AGN SEDs for our high- and low-luminosity subsamples. Left panel: blue (red) dotted curves represent AGN SEDs of sources with L₅₁₀₀ greater (less) than the median L₅₁₀₀ (﹩{10}^{44.55}\,\mathrm{erg}\,{{\rm{s}}}^{-1}﹩). Right panel: the blue and red solid curves represent the median SEDs of the high- and low-luminosity AGN subsamples, respectively. Shaded regions are the 1σ uncertainties derived by bootstrapping. Luminous sources tend to have cooler SEDs (i.e., larger FIR fluxes for fixed MIR emission) than less luminous ones.