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Fig. A.1


Same as Fig. 5, but for Sref sample of galaxies. Left panel: Log SFR – Log M plane colour–coded according to the weighted average B/T in the bin. The white line represents the location of the MS of SFGs, and the error bars show its dispersion. Right panel: B/T ratio as a function of ΔMS (distance from the MS) in different stellar mass bins.

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