Chavez, M.M.ChavezMalagnini, M. L.M. L.MalagniniBUZZONI, AlbertoAlbertoBUZZONIMOROSSI, CarloCarloMOROSSI2024-01-302024-01-3020011405-2059http://hdl.handle.net/20.500.12386/34660We report on preliminary results of a project intended to construct a homogeneous spectroscopic data base of super metal-rich stars (SMR). The data base will serve as a tool for studies of old stellar populations. Using the flu x fitting method we have compared mid-resolution spectroscopic data of a sample o f SMR candidates with a grid of synthetic spectra and derived simultaneously the three leading atmospheric parameters (T<SUB>eff</SUB>, log {g}, [M/H]).STAMPAenConference paper2001RMxAC..11...81CFIS/05 - ASTRONOMIA E ASTROFISICA