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Fig. 5
The observed V-band light curve compared to the theoretical one, based on our PHOEBE solution. The lower panels show a zoom of the curves in the neighbourhood of both binary eclipses and the residua from the model fit. Typical 1-σ observational uncertainties are 0ṃ01. Orbital phases from ephemeris (2) are used.
This figure is made of several images, please see below:
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