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Table B.2

Posterior values for all fitting parameters in our MCMC.

Parameter Unit Prior Value
Orbital period, P d U 4.72018440.0000012+0.0000011Mathematical equation: $4.7201844^{+0.0000011}_{-0.0000012}$
Mid-transit time, T0 BJDTDB U 2458913.37210.0003+0.0002Mathematical equation: $2458913.3721^{+0.0002}_{-0.0003}$
Scaled semi-major axis, a/R U 8.280.12+0.25Mathematical equation: $8.28^{+0.25}_{-0.12}$
Planet-to-star radius ratio, Rp/R U 0.07260.0004+0.0003Mathematical equation: $0.0726^{+0.0003}_{-0.0004}$
Cosine of orbital inclination, cos io U 0.0290.013+0.014Mathematical equation: $0.029^{+0.014}_{-0.013}$
Projected obliquity, λ ° U −5 ± 10
Projected rotational velocity, v sin i km s-1 N(14.2,0.5) 14.4 ± 0.5
Macro-turbulence, ζ km s-1 N(5.68,0.5) 5.7 ± 0.5
Micro-turbulence, ξ km s-1 N(1.36,0.5) 1.4 ± 0.5
Velocity semi-amplitude, K m s-1 U 262 ± 24
Systemic velocity, Γ m s-1 U 6 ± 3
RV jitter, σ m s-1 J 0.0060.006+0.058Mathematical equation: $0.006^{+0.058}_{-0.006}$
Sum of LD coefficients TESS, (q1 + q2)TESS N(0.5432,0.1) 0.540.09+0.10Mathematical equation: $0.54^{+0.10}_{-0.09}$
Difference in LD coefficients TESS, (q1-q2)TESS F(-0.074) ...
Sum of LD coefficients FIES, (q1 + q2)FIES N(0.706,0.1) 0.71 ±0.10
Difference in LD coefficients FIES, (q1 - q2)FIES F(0.2814) ...
Eccentricity, e F(0) ...

Notes. U (J) denotes a uniform (Jeffrey’s) prior. N(a, b) means that a Gaussian prior was applied with μ = a and σ = b. F(c) means that this value was fixed to c.

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