Table 11
Best-fitted solution for the planetary system orbiting HD 134060.
| Param. | Units | HD134060b | HD134060c |
|---|---|---|---|
| P | (d) | 3.2696 |
1291.5646 |
| K | (m s−1) | 4.61 |
1.65 |
| e | 0.45 |
0.11 |
|
| ω | (deg) | −98.23 |
−132.73 |
| TP | (d) | 55499.6542 |
55232.8160 |
| TC | (d) | 55498.1943 |
56057.2704 |
| Ar | (AU) | 0.0444 |
2.3928 |
| M. sini | (MJup) | 0.0318 |
0.0922 |
| M. sini | (MEarth) | 10.10 |
29.29 |
| γHARPS | (m s−1) | 37987.9484 |
|
| σ(O−C) | (m s−1) | 1.64 | |
| log(Post) | −304.2166 |
||
Notes. For each parameter, the median of the posterior distribution is considered, with error bars computed from the MCMC posteriors using a 68.3 % confidence interval. The value σ(O−C) corresponds to the weighted standard deviation of the residuals around the best solution. All the parameters probed by the MCMC can be found in Table B.8. See Table 4 for definition of the parameters.
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