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Table 3

Results from our MCMC analysis.

Parameter TOI-1820 TOI-2025 TOI-2158
P Period (days) 4.860674 ± 0.000005 8.872078 ± 0.000007 8.60077 ± 0.00003
T0 Mid-transit time (BJD) 2458903.0638 ± 0.0006 2458690.2898 ± 0.0004
Rp/R* Planet-to-star radius ratio 0.0777 ± 0.0009 0.0736 ± 0.0004 0.0700 ± 0.0009
a/R* Semi-major axis to star radius ratio 8.7 ± 0.3
K Velocity semi-amplitude (m s−1) 273 ± 4 396 ± 10 75 ± 4
cos i Cosine of inclination 0.097 ± 0.005
0.20 ± 0.02
0.643 ± 0.016
γ1 Systemic velocity FIES (m s−1) -383 ± 19 13 ± 9
γ2 Systemic velocity FIES+ (m s−1)
γ3 Systemic velocity Tull (m s−1) 13947 ± 4
σ1 Jitter FIES (m s−1)
σ2 Jitter FIES+ (m s−1) 19 ± 6
σ3 Jitter Tull (m s−1)
log A1 GP amplitude TESS 30 min. −8.30 ± 0.06
log τ1 GP timescale TESS 30 min. (log days)
log A2 GP amplitude TESS 2 min.
log τ2 GP timescale TESS 2 min (log days) −1.03 ± 0.14
(a,b) Quadratic trend (m s−1 d−2) −0.0015 ± 0.0003 −0.0020 ± 0.0003
(a,b) Linear trend (m s−1 d−1) 1.4 ± 0.2
δMI Dilution I-band/TESS
δMB Dilution B-band
λ Projected obliquity (°)
v sin i* Projected rotational velocity (km s−1) 6.0 ± 0.3
ζ Macro-turbulence (km s−1) 4 ± 1
ξ Micro-turbulence (km s−1)

e Eccentricity 0.043 ± 0.008 0.41 ± 0.02 <0.070 at 3σ(c)
ω Argument of periastron (°) 93 ± 2
i Inclination (°) 84.4 ± 0.3
b Impact parameter
T4,1 Total transit duration (hours) 2.92 ± 0.04
T2,1 Time from 1st to 2nd contact (hours) 0.61 ± 0.05 0.75 ± 0.07
Rp Planet radius (RJ) 1.14 ± 0.02 1.117 ± 0.009 0.960 ± 0.012
Mp(d) Planet mass (MJ) 2.3 ± 0.2 4.4 ± 0.3 0.82 ± 0.08
ρp Planet density (g cm−3) 2.0 ± 0.2 3.9 ± 0.3 1.14 ± 0.12
Teq(e) Equilibrium temperature (K)(c) 1375 ± 12 1167 ± 11 1188 ± 10
a Semi-major axis (AU) 0.061 ± 0.003 0.092 ± 0.004 0.075 ± 0.004

Notes. The parameters above the dashed line are the stepping parameters, and below are the derived parameters. The value given is the median and the uncertainty is the highest posterior density at a confidence level of 0.68. (a)Zero-point for TOI-2158 is 2459302.92570 BJDTDB.(b)Zero-point for TOI-2025 is 2459124.41436 BJDtdb. (c)Two-sided 1σ distribution . (d)Calculated from Eq. (2). (e)Following Kempton et al. (2018).

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