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Fig. 1.
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TESS light curve of ExtEV phased with the orbital period of 32.83016 d. Orbital phase φorb = 0.0 corresponds to the time of the periastron passage derived in Sect. 4.3. The inset shows the light curve near the periastron passage. Stochastic light variations and TEOs can be seen over the entire range of orbital phases.
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