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Fig. B.1
Left panel: Log SFR – Log M⋆ plane colour–coded as a function of the weighted average of the R90/R50 ratio. The white line represent the location of the MS of SFGs, and the error bars its dispersion. Rightpanel: R90/R50 ratio as a function of the distance from the MS (ΔMS) in different stellar mass bins.
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