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Fig. 9.

image

Left panel: calibrated IQR2 values as a function of the distance in kpc from the Galactic plane (H10). Horizontal lines are traced at the average values of the corresponding galactic populations (same colour coding). Right panel: cumulative distribution of IQR2 for GCs of different sub-populations. The P values from two-sample Kolmogorov–Smirnov (K–S) tests are indicated.

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