Fig. 9

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Some examples of SEDs of AGN from our lightcone. We show three representative cases: in the upper panel, we show a type 1 AGN with dominant QSO component in the rest-frame UV band, while in the middle panel, we show a type 1 AGN with similar QSO and host-galaxy contribution for the same band. The lower panel shows a type 2 AGN, with a zoom-in subpanel showing the Hβ and the [O III] λλ 5007, 4959 doublet emission lines. The galaxy component (bulge + disc) is shown with a dotted orange line, and is based on Bruzual & Charlot (2003) models. The AGN component, which consists on a full SED template from Temple et al. (2021) for type 1 and narrow emission lines for type 2 is shown with a dashed violet line. The cyan line shows the composed SED. Dust absorption is applied in all cases.
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