MAGRINI, LAURALAURAMAGRINI0000-0003-0304-9910RANDICH, Maria SofiaMaria SofiaRANDICH0000-0003-4486-6802Kordopatis, G.G.Kordopatis0000-0003-2438-0899Prantzos, N.N.Prantzos0000-0002-3638-5788ROMANO, DonatellaDonatellaROMANO0000-0003-0014-519XCHIEFFI, ALESSANDROALESSANDROCHIEFFI0000-0003-4979-0659LIMONGI, MarcoMarcoLIMONGI0000-0001-6081-379XFrancois, P.P.Francois0000-0002-0845-6171PANCINO, ELENAELENAPANCINO0000-0002-7065-3061Friel, E.E.Friel0000-0002-0338-7883BRAGAGLIA, AngelaAngelaBRAGAGLIA0000-0003-0788-5879Tautvaisiene, G.G.Tautvaisiene0000-0003-3969-0232Spina, L.L.SpinaOverbeek, J.J.Overbeek0000-0003-0636-7834Cantat-Gaudin, T.T.Cantat-Gaudin0000-0002-3589-3203Donati, P.P.Donati0000-0002-6893-2221VALLENARI, AntonellaAntonellaVALLENARI0000-0002-2697-3607SORDO, ROSANNAROSANNASORDOJimenez-Esteban, F. M.F. M.Jimenez-EstebanTang, B.B.TangDrazdauskas, A.A.DrazdauskasSousa, S.S.SousaDuffau, S.S.DuffauJofre, P.P.JofreGilmore, G.G.GilmoreFeltzing, S.S.FeltzingAlfaro, E.E.AlfaroBensby, T.T.BensbyFLACCOMIO, EttoreEttoreFLACCOMIOKoposov, S.S.KoposovLanzafame, Alessandro CarmeloAlessandro CarmeloLanzafameSmiljanic, R.R.SmiljanicBayo, A.A.BayoCarraro, G.G.CarraroCasey, A. R.A. R.CaseyCostado, M. T.M. T.CostadoDAMIANI, FrancescoFrancescoDAMIANIFRANCIOSINI, ElenaElenaFRANCIOSINIHourihane, A.A.HourihaneLardo, C.C.LardoLewis, J.J.LewisMonaco, L.L.MonacoMorbidelli, L.L.MorbidelliSACCO, GIUSEPPE GERMANOGIUSEPPE GERMANOSACCOSbordone, L.L.SbordoneWorley, C. C.C. C.WorleyZAGGIA, SimoneSimoneZAGGIA2020-09-162020-09-162017http://hdl.handle.net/20.500.12386/27398We present the stellar parameters, distances, ages, heights, radial velocities and abundances used in the present work. <P />In Table A.1 we present the stellar parameters and radial velocities of the selected member stars in open clusters, while in Table A.2 their elemental abundances. <P />In Table A.3 we show the stellar parameters, ages, distances and heights on the Galactic plane of the solar neighbourhood sample of field stars and of the inner disc stars. <P />In Table A.4 we present their elemental abundances in the 12+log(X/H) form. (4 data files).enDatabase10.26093/cds/vizier.36030002http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/603/A22017yCat..36030002MFIS/05 - ASTRONOMIA E ASTROFISICA