Sinkmass spectra for models A1, B1, C1, and D1 at various time steps, corresponding to a comparable amount of accreted mass. Various spatial resolutions are explored for the purpose of verifying numerical convergence and direct comparison between models. For models B1, C1, and D1, a peak at ≃ 0.1 M_⊙ is obtained independently of the numerical resolution. While model A1 presents a flat mass spectrum, models C1 and D1 present at high mass a power-law behavior that is compatible with M^−3∕4 (see also Fig. 8).