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Fig. 9

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Overview of the presented companions (encircled in red) compared to known planets from the PlanetS catalog (extended from Otegi et al. (2020); Parc et al. (2024), updated August 2024). The data are color coded by planetary radii. The histogram at the top shows the relative occurrence of the transiting gas giants with masses ranging from 0.1 to 13 MJup. The low-mass star regime remains relatively poorly populated; our three mass characterizations contribute to this population.

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