Left panel: the SED of the Compton-thick sources NGC 7479 and ESO148-IG002 from the 12 μm sample. Right panel: the SED of the two Compton-thick sources in Comastri et al. (2011) compared to that of the candidate Compton-thick source CDFS-309 in Feruglio et al. (2011). The SEDs have been normalised to have the same flux at 0.5 μm.
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