Fig. 9.
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Best-fit AGNSED models for our 3 × 3 MBH-λEdd grids (excluding the two with potential star formation contamination). Different components are shown with the same color convention as in Fig. 8. As no data are involved, we scaled the y-axis to physical values (erg s−1) by setting the AGNSED distance parameter as dL = 100 Mpc and the normalization to 4πdL2.
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