Fig. 8
Comparison of star formation rates of AGN and non-AGN host galaxies. Plotted are the objects detected in at least three Herschel bands (dashed green). A comparison sample of objects (solid magenta) is selected from some of the deepest Herschel data, from PACS-GOODS South field (Rodighiero et al. 2011). The vertical lines correspond to the average values of the FIR-detected (solid lines) and non-detected (dashed lines) stacked subsamples, discussed in Sect. 4.4.
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