Fig. 1
Scatter plot of the predicted CIGALE flux densities against the flux densities from the COSMOS2015 catalogue for the 250 μm (blue points), 350 μm (green points), and 500 μm (red points). The errors for the catalogue flux are instrumental noise plus confusion noise. The one-to-one line (magenta) and y = 0.4x (cyan) illustrate that the data better fits the idea that bright sources in catalogues are overestimated.
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