Fig. 20
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Comparison of our SFR values (derived from our MAGPHYS fits to data in GALEX, SDSS, and WISE filters) to those estimated using only WISE W3 and W4 photometry combined with the relations provided in CL 14. The left panel shows the comparison to the relation using W3, and the right panel shows the comparison to the relation using W4. The typical error is shown in the bottom right corner of each panel. The sample is colour-coded according to morphology, as shown in the legend.
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