Cumulative mass profiles: We display the cumulative mass profiles at the last snapshot of our simulations, for the dark matter particles (black), their embedded stellar component (green) and the stellar component from the simulations without dark matter (dashed red). The blue line depicts the MCMC fit of a Zhao (1996)αβγ model to the dark matter mini-halo (see Sect. 4.2.2), with a fainter blue region encompassing the [2.5, 97.5] percentiles. The dotted lines represent local slopes of the stellar mass distribution at the respective regions shown in the plot.