Notes. Assumed, adjusted – according to Eq. (11) – fitted parameters and their priors, and derived parameters for our model which fits RVs and transit/occultation mid-times in parallel. The third column indicates if the parameter was fitted to model radial velocity (“RV”) and/or mid-transit and mid-occultation times (“Tr/Occ”). The last column shows the results of our analysis. The offset related to ID 1 (V_instr,1) was not included because the first dataset was used to derive the relative velocity between the observer and the center of mass of the system (V_gamma). The solutions are calculated only from those steps of the DE-MCMC that fall within the distribution around the highest peak of the posterior distribution of (see Fig. 6, solution B). Errorbars are given with 1σ confidence level. The reported values and errorbars of the sidereal period P_s, ω₀ and e are not calculated – as , arctan and respectively – from the reported values of and but from the median of the distribution resulting from the combination of the posterior distributions of and . ^(†)Hellier et al. (2011).