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Fig. 25
Confirmed exoplanets around M-dwarf host stars, detected with the RV method and with minimum masses below 10 M⊕ and orbital periods between 1 d and 400 d. The color-coding represents the spectral type. GJ 251 b, HD 238090 b, and Lalande 21185 b are marked in red. Data taken from http://exoplanet.eu
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