Orbital evolution for the proposed group integrating backwards in time for 6 Gyr for the mutual separation of the objects in relation to Leo II using both the MW-only potential and the MW+LMC potential. The thick lines indicate their most likely orbit from the measured proper motions and the thinner lines represent 100 Monte-Carlo realisations within their uncertainties. The black solid lines represent the orbital evolution obtained using the predicted proper motions for each object. The dashed lines represent the mean orbital evolution obtained using only the bound orbits.