Amount of mass accreted over time for an initial 10⁴ M_⊙ MBH (orange lines) with and without uniformly reducing the angular momentum of the gas in the low-mass dwarf galaxy by 20 and 50% (MBH4_L20 and MBH4_L50 in Table 2, respectively). No ISR feedback is considered. The simulation of an initial 10⁴ M_⊙ MBH with L_reduce = 0% corresponds to the MBH4_SNII simulation (see Table 2). A pair of simulations of an initial 10⁶ M_⊙ MBH (green lines) with and without L_reduce = 20% is also conducted (MBH6_L20 and MBH6 in Table 2, respectively).