Table 1
Planet orbital and stellar parameters used to calculate the Rossiter-McLaughlin (RM) effect with the AROME code (Boué et al. 2013).
| Parameter | Value | Units | Reference |
|
|
|||
| a | 0.03120 | au | Triaud et al. (2009) |
| Rstar | 0.766 | R⊙ | Triaud et al. (2009) |
| i | 85.508 | deg | Triaud et al. (2009) |
| λ | −0.85 | deg | Triaud et al. (2009) |
| Vsin(i) | 3.10 | km s-1 | Triaud et al. (2009) |
| β0 | 1.3 | km s-1 | − |
| σ0 | 3.3 | km s-1 | − |
| z | 4.0 | km s-1 | − |
| P | 2.218573 | days | Triaud et al. (2009) |
Notes. The orbital planetary and stellar parameters are taken from Triaud et al. (2009). The remaining parameters, i.e. the line width of the non-rotating star β0, the sigma of the Gaussian fit to the CCF σ0, and the macro-turbulence parameter z, were estimated by us and only have a marginal effect on the resulting RM anomaly.
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