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Table 6

Derived parameters of the atomic lines from the three-night combined transmission spectrum.

Line λ [nm] h [%] Vwind [km s−1] FWHM [km s−1] Rλ [Rp]
Ca II K 393.478 2.283 ± 0.389 8.536 ± 2.528 28.584± 6.144 1.512± 0.145
Ca II K (masked) 1.769 ± 0.372 8.952 ± 3.359 30.705± 8.180 1.413 ± 0.148
Ca II H 396.959 2.410 ± 0.476 −4.201 ± 2.378 23.646 ± 5.713 1.535 ± 0.175
Ca II H (masked) 1.729 ± 0.497 −3.495 ± 3.105 21.294 ± 7.458 1.405± 0.199
Mg I 457.238 ≤0.017 ± 0.035 ≤ 1.005 ± 0.01
Hβ 486.271 ≤0.050 ± 0.010 ≤1.014 ± 0.006
Na I D2(a) 589.158 ≤0.069 ± 0.073 ≤1.019 ± 0.040
Na I D1 589.756 ≤ 0. 067 ± 0.077 ≤1.018 ± 0.043
Hα 656.461 0.341 ± 0.120 −1.786 ± 3.098 18.890 ± 7.109 1.091 ± 0.060
Hα (masked) 0.350 ± 0.14 −3. 025 ± 2. 431 12.899 ± 5.659 1.096 ± 0.072
L II 670.961 0.089± 0.033 4.223 ± 6.167 33.951± 14.425 1.025± 0.018
Li I (masked) 0.080 ± 0.031 5.554 ± 6.514 38.307 ± 15.243 1. 025 ± 0. 017

Notes. The line center wavelength is in vacuum, the depth of absorption line h, the Doppler shift of line center Vwind, line width (FWHM) and the effective planetary radius, Rλ.(a)The Na I D2 measurement is obtained on the transmission spectra generated from only the T2 and T3 data.

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