Comparison between parameter estimates obtained in this work with those obtained with pPXF and the FSPS population synthesis code published in Cappellari (2023). We consider only galaxies in the silver and golden samples (empty and filled symbols respectively) distinguished into Q and SF (magenta circles and blue stars, respectively). The mean difference between BaStA and pPXF estimates, the rms scatter and the mean uncertainties on BaStA estimates (those from pPXF are not provided) are reported in each panel for quiescent (left) and star-forming (right). Stellar metallicities have been reported to a common Z_⊙ = 0.02 scale, and our stellar masses have been rescaled up by 1.75 to match the Salpeter IMF used by Cappellari (2023).