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Fig. B.2.

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Example of calculation of infall time for Auriga simulations. Blue points and dash lines indicate the distance of subhalos 1 (top panel) and 1749 (bottom) from Auriga MW-like Level 3 resolution Halo 27 to the main host galaxy center. Red points and lines indicate the evolution of the virial radius (R200m) of the main host galaxy at different epochs using the linear relation in Fig B.1. Vertical red dashed lines indicate the last infall time of the subhalo.

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