Fig. B.3.
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Star formation rate tracer derived from NUV and MIR emission, following the prescription in Janowiecki et al. (2017), derived in the present paper and compared with different SFR tracer. Left: SFR of the VGS derived from Hα maps (Beygu et al. 2016). Centre: SFR of the xCOLD GASS sample derived from NUV and MIR emission (Saintonge et al. 2017). Right: SFR of the HI-CALIFA sample derived from Hα maps (Catalán-Torrecilla et al. 2015).
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