Fig. C.1
Final configuration of planetary systems after 8 Myr of integration using αmig = 0.0001 and a pebblescale height calculated with α = 0.0001. Planets migrating interior to 1 AU are removed from the simulations. We only show planets with masses larger than 0.3ME. The numbers in front show the pebble accretion efficiency of the whole system in percent.
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