Fourier series for eclipses on exoplanet binaries | Astronomy & Astrophysics (A&A)

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Fig. 10

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Signals and spectra for s₁∕s₂ = 3 and α = (s₁ + s₂)∕r = 4s₁∕3r. This is again the maximum value where partial eclipses always occur. All other parameters are kept the same as Fig. 8. The eclipse contributions to the signals are weaker by roughly a factor of 4∕9 compared to Fig. 9.

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