Fig. 10
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Planetary radii vs. orbital period (upper panel) and planetary masses vs. orbital period (lower panel) of known exoplanets from the NASA Exoplanet Archive (Akeson et al. 2013) with mass and radius constraints better than 50 and 20%, respectively. The light pink highlighted region represents the hot Neptunian desert with boundaries defined by Mazeh et al. (2016). The position of TOI-6651b is shown as a pink star.
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