Left: X-ray-selected AGNs and optically selected AGNs on the M_★ versus SFR plane, as labeled. All galaxies in the sample are displayed as background points, with grayscale intensity encoding their weights. The error bar in the corner indicates uncertainties in M_★ and SFR derived from pyPipe3D SSP decomposition, estimated by comparison with independent measurements (Sánchez et al. 2022). Right: Similar to the left panel, but for the Σ₁ versus Σ_{SFR, 1 kpc} plane. The dashed line depicts the spatially resolved star formation MS from Hsieh et al. (2017). The error bar in the corner indicates approximate uncertainty scales for Σ₁ and Σ_{SFR, 1 kpc} (see Footnote 2).