Fig. 1.

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Examples of SEDs in the three fields CCLS, XMM-XXL and eFEDS (from top to bottom). The dust emission is plotted in red, the AGN component in green, the attenuated (unattenuated) stellar component is shown with the yellow (blue) solid (dashed) line, while the orange lines shows the nebular emission. The total flux is represented with black colour. Below each SED, we plot the relative residual fluxes versus the wavelength.
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