Similar to Fig. 13, but for higher-L_[OIII]/M_★ optical AGNs (left) and lower-L_[OIII]/M_★ optical AGNs (right). Consistent with the clear differences in the mean Σ_SFR profiles presented in Fig. 12, offsets in the median values of the distributions (indicated by short horizontal lines) are observed for both groups in the central regions of galaxies. The overall distributions of Δ log Σ_SFR for individual matched pairs are broad, extending significantly into both positive and negative values.