Fig. 7
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q distributions of the detected unresolved binaries (in the mass range of 0.49-1.2 M⊙) in NGC 2360 and NGC 2682 (M67) shown by red and blue lines, respectively. The grey shaded region indicates the mass-ratio bins below qthresh;Gaia, and the estimated binary fractions for the two mass-ratio thresholds, i.e. qthresh;Gaia and qthresh;Gaia+, are reported along with the Poisson uncertainties.
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