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Table C.1
Posterior estimates for the parameters of the two-planet model from the analysis of CCF and TM RVs. For each parameter we show the MAP estimate and the 68% quantiles of the distribution.
| Np = 2 model | |||
|---|---|---|---|
| Parameter | CCF RVs | TM RVs | Units |
| (adopted) | |||
| Keplerians | |||
| planet b | |||
| P |  |
 |
days |
| K |  |
 |
m s−1 |
| M0 |  |
 |
|
| e |  |
 |
|
| ω |  |
 |
|
| Mp sin i |  |
 |
M⊕ |
| a |  |
 |
au |
| planet d | |||
| P |  |
 |
days |
| K |  |
 |
m s−1 |
| M0 |  |
 |
|
| e |  |
 |
|
| ω |  |
 |
|
| Mp sin i |  |
 |
M⊕ |
| a |  |
 |
au |
| GP | |||
| η1 RV |  |
 |
m s−1 |
| η1 FWHM |  |
 |
m s−1 |
| η2 |  |
 |
days |
| η3 |  |
 |
days |
| η4 |  |
 |
|
| noise | |||
 |
 |
 |
m s−1 |
 |
 |
 |
m s−1 |
 |
 |
 |
m s−1 |
 |
 |
 |
m s−1 |
 |
 |
 |
m s−1 |
 |
 |
 |
m s−1 |
| background | |||
| RV slope |  |
 |
m s−1yr−1 |
| RV quadr |  |
 |
m s−1yr−2 |
| RV offset ESP18-ESP21 |  |
 |
m s−1 |
| RV offset ESP19-ESP21 |  |
 |
m s−1 |
| FWHM offset ESP18-ESP21 |  |
 |
m s−1 |
| FWHM offset ESP19-ESP21 |  |
 |
m s−1 |
| vsys |  |
 |
m s−1 |
| fsys |  |
 |
m s−1 |
Notes. Planet minimum masses and semi-major axes were derived assuming the stellar mass given in Table 1.
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