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Fig. A.5.

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As in Fig. A.4, but here showing the impact of uncertainties on the orbital evolution of the individual systems. For each galaxy, we show as grey lines 100 realisations made by a Monte-Carlo sampling of the position and velocity vector, taking into account errors on distance, proper motion and radial velocity. We show results assuming that the satellites have a total mass of MS = 5 × 109M (left panels) and MS = 5 × 1010M (right panels); the black solid line in all panels represents the MW virial radius rvir = 245 kpc.

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