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Fig. 3

Synthetic spectrum fit to the lanthanum line at 4662 Å and cerium line at 5274 Å. The observed spectrum for the programme star HD 204848 is shown as dots. The grey lines are synthetic spectra with [La/Fe] = 0.20 ± 0.10 and [Ce/Fe] = 0.10 ± 0.10, respectively.
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