Table 9
Posterior values of all parameters used for HD 154088.
| HD 154088 | ||||
|---|---|---|---|---|
| Parameter | Units | |||
| Offset and drift | ||||
| γH03 | m s−1 | 14 298.12 ± 0.16 | ||
| A (†) | m s−1 | 2.46 ± 0.31 | ||
| Noise | ||||
| σH03 | m s−1 | 1.60 ± 0.09 | ||
| σ(O−C) | m s−1 | 1.3 | ||
| Keplerians | ||||
| HD 154088 b | ||||
| P | day | 18.56 ± 0.01 | ||
| K | m s−1 | 1.7 ± 0.2 | ||
| e | <0.193; <0.344 (‡) | |||
| ω | deg | –(‡) | ||
| λ0 | deg | 239 ± 6 | ||
| TPeriastron | BJD | 2 455 498.2 ± 3.5 | ||
| m sini | M⊕ | 6.6 ± 0.8 | ||
| a | AU | 0.134 ± 0.002 | ||
| Ref. Epoch | BJD | 2 455 500 | ||
Notes. We give the values of the mode and the 1σ confidence interval of the posterior distribution from the MCMC. (†) Linear parameter fitted to 
with a Gaussian kernel at a 0.5 yr timescale. (‡)Eccentricity does not differ significantly from zero; the 68 and 95% upper limits are reported. The argument of periastron
ω is therefore unconstrained.
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