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Fig. 9.

Fig. 9. Refer to the following caption and surrounding text.

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First panel: Redshift evolution of the fraction of galaxies whose central MBH underwent at least one (solid line) or five (pale lines) super-Eddington phases (fSupEdd). Second panel: Redshift evolution of the epoch at which MBHs within a given stellar mass bin experienced their most recent super-Eddington accretion phase ( z SupEdd Last Mathematical equation: $ z^{\mathrm{Last}}_{\mathrm{SupEdd}} $). Third panel: Redshift evolution of the epoch at which MBHs within a given stellar mass bin experienced their first super-Eddington accretion phase ( z SupEdd First Mathematical equation: $ z^{\mathrm{First}}_{\mathrm{SupEdd}} $). Fourth panel: Median value of the largest mass inflow (inflow) that triggered the super-Eddington phase in the MBH. The colour coding and mass dependence are the same as in Fig. 4.

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