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Fig. 3.

image

SFR (top) and dust mass (bottom) as function of stellar mass derived by Rowlands et al. (2012). The star formation main sequence at z = 0.13 is plotted as a solid line, with the scatter shown as dotted lines (Speagle et al. 2014). The early-type galaxies within the main sequence are plotted as open symbols. Filled symbols which appear to be within the main sequence are galaxies at higher redshifts, for which the main-sequence is higher. The typical errors are shown as large crosses. The Spearman rank correlation coefficient for the Md − M* diagram is 0.5 with a very small probability (∼3 × 10−5, ∼4σ) of the null hypothesis (no correlation) being acceptable.

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