Fig. 4.

Decorrelated BRITE-Heweliusz photometry of HD 149 404, averaged over the spacecraft orbit, folded with the orbital period of the binary system. The red solid curve yields the best-fit Fourier reconstruction consisting of two sine waves: one at the orbital frequency and one at its second harmonic (see Eq. (2)). The lower panel illustrates the residuals between the data and this fit.
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