Fig. B.50
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Upper panel: OGLE I-band light curve of the eclipsing binary VFTS 702, phased with the derived ephemeris of P = 1.981546 d (the dominant spectroscopic period) and T0 = 54869.033 [JD-2400000]. Lower panel: Same light curve, phased with the second identified period of P = 2.932818 d and T0 = 54869.84 [JD-2400000], The 1.98 d signature was subtracted from the data shown in this panel.
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