Fig. 2.
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Radial velocity (vRV) as a function of Galactic latitude (b) for the data sample with l ∈ [90, 100] deg and 
. The dashed line corresponds to the fitted function and the scatter point correspond to stars with available radial velocity information. The range in b on the horizontal axis corresponds to a range in height spanning roughly Z ∈ [ − 1, 1] kpc at the relevant distance.
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