Fig. B.1
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Run of the contrast dG versus separation in arcsec for companions detected in Gaia DR3. We plotted only companions with separation <10 arcsec. Black filled circles are companions also detected with full astrometric solution in Gaia DR2. Grey filled circles are companions detected in Gaia DR2 but without astrometric solution. Empty circles are companions not detected in Gaia DR2. The blue solid and red dashed lines are the 50% and 1% contrast limits for Gaia DR2 according to Brandeker & Cataldi (2019), respectively.
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