Fig. 7.
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The stellar mass completeness for the sample used in this work (Pozzetti et al. 2010), with a cut at HE < 24, shown as the density of galaxies in the photometric redshifts vs. stellar masses plane. The solid grey line is the 95% stellar mass completeness limit, red dashed-dotted line for passive galaxies, and blue dashed line for SFGs.
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