Our VMP MSS member candidates projected along the Magellanic stream coordinates (panel 1), proper motions along and transverse to the stream (panels 2 and 3), heliocentric distance (panel 4), along projected stream coordinates with their transverse motion highlighted using velocity vectors (panel 5), and line-of-sight radial velocity (where available, from PGS 6D giants, panel 6). All the parameters are plotted against the Magellanic stream longitude. The projection includes particles from both tidal debris models in Besla et al. (2012), LMC, SMC parameters adapted from Kallivayalil et al. (2006a,b), and the Magellanic stellar stream debris discovered by Chandra et al. (2023a).