Table 1
Overview of population syntheses.
| R | E20 | E5 | ND | RD | RA | RI | |
|
|
|||||||
| Initial ne | 10 | 20 | 5 | 10 | 10 | 10 | 10 |
| n sys | 344 | 228 | 483 | 264 | 343 | 344 | 413 |
| Initial np | 2834 | 3241 | 2171 | 1686 | 2480 | 2834 | 3309 |
| Final np | 2519 | 2238 | 2129 | 1236 | 2155 | 2389 | 2921 |
| Initial np at 10 m s-1 | 206 | 160 | 241 | 143 | 217 | 206 | 253 |
| Final np at 10 m s-1 | 204 | 153 | 237 | 132 | 191 | 202 | 244 |
| n coll | 282 | 902 | 000 | 318 | 225 | 378 | 329 |
| n eje | 22 | 84 | 000 | 112 | 86 | 48 | 45 |
Notes. The parameter ne denotes the number of embryo seeds, nsys the number of systems, np (resp. np at 10 m s-1) the number of planets (resp. with a radial-velocity semiamplitude K ≥ 10 m s-1), and ncoll and neje the number of planets removed due to collisions and ejections. The population designations refer to the reference population with ten embryos and full damping (R), the population with 5 and 20 embryos (E5, E20), the population with no (ND) and reduced eccentricity and inclination damping (RD), and the population with a stochastic perturbation to the semimajor axes (RA) or to the inclinations (RI).
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