Fig. 3
Top: fractions of quiescent galaxies (black) and ELGs (yellow), and for w1 cluster galaxies (left), one realization of 
and w0t,M (middle and right). Bottom: prevalence of different ELG classes identified in the DD[NII] from uncensored diagnostic ratios: Hii (blue), transition objects (pale gray), LINERs (red), and Seyferts (magenta), ordered as in the top row.
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