Fig. 27
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Sky distribution in galactic coordinates of the sources in the FPR sample, color-coded by their median RV (the RV range is limited to 150 km s−1 in absolute value for visibility). The velocity pattern resulting from the rotation of the Milky Way Galaxy is clearly visible, as well as several bright sources in the Magellanic Clouds having VR ≳ 150 km s−1.
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