Fig. 10
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TTVs of Kepler-24 e at the top. Details are the same as in Fig. 4. Bottom panel shows the mass posteriors of the planets of Kepler-24, depending on the addition of Kepler-24 e to the model; see Fig. 8 for a description. Adding Kepler-24 e helps to better constrain the masses of Kepler-24 b and Kepler-24 c, despite having a highly degenerate mass itself.
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