Table 1
Synthetic planet population NGM.
| Name | M* |  |
Nemb,ini | Simulated systems | Sampling weights | Resampled systems |
|---|---|---|---|---|---|---|
| NGM10 | 0.1 M⊙ | 2811K | 50 | 1000 | 0.204 | 21 392 |
| NGM14 | 0.3 M⊙ | 3416K | 50 | 997 | 0.368 | 34 768 |
| NGM11 | 0.5 M⊙ | 3682K | 50 | 1000 | 0.388 | 39 862 |
| NGM12 | 0.7 M⊙ | 4430K | 50 | 999 | 0.039 | 3978 |
| NG75(b) | 1.0 M⊙ | 5731 K | 50 | 1000 | 0 | 0 |
Notes. Each of the simulated systems started with Nemb,ini = 50 planetary seeds. Five stellar masses and corresponding effective temperatures were sampled with different weights to match the observed distribution, and a total of 100 000 systems were drawn. Each system was assigned a random, isotropic inclination angle i. The population NG75 extends NGM to solar-type stars (see Emsenhuber et al. 2021b; Burn et al. 2021) but did not have to be sampled to match the M* distribution of the observed sample. Table adapted from Burn et al. (2021).(a)Following Baraffe et al. (2015). (b)Population also discussed in Emsenhuber et al. (2021b).
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