Fig. G.1.
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Left: Best-fit reduced χ2 as a function of SMA for the galaxies analysed radially. Colours are as in Fig.2. Solid (dashed) lines indicate fits performed without (with) a UV upturn component. Right: As in the left panel, but only for NGC 1272. In this case, the solid line indicates a no Upturn model with the addition of a post-starburst component in the SFH.
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