Results of the MCMC fit of the NaCo and SPHERE combined astrometric data of HD 95086 b 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. The reported solutions correspond for the restricted case of orbits with inclination i and longitudes of ascending nodes Ω that ensure a tilt angle with the outer belt resolved with ALMA (i = 150°, Ω = 97°, Su et al. 2017) less than 5°.