Fig. 1.

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SFR as a function of stellar mass for the GAMA sample (top three rows) and the DD20 sample (bottom row). The star-forming MS at median redshift of each redshift bin (grey line) based on Speagle et al. (2014) is shown. Colour coding distinguishes galaxies on or above the MS (blue stars) and galaxies below the MS (red circles). The MS offset of each redshift bin is presented at the bottom right of each panel together with the fraction of MS and below-MS galaxies.
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