Fig. 11
Distribution of the estimated RV is shown in the left panel. The red line shows the best-fit Gaussian with μ ≃ 2.4 and σ ≃ 1.05. The middle and right panels are the estimated RV as functions of Galactic latitude and longitude, respectively. The red curves show the ⟨ RV ⟩, which keeps constant at ~2.5 over all latitudes and longitudes.
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