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Fig. 1
All measured mid-eclipses, Tecl, mean longitudes, Tπ/ 2, and orbital epochs are shown with the best-fit models as a function of the orbit numbers. In all cases, the best-fit model is a quadratic or linear fit to the epochs. The lower panel in each figure shows the residual from the best fit.
This figure is made of several images, please see below:
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