Fig. 5

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Cumulative distribution of aweight for main-belt asteroid analogs in the simulations. The thick black lines represent the aweight distributions for asteroid analogs in all simulations of each model. The solid and dashed blue lines correspond to the aweight distributions for asteroid analogs in a single simulation with ≥10 asteroid analogs and <10 asteroid analogs, respectively. The solid red lines represent the aweight distributions for asteroid analogs in each high-resolution simulation of the classical model.
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