Table 4: Data describing the external surviving protoplanets at the end of giant planet migration.
Scenario N $\overline{m}_{{\rm proto}}~({M}_{\oplus})$ $m_{{\rm max}}~({M}_{\oplus})$ $\overline{a}~({\rm AU})$ $a_{{\rm min}}~({\rm AU})$ $a_{{\rm max}}~({\rm AU})$ $\overline{e}$ $e_{{\rm min}}$ $e_{{\rm max}}$ $\overline{i}~\hbox{$^\circ$ }$ $i_{{\rm max}}~\hbox{$^\circ$ }$

I 39 0.11 0.25 5.43 0.45 37.92 0.51 0.15 0.99 8.85 40.45

II 29 0.16 0.74 4.99 0.71 15.25 0.49 0.045 0.91 8.59 35.45

III 33 0.21 0.64 4.68 0.37 12.22 0.46 0.059 0.89 8.32 43.97

IV 31 0.41 2.35 5.16 0.43 8.92 0.50 0.086 0.94 5.81 41.93

V 23 0.57 2.19 6.88 0.49 18.18 0.45 0.079 0.83 3.53 16.24

**Table 4:** Data describing the external surviving protoplanets at the end of giant planet migration.
Scenario	N	$\overline{m}_{{\rm proto}}~({M}_{\oplus})$	$m_{{\rm max}}~({M}_{\oplus})$	$\overline{a}~({\rm AU})$	$a_{{\rm min}}~({\rm AU})$	$a_{{\rm max}}~({\rm AU})$	$\overline{e}$	$e_{{\rm min}}$	$e_{{\rm max}}$	$\overline{i}~\hbox{$^\circ$ }$	$i_{{\rm max}}~\hbox{$^\circ$ }$
I	39	0.11	0.25	5.43	0.45	37.92	0.51	0.15	0.99	8.85	40.45
II	29	0.16	0.74	4.99	0.71	15.25	0.49	0.045	0.91	8.59	35.45
III	33	0.21	0.64	4.68	0.37	12.22	0.46	0.059	0.89	8.32	43.97
IV	31	0.41	2.35	5.16	0.43	8.92	0.50	0.086	0.94	5.81	41.93
V	23	0.57	2.19	6.88	0.49	18.18	0.45	0.079	0.83	3.53	16.24

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