Fig. A.2
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Results for scenario “55,EDR3,GA,NM”, using the VLBI data and Gaia EDR3 as in Fig. 1, but replacing the VLBI data of stars HD 283572, V410Tau, SS Cyg, Brun 334, TYC 5346-538-1, Haro 1-6, BHCVn, σ2 CrB, HD 199178, AR Lac, IM Peg, and HD 22468 with newly determined models of stellar motion and newly corrected absolute positions as described in Sect. 4.3.
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