Fig. A.2
Relationship between the torus angle with respect to the line of sight (ψ) and the fractional contribution of AGN MIR emission for ULIRGs (left panel) and LIRGs (right panel) for the sample of original ADF-S galaxies (red circles), the ADF-S sample with redshift increased by 0.05 (orange stars) and the ADF-S sample with redshift reduced by value 0.05.
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