Relation between SFR and M_* for RDAGN host galaxies (green), the full control sample (brown), RLAGN subsample (black x’s), RLAGN control galaxies (red x’s), and entire Pipe3D catalog (gray). For reference, the SFMS derived for SDSS-IV MaNGA galaxies is indicated by the dotted line (Cano-Díaz et al. 2019), the dark gray shading represents the errors on slope, and the light gray shading represents the standard deviation. The best-fit relations for radio-quiet AGN (dashed line) and radio-mode AGN (solid line) are from Comerford et al. (2020).