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Fig. 5

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Distribution of the Gaia DR3 radial velocities of the sample of 2.7 million stars used to assess the rate of outliers as a function of S/N and for three different intervals of absolute values of the radial velocities. The three intervals are materialised in green ([0, 200) km s−1), blue ([200, 400) km s−1) and salmon ([400, 1000) km s−1) respectively. We note that the Large Magellanic Cloud (LMC) and the Globular Cluster NGC 3201 both produce a peak visible on top of the distribution of Milky Way stars.

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