Fig. 1
Comparison between observed and modelled flux ratios. The shade of the grey hexagons represents the logarithm of the density of models, with a darker shade indicating a higher number of models in the bin. The observed fluxes are indicated by circles, the colour depending on the galaxy. The median error bars including systematic uncertainties are shown on the upper-left side of the plots. The left plot shows the r′/NUV versus NUV/FUV flux ratios and the right plot shows the 70/FUV versus r′/NUV flux ratios.
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