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Fig. 9

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Planet-to-star ratio obtained from complete light curves (red points) and incomplete ones (black points) when the pulsations have been accounted for in the model fitting. Vertical color-dashed lines indicate the central wavelength of each filter. The dashed/dotted black line shows the best-fitting linear model to the 19 Rp/Rs data points. In red and considering complete primary transits only, the dashed/dotted line shows the low-significant wavelength-dependent trend, while the continuous line accounts for the mean radius ratio.

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