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Fig. 8.

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Distributions of the SFRnorm of type 1 (blue line) and type 2 (red shaded histogram) AGN. Our results show that, in the local Universe (z < 0.2), there is a significant fraction of X-ray AGN that live in quiescent systems (SFRnorm < 0). This appears to be more prominent in the case of type 2 AGN.

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