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Fig. 8


Positions (red stars) of SDP.9 and SDP.11 in the main sequences of AGNs (LX or LAGN vs. M, left panel) and star-forming galaxies (SFR vs. M, right panel). Data based on a mass-selected sample are from Rodighiero et al. (2015; black circles), with the cyan shaded area illustrates the typical scatter around the mean relationship.

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