Fig. 1.

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Position-space separations as a function of time before and after reducing the spread in the curves. Left: Time evolution of separation in position space for each S-star and the central black hole. Right: y = −0.00018446 ⋅ a/au + log(e)+4.3103 subtracted from the time evolution of log10(δr) for each S-star. The grey shading shows the region between the non-reduced maxima and minima of δr over the whole system at each time step, indicating the magnitude of reduction in the spread of the curves, although its lower section is obscured by the coloured curves.
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