Fig. 10
Cumulative distributions of a number of planets per system for giant planets (≥0.1 MJ, top panel), and Es/SEs (0.1 ME−0.1 MJ, bottom panel). The blue, orange, and red correspond to the stellar metallicities of [Fe/H] = 0.5, 0.0, and –0.5, respectively. The fractions of planetary systems with zero planets decrease with stellar metallicities both for giant planets and Es/SEs.
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