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We present a new stellar atmosphere interpolator which we will use to computestellar population models based on empirical and/or synthetic spectra. Wecombined observed and synthetic stellar spectra in order to achieve more orless uniform coverage of the (T_eff , log g, [Fe/H]) parameter space. Wevalidated our semi-empirical stellar population models by fitting spectra ofearly-type galaxies from the SDSS survey

Stellar atmosphere interpolator for empirical and synthetic spectra