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Fig. 10

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Final position of the planets in the distance-mass diagram. Three different syntheses are shown. Blue, up-facing triangles show the reference synthesis. The other two population calculations are made with the migration model of Paardekooper et al. (2011). Red, left-facing triangles represent planets obtained with this model and the adiabatic coefficient γ calculated by our EOS. Green, right-facing triangles show the aM positions obtained with the Paardekooper et al. (2011) model with a fixed γ = 1.4.

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