Presence (or not) of a broad component of the Hα line in four AGNs with different fractions of light in the young population (f_y) according to the STARLIGHT fit: NGC 7582 and NGC 3081 do not show broad components of the Hα line, and yet STARLIGHT finds a young stellar population in these two galaxies. And, vice versa, in NGC 2992, there is a very strong broad component to the Hα line, but no young stellar population is found. Only in MCG-05-23-016 do we find both a young population and a broad component. Overall this confirms the robustness of the detection of young stellar light, and that it is likely not confused with the non-stellar continuum from the AGN.