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Fig. 6


The mass of synthetic planets (in Jupiter masses) as a function of the initial disk mass for the nominal population (black dots). The dotted line indicates a mass half as high as the initial gas disk mass, showing the linear correlation of disk mass and maximum planet mass for most of the domain. The solid line shows the upper limiting envelope in a non-nominal population where the limiting effect of gap formation on the gas accretion rate is taken into account, using the fit of Veras & Armitage (2004).

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