Fig. 9.
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Metallicity inferred from the Mghost (MBhost) and M* using the relations from Tremonti et al. (2004, circles) and Berg et al. (2012, stars). Left: Metallicities estimated with both relations across the full parameter range. Right: Metallicities derived within specific ranges of stellar mass and absolute magnitude. The dashed orange line denotes the one-to-one (x = y) relation.
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