Fig. 9

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Synthetic populations of planets resulting from the two Monte Carlo runs of 2×105 extractions each with GroMiT. The plot shows the final masses and orbital periods of the simulated growth tracks. The vermilion symbols indicate those planets formed in disks dominated by mm-sized pebbles, while with cactus green we denote cm-sized pebble-dominated disks. Planets b and c are indicated using two larger cyan circles and the boxes around them highlight the region of parameter space populated by the successful solutions.
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