Fig. A.3.

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SFR-stellar mass relation for galaxies from the MS sample, colour-coded as a function of redshift. Despite the applied normalisation to redshift z0 = 0.7, we still see a dichotomy. High redshift galaxies tend to align along lines with the largest specific star formation rate (sSFR), while low redshift galaxies tend to align along lines with the lowest sSFR because of the survey design.
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