Open Access
Table 2
Average number of planets with masses larger than 0.5 Jupiter masses at the end of our simulations at 100 Myr with different K damping values and initial number of planets (seeds) that are detectable by RV measurements with 1 m s−1 up to a distance of 5.2 AU.
| K | 15 seeds | 30 seeds | 60 seeds | 30 seeds, Speb = 5.0 |
|---|---|---|---|---|
| 5 | 1.64 ± 0.85 | 1.00 ± 0.90 | 1.16 ± 1.04 | 0.78 ± 0.84 |
| 50 | 1.56 ± 1.01 | 1.30 ± 0.93 | 1.38 ± 1.11 | 1.60 ± 0.93 |
| 500 | 1.62 ± 1.01 | 2.02 ± 1.20 | 2.30 ± 1.28 | 2.78 ± 0.95 |
| 5000 | 1.50 ± 1.09 | 1.74 ± 1.23 | 1.48 ± 1.33 | 2.42 ± 1.25 |
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