Orbit of HIP 99770 b relative to its host, i.e., fixed at the origin. The visualised orbits were generated from a random subset of 100 parameter sets drawn from the posterior sampling. While the previously available astrometric epochs obtained by SCExAO/CHARIS and Keck/NIRC2 are shown along with their respective uncertainties in ΔRA and ΔDec, knowledge of the correlation coefficient, ρ, allowed us to visualise the VLTI/GRAVITY epoch as a 1 σ confidence ellipse.