The Rossiter-McLaughlin effect reloaded: Probing the 3D spin-orbit geometry, differential stellar rotation, and the spatially-resolved stellar spectrum of star-planet systems

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Table 1

Fixed parameters for HD 189733.


Parameters	Value	Reference


T₀	2 454 279.436714 ± 0.000015 d	Agol et al. (2010)
P	2.21857567 ± 0.00000015 d	Agol et al. (2010)
i _p	85.710 ± 0.024°	Agol et al. (2010)
R _⋆	0.805 ± 0.016 R_⊙	Boyajian et al. (2015)
R _p	0.15667 ± 0.00012 R_⋆	Sing et al. (2011)
a/R_⋆	8.863 ± 0.020	Agol et al. (2010)
T_dur	1.827 h	Torres et al. (2008)
K	200.56 ± 0.88 m s^-1	Boisse et al. (2009)
e	0
ω	90°
u ₁	0.816 ± 0.019	Sing et al. (2011)
u ₂	0	Sing et al. (2011)
u ₁	0.548	simulation^a
u ₂	0.213	simulation^a
T _eff	4875 ± 43 K	Boyajian et al. (2015)
log g	4.56 ± 0.03	Boyajian et al. (2015)

Notes.

^(a)

The radiative MHD simulations naturally include limb darkening, and as a result these values were obtained by fitting the limb darkening function to the simulated line profiles.

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