Fig. 1
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Overview of hot Jupiters (red) with close-by companions (black), including TOI-2109 b. Sizes are to scale. We note that the WASP-47 system also contains a long-period companion that is not shown here. System parameters are taken from Cañas et al. (2019), Wong et al. (2021), Hord et al. (2022), Korth et al. (2023), Maciejewski et al. (2023) and Nascimbeni et al. (2023).
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