Gallery of AGN emission templates. On the left panel, the red lines are the observed AGN emission templates built with a fixed δ_AGN = 1 and our new α_IRX variation. On the right panel, the black lines show a gallery of AGN templates built with varying δ_AGN to lower values. These lower values of the new δ_AGN produce a larger variation in UV slopes and IR behavior compared to those generated by the previous standard accretion disk model.