Figure A1.
Quasar (thick solid lines) and radio (faint dashed lines) mode fractions for AGN in fable as a function of redshift. All models show a clear average decrease with redshift of AGN fraction in quasar mode. The quasar mode dominates at $z \gtrsim 4$, whereas the radio mode becomes more important below this redshift. The Fiducial model has an overall higher quasar mode fraction due to its lower quasar mode threshold (see Table 1).

Quasar (thick solid lines) and radio (faint dashed lines) mode fractions for AGN in fable as a function of redshift. All models show a clear average decrease with redshift of AGN fraction in quasar mode. The quasar mode dominates at |$z \gtrsim 4$|⁠, whereas the radio mode becomes more important below this redshift. The Fiducial model has an overall higher quasar mode fraction due to its lower quasar mode threshold (see Table 1).

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