Resulting rest-frame SED decompositions for half of the sources (continues in Fig. 6). Black circles are the rest-frame photometric points corresponding to the observed bands used to constrain the SED. Black open circles represent the photometric points not included in the fits (at λ < 1216 Å due to Ly-α absorption, see the text for more details), while the black arrows correspond to upper limits on the observed flux densities at 1σ. Lines (and shaded areas) correspond to the model templates (and the 1σ error) found as best-fit solution to describe the photometric points through the χ² minimisation: blue is the accretion disc plus torus template (AD + T), red is the cold dust component (CD) while dark green is the NIR excess (NE) when present. Finally, the black line shows the sum of all these contributions. Blue, orange, and light green shaded areas correspond to the accretion disc plus torus, the cold dust, and the NIR excess templates within 1σ of the best-fit template, and light grey shaded area to their sum.