Abstract
We present integrated spectra in the optical range for 10 concentrated Magellanic Clouds' (MCs) stellar clusters (SCs), six of them belonging to the Large Magellanic Cloud (LMC), and the other four to the Small Magellanic Cloud (SMC). We estimate simultaneously age and foreground reddening by comparing the continuum distribution and line strengths of the cluster spectra with those of template spectra. The present cluster sample complements previous ones, in an effort to create a spectral library for the MCs with several clusters per age bin.
