Fig. 1

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Proper motions of HVS candidates selected from Gaia DR2 with PM>20 mas yr−1 Plx>0.1 mas, available BP, RP photometry, and vtan_g>500 km s−1. All 1520 high-priority candidates with Plx/e_Plx>5 are shown. The red symbols are objects with unconfirmed (crosses) or not measured (plus signs) proper motions in DR3. The magenta circle and symbols indicate the minimum HPM of 60 mas yr−1 and the six extreme (vtan_g>700 km s−1) nearby HVS candidates selected with additional DR2 quality criteria by Scholz (2018), respectively. The three labelled objects have still vtan_g>700 km s−1 when DR3 is used.
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