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Fig. 7

Fig. 7 Refer to the following caption and surrounding text.

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Kinematic map of the BSS population in NGC 188. Arrows represent relative proper motion vectors scaled to 8 times their annual displacement. The crimson stars denote the two identified ejected candidates, characterized by high velocities and high alignment scores (cos θ). The core and halo limits are indicated by dashed and dotted circles, respectively. Black crosses denote excluded interlopers.

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