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Fig. 3


SED decomposition obtained with the code by Berta et al. (2013). Filled squares represent the available photometric data, long-dashed red, dashed blue, and solid black lines represent the AGN+torus component, the emission by stars and dust associated with star formation, and the sum of the two, respectively. Bands are, from left to right, u,b,v,g,r,i,z,J,K, IRAC3.6, IRAC4.5, IRAC5.8, IRAC8.0, MIPS24, PACS100, PACS160, SPIRE250,SPIRE350, SPIRE500. The photometric point at λ(rest) ~ 5000 Å is contaminated by broad and bright [O III] emission (see Sect. 4) and, therefore, is above the best-fit model.

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