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Fig. 9

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Similar residuals as Fig. 8, but projected onto the 2-D sky plane and the 50 random draws from the posterior only consider the motion of a potential exomoon (and not residual uncertainties in the orbit of B, which are shown in Fig. 8). The colors of both the data and the models correspond to the 275-day phase, as specified by the colorbar and defined in Fig. 8.

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