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Fig. A.1

image

Evolution of the CIGALE to true relative difference of M and SFR with the fraction of AGN in the case where the AGN component is not taken into account in the fitting procedure. Left panel shows the results for the stellar mass, middle panel for the SFR, and the right panel the distribution. Blue, green, and red data are for Type-1, intermediate-type, and Type-2 AGNs, respectively.

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