Fig. 7.

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Proper motions of the full spectroscopic sample. The plot is restricted to an area around the proper motion of Boo II for the sake of visibility, but other stars (clearly non-members) are located outside this region. The density background shows the density of MW star in the field of Boo II, with 1 and 2σ contours shown as dashed black lines. The colour and marker schemes are the same as in previous plots.
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