Fig. A.2
Comparison between the ratio of the SFR as obtained from the SFR calibrators MIPS 24 μm and PACS 70 μm (top), FUV+MIPS 24 μm and FUV+TIR (middle) and FUV+MIPS 24 μm and FUV+1.4 GHz (bottom) as a function of oxygen abundance. Galaxies are color-coded according to metallicity with increasing oxygen abundances ranging from black then blue, green and yellow to red colors. The dotted red and dashed black lines represent the best fit and a perfect one-to-one correlation, respectively. The dispersion around the best fit is indicated in the bottom right corner.
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