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Fig. 9.

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Fraction of quiescent galaxies, fr, as a function of the B-band absolute magnitude (left panel) and stellar mass (right panel) at different redshift (see inset). The dashed lines illustrate the absolute magnitude and stellar mass range for which our quiescent sample is under a completeness level of 𝒞 = 0.25 and 0.05, respectively, meaning that the fraction of red galaxies are obtained through a extrapolation of our results.

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