Fig. 1.

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Distribution of the relative errors (from left to right): radial velocity (eRV), proper motions in right ascension (ePMRA), and declination (ePMDEC), and in heliocentric distance eD⊙. Blue histograms represent the error distributions. The following GCs are not shown because the error values are too high: Crater, Lae 3, NGC 6760, BH 261, NGC 6553, and Pal 13, except in the graph in the bottom right panel.
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