Fig. 4.

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Differences between aperture-corrected (x axis) and non-corrected quantities (y axis), such as sSFR (left-hand-side panel), present-day stellar mass as obtained by FADO (central panel) and stellar surface density (right-hand-side panel), for the EELG sample. Identity lines are represented in grey. As in Fig. 3, data points are coloured as specified by their redshift distribution.
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