The remaining posteriors of the dynamical properties of the best-fit dynamical model that are not displayed in the main text. The two-dimensional contours indicate 1-, 2- and 3-σ confidence levels of the posterior distribution. The red crosses indicate the median of the posterior probability distribution. Top to bottom and left to right: The RV offsets of CARMENES, HIRES and HARPS, respectively, the RV jitter, as well as the mean semi-amplitude K, mean argument of periapsis ω, the mean anomaly MA of each planet and the GP rotational kernel amplitude, time scale, period, and factor.