Fig. 9
Correlations between the star formation rates (PAH- and TIR-derived) and stellar masses of the 231 successfully fitted ATLAS3D galaxies. Data points are colour coded according to their mass-weighted stellar population age (McDermid et al. 2015). Dotted black lines show the star formation main sequence of local star-forming galaxies (Elbaz et al. 2007). Dotted blue, green, and red lines show the best linear fits for the age range 3–7, 7–11, and 11–14 Gyr, respectively.
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