Fig. 7.

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Central panel: comparison between i and Ks-based masses. Blue and red dots represent ELGs and passive galaxies, respectively. The gray line corresponds to the 1:1 line ratio. Upper panel: distribution of optical luminosity based stellar masses. The black line shows the mass distribution of the complete sample, whereas the blue and red areas indicate the distribution of ELGs and passive galaxies, respectively. Right panel: distribution of near-infrared luminosity based stellar masses.
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