Enhanced star formation rates in AGN hosts with respect to inactive galaxies from PEP-Herschel observations

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Fig. 1

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Intrinsic X-ray luminosities at 2–10 keV (L_X) as a function of redshift in the three fields for the final AGN sample used in the analysis (Sect. 2.4). Horizontal red lines show the thresholds used to split the sample into high- and low-L_X subsamples (Sect. 5.1).

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