Fig. 6.

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Comparison of stacked W80 profiles and host galaxy properties between non-AGNs and optical AGNs. In each plot, blue corresponds to the behavior of a specific parameter for optically selected AGNs and black for non-AGNs. We show the W80 stacked radial profile, the log(M⋆) distribution, the log(L[O III]) distribution, and the log(SFR(Hα)) distribution. For this comparison, only log(M⋆), redshift, and morphology were controlled.
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