Fig. 3.
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Normalized SFR (SFRnorm) for the three AGN populations as a function of key physical parameters. Top left: SFRnorm versus [OIII] luminosity. Top right: SFRnorm as a function of black hole mass. Bottom left: SFRnorm as a function of environmental density. Bottom right: Distributions of stellar ages, using the D4000 index as a proxy.
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