Fig. 12
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Left panel: planet mass distribution of the Ariel MCS analysed in this work divided into planets belonging in single (blue) and multiple (orange) systems. The vertical horizontal line separates the high and low-mass planets at the limit value of 0.2 MJ. Right panel: stellar mass distribution of the Ariel MCS analysed in this work divided into planets belonging in single (blue) and multiple (orange) systems.
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