Power of wavelets in analyses of transit and phase curves in the presence of stellar variability and instrumental noise - I. Method and validation

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Fig. 6

Result of the light curve test for the impact parameter b. The ordinate is the S/N-ratio defined by Eq. (34). The y-axis is the difference between the simulated and the retrieved impact parameter. We also plotted the 1σ error bar of the impact parameter for this figure. See the meaning behind the black and gray points in Fig. 5.

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