Fig. 1

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Observed and simulated stellar sample. Top: combined observed stellar mass distribution is composed of different distributions for the HARPS (purple) and CARM70 samples (yellow), respectively. The host star masses in the synthetic NGM population are discrete. By weighted resampling of its systems according to the combined observed sample (red), we obtain a new distribution that approximates it (blue). Bottom: number of observations per stellar mass bin with the same color code as the top figure. Every target star is represented by a white box.
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