Fig. 14
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Mass-radius diagram of exoplanets with an accurate mass and radius determination from the updated version of Otegi et al. (2020a, accessible on the Data & Analysis Center for Exoplanet DACE5). Exoplanets around M dwarfs are highlighted in black. The curves are the composition lines of iron, Earth-like, and pure water planets (at Teq = 693 K).
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