Bonifacio, P.P.Bonifacio0000-0002-0571-4163Caffau, E.E.Caffau0000-0001-6081-379XSpite, M.M.Spite0000-0002-3589-3203LIMONGI, MarcoMarcoLIMONGI0000-0003-0636-7834CHIEFFI, ALESSANDROALESSANDROCHIEFFIKlessen, R. S.R. S.KlessenFrancois, P.P.FrancoisMOLARO, PaoloPaoloMOLAROLudwig, H. -G.H. -G.LudwigZAGGIA, SimoneSimoneZAGGIASpite, F.F.SpitePlez, B.B.PlezCayrel, R.R.CayrelChristlieb, N.N.ChristliebClark, P. C.P. C.ClarkGlover, S. C. O.S. C. O.GloverHammer, F.F.HammerKoch, A.A.KochMonaco, L.L.MonacoSbordone, L.L.SbordoneSteffen, M.M.Steffen2020-05-212020-05-212015http://hdl.handle.net/20.500.12386/25060We analyse both X-Shooter and UVES spectra acquired at the VLT. We used a traditional abundance analysis based on OSMARCS 1D Local Thermodynamic Equilibrium (LTE) model atmospheres and the TURBOSPECTRUM line formation code.(2 data files).enDatabasehttp://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/579/A282015yCat..35790028BFIS/05 - ASTRONOMIA E ASTROFISICA