Notes. A truncated-normal distribution was defined for the priors of periods and masses of the planets as 𝒯 𝒩(µ₀ = µ, ${\sigma }_0^2=s\sigma$, lower_limit=µ-kσ, upper_limit=µ+kσ), where µ and σ are the reported mean and the error of each parameter. The width of the distribution and the truncation limits were defined by setting (s, k) = (2.5,3) and (s, k) = (1,5) for the periods and masses, respectively. No negatives masses were allowed. A half-normal distribution was used for the eccentricities $\text{h}-\mathcal{N}\left({\mu }_0,{\sigma }_0^2\right)$. The time results of the mean TTV models (RMS and maximum amplitude) are also reported.