Tautvaisiene, G.G.Tautvaisiene0000-0001-6081-379XDrazdauskas, A.A.Drazdauskas0000-0002-0845-6171Mikolaitis, S.S.Mikolaitis0000-0002-0338-7883Barisevicius, G.G.Barisevicius0000-0003-0788-5879Puzeras, E.E.Puzeras0000-0003-4486-6802Stonkute, E.E.StonkuteChorniy, Y.Y.Chorniy0000-0003-2438-0899MAGRINI, LAURALAURAMAGRINI0000-0002-3638-5788ROMANO, DonatellaDonatellaROMANO0000-0003-0014-519XSmiljanic, R.R.SmiljanicBRAGAGLIA, AngelaAngelaBRAGAGLIACarraro, G.G.CarraroFriel, E.E.FrielMorel, T.T.MorelPANCINO, ELENAELENAPANCINODonati, P.P.DonatiJimenez-Esteban, F.F.Jimenez-EstebanGilmore, G.G.GilmoreRANDICH, Maria SofiaMaria SofiaRANDICHJeffries, R. D.R. D.JeffriesVALLENARI, AntonellaAntonellaVALLENARIBensby, T.T.BensbyFLACCOMIO, EttoreEttoreFLACCOMIORecio-Blanco, A.A.Recio-BlancoCostado, M. T.M. T.CostadoHill, V.V.HillJofre, P.P.JofreLardo, C.C.Lardode Laverny, P.P.de LavernyMasseron, T.T.MasseronMoribelli, L.L.MoribelliSousa, S. G.S. G.SousaZAGGIA, SimoneSimoneZAGGIA2020-03-042020-03-042015http://hdl.handle.net/20.500.12386/23106Observations were conducted with the FLAMES (Fiber Large Array Multi-Element Spectrograph) multi-fiber facility in spring of 2012 and 2013. Spectra of high-resolving power (R~47000) were obtained with UVES (Ultraviolet and Visual Echelle Spectrograph) The spectra were exposed onto two CCDs, resulting in a wavelength coverage of 4700-6840Å with a gap of about 50Å in the centre. <P />(6 data files). <P />enDatabasehttp://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/573/A552015yCat..35730055TFIS/05 - ASTRONOMIA E ASTROFISICA