Malagnini, M. L.M. L.MalagniniMOROSSI, CarloCarloMOROSSIBUZZONI, AlbertoAlbertoBUZZONIChávez, M.M.Chávez2023-02-062023-02-0619990004-640Xhttp://hdl.handle.net/20.500.12386/33174We present the results obtained by comparing mid-resolution stellar spectra of super metal rich candidates with synthetic spectra computed in the wavelength range 4850-5400 Å. Atmospheric parameters, derived by using the flux fitting method, are illustrated for a sample of representative stars. The final aim of the project is the definition of a fully consistent metallicity scale for SMR stars.STAMPAenArticle10.1023/A:1002140700934https://link.springer.com/article/10.1023/A:10021407009341999Ap&SS.265..341MFIS/05 - ASTRONOMIA E ASTROFISICA