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Table 1

Nature of the discard events of planetesimals and embryos.

Accreted Final inner Remaining mass
Index by giants Ejected eccentricity in M
or the star (min-max) (max)
2_01 51.9% 48.1% 0.228 (0.132-0.291) 0.033 (0.055)
2_02 44.3% 55.7% 0.143 (0.034-0.196) 0.061 (0.115)
2_03 43.6% 56.4% 0.385 (0.186-0.528) 0.110 (0.285)
2_04 82.6% 17.4% 0.430 (0.311-0.553) 0.000
2_05 57.9% 42.1% 0.070 (0.026-0.194) 0.183 (0.168)
2_06 65.5% 34.5% 0.406 (0.203-0.716) 0.0003
3_01 47.0% 53.0% 0.410 (0.087-0.855) 0.000
3_02 43.2% 56.8% 0.434 (0.186-0.784) 0.009 (0.580)
3_03 90.9% 9.1% 0.329 (0.081-0.823) 0.101 (0.313)
2_07 37.0% 63.0% 0.155 (0.077-0.279) 1.348 (0.925)
2_08 8.8% 91.2% 0.105 (0.041-0.186) 1.851 (1.180)
2_09 22.2% 77.8% 0.160 (0.064-0.384) 1.626 (1.283)
3_04 51.8% 48.2% 0.331 (0.139-0.774) 0.023 (0.198)
3_05 33.1% 66.9% 0.233 (0.097-0.569) 0.099 (0.688)

Notes. For the nine runs per configuration (index in the first column), the average percentage of collisions with a giant or the star is given in the second column and that of ejections in the third column. The fourth column shows the average final eccentricity of the innermost giant planet for the nine runs per configuration, while the minimum and maximum values are given in brackets. The last column indicates the average remaining mass (in M) of the terrestrial disc after 100 Myr, while the maximum mass of the formed terrestrial planets in each set is indicated in brackets.

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