Fig. 6
Averaged SED for OJ 287 from the data in Fig. 5, including data from the IRAS faint source catalogue, scaled by × 0.4 to bring them to the same level as the interpolation of the Herschel and visible to near-IR data. A nominal 10% error bar has been plotted on each datum. There is no evidence of a 60 μ m bump from possible dust emission from the host galaxy.
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