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Fig. 10

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Detectability of planet b transit in TESS light curves of GJ 4274 versus orbital inclination and planetary radius. Colors indicate the detection probability, as described in Sect. 5.3. The shaded gray area shows the predicted radius range corresponding to the planet minimum mass, with the darkest shade representing the 64% confidence interval and the lightest shade the 95% interval. The vertical gray line marks the median value derived using spright.

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