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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