Fig. 15
Minimum mass vs. orbital period diagram for known Neptune-type and super-Earth planets (colored dots) around M dwarfs only detected with RV method (available data at http://www.exoplanet.eu). The light blue star indicates the locationof the planet GJ 720 Ab. The color-coding divides the sample by the spectral type of the host star with − 2.0, 0.0, and 7.0 corresponding to K5.0V, M0.0V, and M7.0V, respectively.
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