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The program package SME (Spectroscopy Made Easy), designed to perform ananalysis of stellar spectra using spectral fitting techniques, was updated dueto adding new functions (isotopic and hyperfine splittins) in VALD andincluding grids of NLTE calculations for energy levels of few chemicalelements. SME allows to derive automatically stellar atmospheric parameters:effective temperature, surface gravity, chemical abundances, radial androtational velocities, turbulent velocities, taking into account all theeffects defining spectral line formation. SME package uses the best grids ofstellar atmospheres that allows us to perform spectral analysis with thesimilar accuracy in wide range of stellar parameters and metallicities - fromdwarfs to giants of BAFGK spectral classes.

Program package for the analysis of high resolution high signal-to-noise stellar spectra