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Table A.1

Median values and 68% confidence intervals for parameters from the pyaneti analysis

Parameter Unit Value
Input stellar parameters

M*…………… (M)… 0.96 ± 0.04
R*…………… (R)… 0.92 ± 0.06
Teff…………… (K)… 5300 ± 100
υrot sin i*…………… (km s−1)… 4.1 ± 1.0
J mag…………… (mag)… 9.40 ± 0.02

Fitted parameters

T0…………… (BJDTDB)…
P…………… (days)…
…………… ()……
…………… ()……
b…………… ()……
a/R*…………… ()……
Rp/R*…………… ()……
K…………… (m s−1)…

Derived parameters

Mp…………… (M)…
Rp…………… (R)…
e…………… ()……
ω…………… (deg)…
i…………… (deg)…
a…………… (AU)…
Depth…………… (ppm)…
RM…………… (m s−1)…
Received irradiance…………… (F)…
Transmission spectroscopy metric1…………… ()……
ρ*2…………… (g cm−3)…
ρ*3…………… (g cm−3)…
ρeq4…………… (K)…
Ttot…………… (hours)…
Tfull…………… (hours)…
ρp…………… (g cm−3
gp5…………… (cm s−2)…
gp6…………… (cm s−2)…
Jeans Escape Parameter7…………… ()……

Other parameters

q1…………… ()……
q2…………… ()……
u1…………… ()……
u2…………… ()……
Sys. vel. TCES…………… (km s−1)…
Sys. vel. Tull…………… (km s−1)…

Comments: 1 - based on the equation from Kempton et al. (2018); 2 - based on the equation from Winn (2010); 3 - from stellar parameters; 4 - based on the equation from Kempton et al. (2018); 5 - from K & Rp/R* 6 - from planetary parameters; 7 - based on the equation from Fossati et al. (2017)

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