Fig. 9
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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