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Fig. 2


[Ti/Fe] as a function of metallicity for the full APOKASC sample for the 15 873.8 Å, 15 715.6 Å, 15 334.8 Å, and 15 381.1 Å lines from top to bottom, respectively. The stars are color-coded by the BACCHUS method-to-method dispersion, which is defined as the standard deviation of the abundance derived from the four procedures.

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