Аннотация: We propose a method for extracting kinematics, age and metallicity of the stellar population in the inner kpc of active galactic nuclei, based on pixel fitting of high-resolution (R > 1500) spectra with synthetic stellar populations. Our analysis method can efficiently constrain the kinematics of the stellar population beneath the AGN and restore the age and metallicity. But the constraint on the AGN contribution to the continuum remains poor.