Fig. 15.
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Amount of mass accreted over time by MBHs of different initial masses. For the initial 104 M⊙ MBH, the MBH4_SNII is displayed, while for the initial 103 M⊙ and 105 M⊙ MBHs, the MBH3 and MBH5 simulations in the Black Hole Mass subset (see Table 2) are, respectively, shown. Dashed coloured lines indicate the percentage growth of each MBH (with respect to their initial masses).
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