Fig. 7.

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Dust mass as a function of the SFR. Progenitors of the selected ETGs are connected with the lines. Empty red (blue) circles show the progenitor galaxy with a major (minor) merger event before that snapshot. Each row corresponds to one selected ETGs. The left column shows the colour-coded bulge-to-total mass ratio, whereas the right shows the same galaxy but colour-coded by the black hole mass.
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