Fig. 6
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Transits of the three innermost planets in the HD 224018 system as observed by K2. For planets b and c, the transits are phase-folded to their corresponding orbital periods. The blue lines represent the best-fit transit models. The shaded blue area indicates the 1σ uncertainty in the transit depths (rp/R*)2. The O-C data points are the residuals of the best-fit models.
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