The abundance of alpha and iron peak elements of the Gaia FGK benchmark stars is determined by combining 8 methods. The Tables indicate the elemental abundances determined for each star, element, line and method. <P />(36 data files). <P />enDatabasehttp://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/582/A812015yCat..35820081JFIS/05 - ASTRONOMIA E ASTROFISICA