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Fig. 4

image

U-V diagram showing the position of LS IV-14°116 (thick error bars) as compared to 3σ thin-disk and 3σ thick-disk contours. Stars located outside these contours have kinematic properties of the halo population. The points inside the contours correspond to the reference white dwarf sample of Pauli et al. (2006). These authors performed a detailed kinematic analysis of 398 DA white dwarfs using the same method as applied here.

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