Fig. 14.

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Fractional values of the total mass gained (left) and fraction of time spent (right) by the BH in the ‘sEdd’ (filled orange) and ‘sEddThm’ (hashed violet) runs in fEdd bins, mirroring the three accretion/feedback regimes. Despite not spending much time in the super-Eddington regime, this mode (fEdd > 1) still contributes significantly to increasing the mass of the BH, and dominates the mass growth in the ‘sEddThm’ case.
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