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Fig. D.1.

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Observed-frame, best-fit SED models of lid_1639. Purple empty circles mark observed flux densities, purple empty triangles the observational upper limits and red filled circles indicate the best-fit model prediction. Yellow (blue dashed) lines are for the stellar (un)attenuated emisson; green lines for the nebular emission; red lines for dust emission; orange lines for the AGN component and black lines for the total, best-fit model. The SEDs of the rest of the AGN sample are available on Zenodo at the following link: https://doi.org/10.5281/zenodo.13149280.

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