Comparison of SFR residuals from the SFMS and SFMS+gas model against various AGN parameters. Upper left panel: histograms of the residuals for SFMS and SFMS+gas for both Hα and IR models, with the red, blue, and purple colors corresponding to the previous plots (Figs. 6 and 7, background colors). The other panels show the comparison of the AGN parameters taken from Husemann et al. (2022) and Singha et al. (2022): logarithm of BH mass (upper center), logarithm of AGN bolometric luminosity (upper right), number of the objects, containing extended outflows (lower left), logarithm of Eddington ratio (lower center), and b/a morphological parameter (lower right). Each of the four models is represented with three bins (from left to right: negative red, central blue, positive purple) and the forth bin with the upper limits (gray). The error bars of the bins also represent the distribution of the parameters within the bins. The black dots and lines highlight the trend of the mean values that are written over the bins.