Table A.1
MCMC results for modeling of the RM effect.
| Parameter | Symbol | Unit | MCMC median | T18 (prior) | L17 |
|---|---|---|---|---|---|
| Scaled semimajor axis | a∕R* | − | 7.50 ± 0.04 | 7.50 ± 0.04 |  |
| Projected obliquity | λ | ° |  |
0.6 ± 4 | 3.4 ± 2.1 |
| Orbit inclination | ip | ° | 86.16 ± 0.5 |  |
 |
| Projected stellar rotation speed | v sin i* | km s−1 |  |
114 ± 3 | 115.9 ± 3.4 |
| RV offset | − | km s−1 | 0.7 ± 3.1 | 0 ± 5* | − |
Notes. The model consists of the four parameters listed in Col. 1, plus a global RV offset. The MCMC median values are listed in Col. 4. Uncertainties correspond to the 16th and 84th percentiles. For comparison, we list literature values in Col. 5, and their references in Col. 6. T18 denotes Talens et al. (2018), and L17 denotes Lund et al. (2017). The asterisk indicates an RV offset prior that is not taken from the literature.
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