Fig. 10.

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SFR vs M★ for the three AGN types. We show the SED AGN as a 2D distribution. In each panel, the contours (from 10% to 90%, with intervals of 10%) represent the non-AGN distribution. The dashed blue and the dash-dotted green lines indicate the MS at z = 2 and z = 0.5 from Popesso et al. (2023), respectively. On top of each panel is the M★ distribution of the AGN and the corresponding non-AGN (grey).
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