SFRs and stellar masses M_* for all HECATE galaxies in the eFEDS field (filled black circles) and the eFEDS-HECATE matches split into their respective classifications as described in Sect. 2.3. Only galaxies that have these parameter estimates are shown. The symbol size is proportional to the eROSITA detection likelihood. We also overlay lines of sSFR for reference. The AGN-hosting galaxies are at preferentially lower SFR (early-type) when compared with the star-forming galaxies. We only plotted galaxies having M_* > 10⁸ M_⊙; there are 13 galaxies below this limit.