Comparison of our stellar spectroscopic masses derived from GSP-Spec parameters and Gaia data with APOKASC masses of giants (red points) and dwarfs (blue points) from Pinsonneault et al. (2018) and Serenelli et al. (2017), respectively. The selection is restricted to sources for which the agreement in log(ɡ) is better than 0.05 dex between GSP-Spec and APOKASC, as the spectroscopic masses are sensitive to the stellar surface gravity.