HD 110067 c has an aligned orbit - Measuring the Rossiter–McLaughlin effect inside a resonant multi-planet system with ESPRESSO

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Table 3.

MCMC analysis results.

Parameter	Prior	Result
T_c − 2 460 000 (d)	𝒩(T₀ ± 0.01)	354.8018 $_{- 0.0022}^{+ 0.0020}$ $^{+0.0020}_{-0.0022}$
λ (deg)	𝒰(−180, 180)	6 $_{- 26}^{+ 24}$ $^{+24}_{-26}$
v sin i_* (km s⁻¹)	𝒰(0, 5)	1.39 $_{- 0.19}^{+ 0.26}$ $^{+0.26}_{-0.19}$
R_p/R_s	𝒩(0.0278, 0.0003)	0.0278 ± 0.0003
a/R_s	𝒩(28.37, 0.30)	28.52 $_{- 0.30}^{+ 0.29}$ $^{+0.29}_{-0.30}$
i (deg)	𝒩(89.687, 0.163)	89.64 $_{- 0.17}^{+ 0.19}$ $^{+0.19}_{-0.17}$
γ (km s⁻¹)	𝒰(−8.48, −8.58)	−8.5306 ± 0.0001
K (km s⁻¹)	𝒰(−0.02, 0.02)	−0.001 ± 0.003

Notes. 𝒩 denotes priors with a normal distribution and 𝒰 priors with a uniform distribution.

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