Examples of the best SED fittings of the different AGN types: The blazar Mrk 421 is shown in the top panel, the Seyfert1 PG0052+251 in the second panel, the Seyfert 1.5 Mrk 290 in the third panel, and the Seyfert 2 Ark 564 in the bottom panel. The yellow and green solid curves show the emission from the stellar population and cold dust of the galaxy, respectively. Purple, dark blue, and light blue solid curves show the torus, accretion disk, and radio AGN emission models, respectively. Ten models constructed from combinations of parameters randomly selected from the posterior PDFs (hereafter referred to as realizations) are plotted as shaded areas and the residuals of each fit realization are presented in the graphs below each source. A flexible energy balance prior was assumed so that the cold dust IR emission is at least comparable to the dust-absorbed stellar emission.