Fig. A.4.

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Orbital evolution of the bright dwarfs of the VPOS integrating backwards in time for 10 Gyr assuming the MWPotential2014 (Bovy 2015) and taking into account the effects of dynamical friction, assuming that the satellites have all a total mass of MS = 5 × 109 M⊙ (top left), MS = 1010 M⊙ (top right), MS = 5 × 1010 M⊙ (bottom left), and MS = 1011 M⊙ (bottom right); the black solid line in all panels represents the MW virial radius rvir = 245 kpc.
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