The optical-infrared relation for active galactic nuclei: The role of contaminations

Open Access

Fig. 5.

Transition luminosity above which the SED fit is dominated by the AGN components in the consecutive redshift bins. The red points show $L_{IR}^{photo}$ $Mathematical equation: $ L_{\mathrm{IR}}^{\mathrm{photo}} $$ , which approximates the dusty torus, and the green points reveal the corresponding fluxes. The blue points visualize $L_{OPT}^{photo}$ $Mathematical equation: $ L_{\mathrm{OPT}}^{\mathrm{photo}} $$ , which correspond to the accretion disk.

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