Fig. 3
Best-fit infrared spectral energy distribution (SED) of the quasar 3C 318. Red circles represent the observed photometry, and green circles the estimated photometry (see text). The total SED (black) is given as the sum of AGN-heated hot dust close to sublimation temperature (blue), of torus emission (green, from the library of Hönig & Kishimoto 2010), and of star-formation-heated dust (yellow).
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