Fig. 5
Spectral energy distribution (SED) of the unresolved central point source and the extended far infrared emission observed with Herschel PACS and SPIRE. The blackbody curve shown for the central (point source) emission is derived from the near- to far-infrared SED shown in Fig. 6. The modified black body shown for the extended emission is the best-fit to the Herschel measurements (averaged over all epochs).
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