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Fig. 3

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Upper panel: eclipse time delays with respect to a constant orbital period model plotted versus the orbital cycle for all the available X-ray eclipse time measures together with the best-fit parabola. Lower panel: residuals in units of σ with respect to the best-fit parabola. The black full squares points are from BU10, the red diamonds are the data added in this work. (This figure is available in color in the electronic form.)

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