Notes. The global parameters are independent of the passband or light curve, the passband-dependent parameters are repeated for each passband, and the light-curve-dependent parameters are repeated for each separate light curve. Ν(μ, σ) stands for a normal prior with a mean μ and standard deviation σ, 4U(a, b) stands for a uniform distribution from a to b, and ‘Cont. temperature’ stands for the effective temperature of the contaminating star. ^(a)The zero epoch is given a normal prior N(2459255.694, 0.015) and the period is given a normal prior N(2.3262, 0.0002). ^(b)The TESS transits are given a separate apparent radius ratio that effectively makes the TESS contamination independent of the contamination in the ground-based observations. ^(c)The limb darkening coefficients correspond to the transformed power-2 limb darkening law coefficients (Maxted 2018) and have normal priors calculated using LDTK. ^(d)The average log10 white noise parameters for each light curve have uninformative uniform priors. ^(e)The linear baseline model coefficients have loose normal priors based on the light curve variability. We do not write them here explicitly, but they can be found from the 02_joint_analysis.ipynb notebook in the project's GitHub repository.