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Fig. A.1

image

Example of a SED fitting test. Left panel: distribution of the AGN luminosity, SB luminosity, and stellar mass obtained in 100 iterations obtained from theoretical SEDs, and by varying the photometric points according to the observed uncertainties compared to the theoretical value represented by the dashed line. Right panel: as before, but we plot the distribution in percentage of the relative errors for the parameters in each iteration.

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