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Fig. 3

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Histogram showing the total planetesimal mass that has either been accreted onto the planets, that remains in the system at the end of the simulation, or that has been scattered beyond the simulation domain for all simulations in gas accretion scheme 1 (left) and gas accretion scheme 2 (right). Small planetesimals experience more efficient gas drag than large planetesimals, and they are retained in the system at a higher rate.

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