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Fig. C.1
Comparison of the resulting LX–a-distributions using different values for the planetary accretion efficiency. Top panel: default model using Eq. (C.1), while in the other two models, it was set to a constant value of ϵ∕ϵmax= 1.0 (centre) and ϵ∕ϵmax = 0.3 (bottom). The colour-coding represents the planet mass.
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