Fig. 6.
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Best fit to the primary (blue) and secondary (red) times of minimum light of V889 Aql, after subtracting the linear ephemeris (top left), after subtracting the linear ephemeris and the effect of the third body (bottom left), and after subtracting the linear ephemeris and the apsidal motion (top right). The panel at the bottom-right shows the residuals from all the fits.
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