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Fig. 9


Eccentricity-period relationship for transiting brown dwarfs and giant planets (0.5–13 MJup) with percentage errors <10% for both mass and radius and a defined eccentricity in the NASA Exoplanet Archive1: a total of 129 previously known planets, including 17 with masses greater than 4 MJup. Transiting brown dwarfs are from the literature summary found in Mireles et al. (2020), for a total of 16 with well-defined masses and radii.

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