Adaptation of Fig. 21 from Suárez Mascareño et al. (2017), showing minimum mass vs. orbital period for the known planets with determined masses around M dwarf stars (using exoplanet.eu data) divided by the spectral type of the host star. The red filled stars show the positions of HADES planets, the red filled dot shows the position of the planet GJ 625 b, the black asterisk has been added to show the position of Gl 686 b. 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.