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Table 5

PyTTV model parameters and priors.

Description Units Prior
Stellar parameters

Stellar mass (M) 𝒩 (1.447,0.077)
Stellar radius (R) 𝒩 (1.698,0.060)
Limb darkening q1(a)${{\rm{q}}_1^{(a)}}$ (–) 𝒰 (0, 1)
Limb darkening q2(a)${{\rm{q}}_2^{(a)}}$ (–) 𝒰 (0, 1)
Planet b parameters

log10 mass (log10 M) 𝒰 (−2.8,−2.l)
Radius ratio (R) 𝒩 (0.08,0.001)
Transit centre (BJD) 𝒩 (2459 378.46,0.02)
Orbital period (d) 𝒩 (0.67247414, 0.005)
Impact parameter (R) 𝒩 (0.75,0.01)
e$\sqrt e $ cos ω () 𝒰(−0.25,0.25)
e$\sqrt e $ sin ω () 𝒰(−0.25,0.25)
Ω (rad) N(π, 0.0001)
Planet c parameters

logio mass (log10 M) 𝒰(−5.2, −3.0)
Radius ratio (R) 𝒩(0.05, 0.0001)
Mean anomaly at Tref (rad) 𝒰(0, 2π)
Orbital period (d) Depends on the scenario
Impact parameter (R) 𝒰(1.0,3.0)
e$\sqrt e $ cos ω (–) 𝒰(−0.25, 0.25)
e$\sqrt e $ sin ω (–) 𝒰(−0.25, 0.25)
Ω (rad) N(π, 0.0001)
RV parameters

Linear trend (m/s/d) 𝒩 (−0, 1.0)
Systemic velocity 1 (m/s) 𝒩 (−25 855,200)
Systemic velocity 2 (m/s) 𝒩 (−25 416,200)
log10 jitter 1 (log10 m/s) 𝒩 (−1,0.1)
log10 jitter 2 (log10 m/s) 𝒩 (−1,0.1)
Additional priors

Both eccentricities 𝒩 (0.0, 0.023)

Notes. All the planetary parameters except the radius ratio and log10 mass are defined at a reference time, tref = 2459 378.46. (a)We use the triangular parametrisation for quadratic limb darkening introduced by Kipping (2013).

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