Correlation maps of the posterior probability following the Bayesian analysis of the orbit of HIP 93511: (top, left) The argument of the periastron (ω) vs. the longitude of the ascending nodes (Ω), (top, right) the semi-major axis a vs. the eccentricity e, (bottom, left) the orbital period T₀ vs. the semi-major axis a, (bottom, right) the orbital period T₀ vs. the periastron passage T₁.