Fig. C.1

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Snapshots of orbital integration around an eccentric giant planet. The left and right columns show the eccentricity and inclination, respectively, with the semi-major axis of planetesimals. Time progresses from upper to lower panels. The solid lines in the left column show efall. The small boxes on the right side of each panel show the histogram. The total number of planetesimals N is written in the boxes. Here, we show the case with ap = 1 au, ep = 0.99, sin ip = 0, Mp = MJup and Rp = RJup.
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