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Fig. 5.

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Best-fitting models for C1 and C6 returned by the CIGALE fitting code. The optical-to-mm photometric points were collected from Hill et al. (2020, 2022), while for C6, we added the radio measurements of Chapman et al. (2024). The absorption-corrected X-ray fluxes correspond to the X-ray models discussed in Sects. 3.1 and 3.3. The sub-mm/mm photometry of C1 is dominated by the AGN-reprocessed emission. The AGN in C6 contributes more modestly at such wavelengths, but dominates the radio emission.

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