MAMBO: An empirical galaxy and AGN mock catalogue for the exploitation of future surveys

Open Access

Fig. A.1

Probability of a galaxy to be an AGN as in Fig. 4 but using the original Schechter fit from B16 to assign the AGN fraction at z < 1.15. The biggest difference with respect to the distribution shown in Fig. 4 is in the high density of low-mass AGN at low redshift.

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