Fig. 15
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Timing residuals of the simulated data files versus orbital phase for binary systems with orbital periods of 4.5 h, 3 h, 2.45 h, and 1 h. The spiky features appearing at the superior conjunction (ψ = 90°) demonstrate the limitations of the current software, in this case, the ‘polyco’ predictor. The simulation was done with TZNSPAN=3 min and 20 coefficients.
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