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Fig. 4.
Part of the HR10 spectrum of S08-6 (top), S08-242 (middle) and S05-67 (bottom) in black with their synthetic best fits over-plotted in red. A set of lines used in abundance determination are indicated for each star. The stars are ranked from top to bottom by decreasing signal-to-noise ratios: 83, 38, and 23.
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