Fig. 2.
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Photometric and spectroscopic selection criteria. Top: UVJ diagram for the main selection steps. Galaxies above the dashed line are qualified as passive following the criterion in McLure et al. (2018). Bottom: EW[OII] versus H/K ratio, colour-coded by S/N[OII], for the sample after the UVJ cut. The shaded areas show the discarded ranges for both quantities.
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