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Fig. 1.

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Examples of SEDs from sources used in our analysis. The top panels present AGN classified as type 1 based on their optical spectra. Their SFR and stellar mass are log [SFR(M yr−1)] = 1.63, log [M*(M)] = 10.06 (top, left panel) and log [SFR(M yr−1)] = −0.45 and log [M*(M)] = 10.75 (top-right panel), respectively. The bottom panel presents the SEDs of two AGN classified as type 2 based on their optical spectra. Their SFR and stellar mass are log [SFR(M yr−1)] = 1.87, log [M*(M)] = 10.30 (bottom, left panel) and log [SFR(M yr−1)] = −1.0 and log [M*(M)] = 10.24 (bottom-right panel), respectively.

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