Fig. 9.
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Same as Fig. 7, but for m1 against (a) the total stellar mass (M⋆) and (b) the total system mass (Mgrp). The additional solid brown line and shaded band in panel b represent the linear fit and its associated uncertainty derived from the moderately strong positive linear correlation (r = 0.42) between log(m1) and log(Mgrp), calculated after excluding non-BGG groups.
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