Fig. C.1.
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Spectral energy distribution of 3C 326 N. The MIR-to-FIR photometry is fitted using CIGALE. The stellar attenuated and unattenuated contributions are shown in blue and orange, respectively. The reprocessed IR emission is presented in purple and the AGN emission is in green. The best model is shown as a solid black line. The observed uncertainties are added in quadrature with a 10% floor value to account for possible instrumental errors.
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