Fig. 6
ASAS-3 V-band (top), V − I (middle), and I-band (bottom) light curves outside of the eclipse, phased with period 
. The small amplitude of the observed V variation and its strongly non-sinusoidal shape with a wide minimum are related to the presence in the system of the second component which strongly dominates in this wavelength range (see Sect. 3.7).
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