Fig. 7
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Initial planet location relative to the binary separation, ap,0/abin, vs. final planet mass (top panel) and initial planet location relative to the disc truncation radius, ap,0/Rtrunc, vs. final planet mass (bottom panel) for systems that formed a planet at least more massive than Mars. The colour bar indicates the initial mass of solids in the disc after truncation. The x-axis scale is different in each plot.
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