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Fig. 14.
Relation between W [OIII] and 5100 Å luminosity for the cosmo sample and the total [OIII] SB+NC emission. Red color: Sulentic et al. (2017); purple: Netzer et al. (2004); gray: low-z sample (Marziani et al. 2003). Open squares are Pop. B, filled circles Pop. A. The cosmo sample data points are shown as filled blue circles.
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