Fig. 21
Minimum mass vs. orbital period for the known planets with determined masses around M-dwarf stars (using data from exoplanet.eu) divided by the spectral type of the host star. The red filled dot shows the position of GJ 625 b, and the red filled stars show the position of GJ 3998 b, c and GJ 3942 b (Affer et al. 2016; Perger et al. 2017b). The horizontal dashed lines show the mass of the solar system planets for comparison. The distribution for each parameter is shown at the edges of the figure.
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