Same as Fig. 6 (right), but illustrating the possible outcomes given lacking velocity measurements. The colored stars show the possible axis ratios and fractions of corotation in the data. The flatness of the structure will not change with new velocity information because distance measurements are available for all dwarfs. The fractions of corotation can vary from 0.5 (15/30) to 0.76 (23/30). For each possible scenario, the fraction of simulated systems that match or exceed the degree of kinematic correlation is shown in the histogram to the right. The fractions of systems that show both flatness and a degree of corotation similar to or more extreme than the data are shown in the center.