Projected Ω vs. i traces determined via Monte Carlo sampling over a flat distribution in radial velocity for all stars that have a subset of solutions that corresponds to at least one of the known GC disk features using only a single sign for the z coordinate. The features are shown here by ellipses (see, e.g., Bartko et al. 2009; Yelda et al. 2014; vF22). Disk features are as calculated for Fig. 7 of vF22. The color of the trace indicates the 3D position vector of the source given by . This illustrates that the stars with the lowest r_3D appear on the CW disk. This is consistent with the findings of vF22.