Posterior distributions of the classical seven orbital elements, plus the (fitted) orbital parallax, together with the Gaia DR2 trigonometric parallax and its ±1σ error, the systemic velocity, the velocity amplitudes for both components, the mass sum, the mass ratio, and the individual component masses. The cut on the lower end of the V_CoM histogram is a consequence of the fact that we discard solutions with m_S/m_P > 1. However, the method still provides a good estimate of the orbit and the distribution of orbital parameters.