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Fig. 5.

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SFR derived from the relations given in Brown et al. (2017) using GALEX FUV and the attenuation law from Calzetti et al. (2000) (left) and Hao et al. (2011) (right). Blue points represent the VIPERS galaxies and density hexabin represent the GSWLC galaxies sample. The blue line is the fit for VIPERS galaxies, the red line is the fit for GSWLC galaxies, and the green line is the 1:1 relation. The agreement is better with the Hao et al. (2011) attenuation correction recipe, both for VIPERS (mean and scatter of 0.01 and 0.05 dex) and GSWLC (−0.02 and 0.25 dex), compared to Calzetti et al. (2000) (0.09 and 0.10 dex for VIPERS, 0.02 and 0.30 dex for GSWLC).

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