Here we present the distribution of the AGN contribution to the continuum and the AGN-continuum slope for the different BPT classes. Top: distribution of the AGN relative contribution (f_5100, AGN/f_{5100, cont.}). For different BPT classes, according to the [OIII]/H_β vs. [N II]/H_α diagram. The distributions for different classes, star-forming (purple), composite (pink), and Seyfert/LINER (brown) are similar to the Seyfert/LINER objects concentrated between 0.3 < f_5100, AGN/f_{5100, cont.} < 0.75. Bottom: Distribution of the fitted power slope for the same BPT classes.