Fig. 9.
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Fraction of NSS solutions among EDR3 sources vs. parallax (left) and fraction of NSS sources in GCNS (right). In both figures, we added AstroSpectroSB1 counts to Orbital counts and to SB*=SB1+SB2 counts in addition to counting them individually, and we restrict the ratios to GRVS < 12 sources only for SB* and NonLinearSpectro, to G < 19 for Orbital and Acceleration solutions, and to G < 20 for eclipsing binaries.
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