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Fig. 7


Relative difference between the cumulative distributes of the masses of the bound planets initially and at 11 Myr. Positive values indicate an overabundance at the end of the simulation. Initially, the mean planet mass is 1.398 ± 1.05 MJup at 11 Myr the mean mass is only fractionally different at 1.404 ± 4.191 MJup; the latter value is indicated by the vertical green line.

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