Fig. B.2
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Run of the contrast dG versus separation in arcsec for companions detected in Gaia DR3 in a sample of about 1300 young nearby star. We plotted only companions with separation <10 arcsec. Black filled circles are companions detected by Gaia DR3. Grey filled circles are companions for which Gaia DR3 gives only position, but not G magnitude. Empty circles are companions not detected in Gaia DR3. 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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