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Fig. 4.
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In situ mass fraction fin, NSC versus log(MNSC/MGCS) (left) and MNSC (right) as seen in Fig. 3. The solid line shows the fit using only the ACS data (Fornax and Virgo galaxies), and the dashed line when using all data. Bottom panels: residual scatter. The standard deviations are shown in the label.
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