Fig. 8
Mass-period diagram of all super-Earth planets, with masses determined from RVs or TTVs, orbiting mid- and late-type M dwarfs (left panel) and for all M dwarfs (right panel) taken from the NASA Exoplanet Archive from May 2018 (https://exoplanetarchive.ipac.caltech.edu). Single- and multi-planet systems are drawn with circles and triangles, respectively.The colorbar indicates the effective temperature of the host star.
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