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Fig. B.1.


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From top left to bottom right: SED fitting of J1524+4409, B1608+656, J1330+1810, J1455+1447, J1633+3134, and J0924+0214. The black dots represent the observed data points; 3σ upper limits are shown as downward arrows. The best-fit SED obtained with AGNfitter (Calistro Rivera et al. 2016), as well as the different components used to model the total flux are shown as labelled in the figure. Ten realisations picked from the posterior distribution are shown.

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