Fig. 3.
U − V diagram showing the positions of Feige 46 (star) and LS IV−14 ° 116 (cross) compared to the 3σ thin-disk (solid line) and thick-disk (dashed line) contours as defined by Pauli et al. (2006). Stars outside these contours have kinematic properties of the halo population. The larger error bars are centered on the values derived by Randall et al. (2015) for LS IV−14 ° 116.
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