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Fig. 10


For each giant planet configuration, mass (top panels), eccentricity (middle panels), and inclination (bottom panels) of the 116 planets formed in our simulations (at 100 Myr) as a function of the semi-major axis. In the three right-hand panels, the additional reference sets of simulations are shown for comparison: no_giants, only_Jupiter, and Solar_System (see text for details).

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