Dusty torus model fits. The data points are the same as in Fig. 2, with the X-ray and radio ranges cropped. The red line represents the AD model, with a break to f_ν ∝ ν² indicated by the red dashed line beyond 3 μm in the rest frame (Hönig & Kishimoto 2010). The AD and BB (orange line) models were subtracted from the WISE/Herschel/SCUBA-2 data, and the 960 models of Hönig & Kishimoto (2010) were fitted to the subtracted data. The solid blue lines show the median (darkest) of the fits and the 68% and 95% (lightest) ranges. The dotted blue lines represent the statistical uncertainty for an individual fit.