Median distribution of the SED estimated and observed fluxes. On the x-axis, each wavelength corresponds to the photometric bands used in the SED fitting. The difference between the computed Bayesian flux with CIGALE and the observations is shown in the y-axis. Each object in our sample is drawn as a gray dot with a S/N > 3 in each band. Median values are shown as green squares. The median values for objects with S/N > 3 in both Herschel PACS 100 μm and Herschel PACS 160 μm are presented as red squares. Dispersion on the flux difference at each wavelength is reported on top.