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Fig. 10.

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Colour–colour diagrams using JWST filters. Left panel: smooth CYGNUS torus model SEDs at z = 0. Right panel: smooth CYGNUS torus model SEDs at z = 1. Blue circles correspond to the broad-band filter ratio for all the SEDs of smooth CYGNUS torus models. Grey stars represent those ratios of the model SEDs of deeply obscured nuclei (classified based on the continuum ratio criteria presented in Sect. 5). The purple square denotes the region where CON-dominated sources are located (see Sect. 6). Colour-coded squares correspond to the host galaxy contribution of the track of simulated spectra for a galaxy containing a CON shown in Fig. 5.

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