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Fig. 22.

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EWHα versus [NII]/Hα-computed frequencies (criteria of Gavazzi et al. 2011) of SF, SEY, LIN and RET as a function of log(Mstar/M⊙) (represented by the six bins M1, ..., M6) in the three halo-mass bins defined in Sect. 2.3.2.
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