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Fig. 10

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Comparison of TOI-4860 b with known exoplanets. Left: mass-radius diagram of known exoplanets. Grey dots are transiting planets listed in the NASA Exoplanet Archive (https://exoplanetarchive.ipac.caltech.edu/) with planetary radius and mass uncertainties below 20%. TOI-519, TOI-3235, and TOI-5205 are shown (from left to right) as red dots. The blue open circle with error bars marks the position of TOI-4860 b. Centre: idem for planetary versus stellar radii (restricted to planets with planetary radius uncertainties below 20%). Right: idem for planetary radii versus orbital period.

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