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Fig. 7.

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Comparison of stacked W80 profiles and host galaxy properties between non-AGNs and sample A. In each plot, blue corresponds to the behavior of a specific parameter for sample A (see Sect. 4.1) and black for non-AGNs. For each column of plots, from left to right, we show the W80 stacked radial profile, the log(M) distribution, the log(L[O III]) distribution, and the log(SFR(Hα)) distribution. The plots in the bottom row show how both samples behave after they are matched to have the same log(M) and log(L[O III]). The plots in the top row show how both samples behave if the matching is done only for log(M). The Venn diagrams shown in each W80 plot represent sample A. The discrepancy in the Venn diagram numbers in sample A arises from the incorporation of L[O III] into the control.

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