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Fig. 3.

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Monte Carlo sample distribution of the motion integral of NGC 6779 (red) and star Gaia EDR3 1189399628220805760. The metallicity difference and p of this pair are 0.27 and 0.87, respectively. The marginal two-dimensional and one-dimensional kernel density estimates are represented by the frame and top histogram, respectively. The histograms are normalized to their maximum values for ease of presentation.

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