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Fig. 3

image

AGN host galaxy starburstiness RSB as a function of M for DI scenario (upper panels, solid contours for the fiducial model and black dashed contours for α = 2) and IT scenario (lower panels) in three different redshift bins. Only AGN with luminosity LX> 1042.2 erg s-1 are considered. The filled contours correspond to equally spaced values of the density (per Mpc3) of model AGN in logarithmic scale: from 10-7 for the lightest filled region to 10-4 for the darkest. The data points indicate the XMM-COSMOS AGN with LX> 1042.2 erg s-1. Circles and arrows indicate AGN with SFR derived from LFIR, triangles indicate AGN with SFR derived from SED fitting. Solid lines show the position of the galaxy main sequence, dashed lines denote the limits of the starburst and passive regions, defined as RSB> 4 and RSB< 1/4, respectively.

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