Results of the MCMC fit of the NaCo and GPI combined astrometric data of HD 95086 b. Measurements are directly taken from Table 1 of Rameau et al. (2016). The results are reported in terms of statistical distribution matrix of the orbital elements a, e, i, Ω, ω and t_p. The red line indicates the position of the best LSLM model obtained for comparison. Considering the new distance estimate of 83.8 pc, a correction factor of 0.93 in sma and 0.89 in period must be applied for direct comparison with Fig. 3 of Rameau et al. (2016). The MCMC tool used in this workand the MCMC OFTI tool of Blunt et al. (2017) show a relatively good match confirming both MCMC methods.