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Fig. 6.

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sSFR for the galaxy sample, averaged over three mass bins, indicated by the legend, as a function of cosmic time. Thick lines correspond to the mean values and the surrounding shaded area to the 1σ dispersion of the distributions. Diamonds and stars indicate the mean sSFR from SED and [O II] emission line measurements, respectively, placed in arbitrary positions in the x-axis for better visualisation.

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