SFR surface density profiles estimated from Hα, of X-ray AGNs with lower L_X/M_★ (log L_X/M_★ < 30.5) and normal galaxies utilized in Fig. 11. We can see that even the mean Σ_SFR estimated from Hα emission from spaxels that are not AGN-dominated is elevated compared to that of non-AGNs in the control galaxy sample, suggesting that a minute level of SF enhancement is likely among the hosts of these very weak AGNs, when we select an SF indicator that is sensitive to very recent SF activity.