CaRM: Exploring the chromatic Rossiter-McLaughlin effect - The cases of HD 189733b and WASP-127b

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Table E.1.

Reference values for the retrievals, CaRM and PLATON.

	HD189733		WASP-127

Parameter	Value	Source	Value	Source
R_⋆ [R_⊙]		Triaud et al. (2009)	1.303 ± 0.037	Allart et al. (2020)
T_eff [K]	4969 ± 43	Sousa et al. (2018)	5842 ± 14	Allart et al. (2020)
log(g)	4.60 ± 0.01	Sousa et al. (2018)	4.23 ± 0.02	Allart et al. (2020)
[Fe/H] [dex]	−0.07 ± 0.02	Sousa et al. (2018)	−0.19 ± 0.01	Allart et al. (2020)
T₀ [MBJD]		Triaud et al. (2009)	2456776.621238 ± 0.00023181	Seidel et al. (2020b)
P [days]		Triaud et al. (2009)	4.17806203 ± 0.00000088	Seidel et al. (2020b)
a [R_⋆]		Triaud et al. (2009)	7.808 ± 0.109	Seidel et al. (2020b)
λ [°]		Triaud et al. (2009)		Allart et al. (2020)
vsin(i_⋆) [km s⁻¹]	3.05	Triaud et al. (2009)		Allart et al. (2020)
R_p [R_⋆]	0.1581 ± 0.0005	Triaud et al. (2009)	0.10103441 ± 0.00047197	Seidel et al. (2020b)
K [m s⁻¹]		Triaud et al. (2009)	21.51 ± 2.78	Seidel et al. (2020b)
i [°]		Triaud et al. (2009)	87.85 ± 0.35	Seidel et al. (2020b)
σ₀ [km s⁻¹]	3.10 ± 0.01	This work ^(a)	3.146 ± 0.002	This work ^(a)
β₀ [km s⁻¹]	2.518 ± 0.001	This work ^(b)	3.313 ± 0.004	This work ^(b)
ζ_t [km s⁻¹]	4.0	Di Gloria et al. (2015)	3.79 ± 0.05	This work ^(c)

Notes.

^(a)

Computed using the average standard deviation of the Gaussian fit to the out-of-transit measurements.

^(b)

Estimated as described in Santos et al. (2002).

^(c)

Computed with the calibration of Doyle et al. (2014) and valid for stars with T_eff from 5200K to 6400K and log(g) between 4.0 and 4.6.

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