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Fig. 2

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Synthetic NLTE spectra showing the shape of the aluminium lines 3944 Å and 3961 Å and their blends as indicated. For the synthetic spectra, the star HD 177095 at [Fe/H] = −0.74 serves as an example for the NLTE calculations. Dashed lines indicate a spectrum with no aluminium present, while the red and blue lines show spectra with [Al/Fe]=−0.5 and 0.0, respectively.

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