Fig. 6
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Detectability of transit events of the candidate planet b (top) and the confirmed planet c (middle) in the TESS data of Gl 725 AB as a function of orbital inclination and planet radius. Bottom: posterior distributions of the planetary radii for Gl 725 Bb (blue) and Gl 725 Bc (brown) inferred using the spright tool (Parviainen et al. 2024).
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