Fig. 2.
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Distribution of sources in the (u − r)0 vs. (r − z)0 colour-colour plane. The parent sample is shown in grey, while the increasingly restrictive subsamples (adding velocity dispersion, query and spectroscopic information) are shown in light blue, dark blue and maroon, respectively. The dashed black line defines the passive galaxy region (Holden et al. 2012).
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