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Fig. B.1


Left: comparison between the 24 μm-based SFR used in the analysis (x-axis) and the SFR measured by fitting the average FIR stacked flux densities for each bin of the grid (y-axis). The colour code indicates the mean stellar mass in each bin. Right: same as the left panel, but FIR-based SFR are compared to the SFR measured by means of a “ladder” approach (see text).

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