Fig. 3.
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Consistency of Mg abundance from the lines 5528 and 5711 Å. For the TITANS, difference between Mg abundances from the lines λ5528 Å and λ5711 Å as functions of the atmospheric parameters. The red lines are the linear regressions and the shaded areas indicate 1σ and 2σ dispersions. The reference stars HD 22879, HD 140283, and HD 84937 are identified with bold contours.
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