The Rossiter–McLaughlin effect revolutions: an ultra-short period planet and a warm mini-Neptune on perpendicular orbits

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Table 2

Out-of-transit CCF_DI properties.

Instrument	HARPS-N		ESPRESSO

Mask	Classic	Custom	Classic	Custom
⟨Contrast⟩ (%)	65.936	56.694	66.569	55.238
e_Contrast (%)	0.016	0.015	0.015	0.014
σ_Contrast (%)	0.025	0.020	0.027	0.015
(ppm)	382	360	407	268

⟨FWHM⟩ (km s⁻¹)	8.1129	6.4130	7.7244	6.1144
e_FWHM (m s⁻¹)	2.0	1.7	1.8	1.6
σ_FWHM (m s⁻¹)	3.5	2.1	3.2	2.2
(ppm)	435	322	410	365

e_RV (cm s⁻¹)	99	83	88	80
σ_RV (cm s⁻¹)	109	72	111	83

Notes. σ indicates standard deviations of the contrast, FWHM, and Keplerian RV residuals with respect to their mean out-of-transit value (⟨ x⟩). The σ^rel dispersions have been normalized by this mean to allow for a direct comparison between masks. e_x indicate the mean out-of-transit error on x.

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