Fig. 4.
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Distributions of the main physical parameters obtained through SED fitting for the initial and final, reduced, sample. Top-left panel: redshift distribution. Top-right panel: AGN fraction distribution, computed in the 5–40 μm range. Bottom-left panel: logarithm of stellar mass distribution, in units of solar masses. Bottom-right panel: logarithm of the dust luminosity in solar luminosities.
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