Table C.1
Summary of posteriors obtained with our MCMC algorithm for known planets.
| Parameter | HD 16905 b | HD28254 b | HD44219 b* | HD62364 Β | HD89839 b | HD 100777 b* | HD111998b* | HD 114783 c | HD 140901 b |
|---|---|---|---|---|---|---|---|---|---|
| a (au) |  |
 |
 |
6.4 ±0.1 | 4.9 ±0.1 |  |
 |
5.0 ± 0.1 |  |
| Ρ (days) |  |
1333 ± 4 |  |
5172 ±30 | 3448 ± 26 | 383 ± 1 |  |
 |
 |
| Ecc |  |
 |
 |
 |
0.20 ± 0.02 | 0.38 ± 0.02 |  |
 |
 |
| I (°) | 43 ± 3 or 136 ± 3 |  |
fix to 90 | 42 ±2 or 131 ±2 |  |
fix to 90 | fix to 90 |  |
 |
| Mass (MJup) |  |
 |
 |
 |
5.2 ±0.8 | 1.23 ±0.05 (< 18.0) | 4.8 ± 0.2 (< 12.8) |  |
1.8 ±0.5 |
| Ω (°) |  |
 |
fix to 0 | 136 ± 3 or 273 ± 5 |  |
fix to 0 | fix to 0 |  |
 |
| ω (°) | 248 ± 1 |  |
 |
0± 1 |  |
 |
 |
 |
 |
| Ρtime | 1856 ±8 |  |
 |
3570 ± 5 |  |
224 ±3 |  |
 |
 |
 |
−0.31 ± 0.02 |  |
 |
0.778 ± 0.003 |  |
-0.56 ± 0.02 |  |
 |
 |
 |
−0.766 ± 0.007 |  |
 |
 |
 |
 |
 |
 |
 |
| Jitter (m s−1) |  |
 |
 |
 |
4.3 ± 0.4 | 2.4 ± 0.4 | 18.7 ± 1.2 |  |
9.2 ±0.3 |
| rms (m s−1) |  |
 |
10.8 ±0.3 |  |
 |
2.6 ± 0.02 |  |
3.9 ±0.1 |  |
| H03 = 64804 ± 2 | H03 = −9324 ± 1 |  |
H03 = 35510 ± 1 | H03 = 31758 ± 1 | H03 = 1250 ± 1 | H03 = −3 ± 3 | H03 = 0 ± 1 | H03 = −6701 ± 2 | |
| Instrumental | H15 = 64817 ± 1 |  |
 |
H15 = 35525 ±2 |  |
 |
AAT = −3 ± 1 | ||
| offset (m s−1) | HRS = 0 ± 1 | PFS = −6 ± 2 | |||||||
| Hir94 = 0 ± 1 | |||||||||
| Hir04 = 0 ± 1 | |||||||||
Notes: The median and 1σ confidence interval are given for each parameter. * corresponds to the solutions found considering only the RV data points. The reported masses are therefore the minimum masses. In these cases, the maximum value of the true mass of the companions, estimated with Gaston, with a confidence index of 3σ, are noted between parentheses.
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