Fig. 1
Frequency of Rp used in the two simulation runs, which shows the shape of the planetary radius distribution used in the simulations. Left: from simulation run # 229 using a polar-biased starspot distribution of a M dwarf host star with a starspot filling factor of 4.0% ± 1.0%. Right: from simulation run # 807 using a mid-latitude starspot distribution of a K dwarf host star with a starspot filling factor of 0.3% ± 0.1%.
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