Evolution of the SFR after 160 Myr for the simulations with accretion capped at the Eddington limit (‘EddLim’ – dotted blue) and above the Eddington limit with (‘sEdd’ – solid orange) and without (‘sEddThm’ – densely dash-dotted violet) kinetic feedback starting at 206.4 Myr (orange/violet filled semi-circles). The SFR does not decrease below 10 M_⊙ yr⁻¹ after the BH was added, even in the case of the super-Eddington feedback. The difference between the runs is small, showing that AGN feedback does not majorly impact the SFR in this particular setup.