Fig. 1
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Example region of stellar spectra. An example spectrum obtained with the MIKE spectrograph at the Clay Telescope at Las Campanas Observatory is shown in blue, and a synthetic spectrum built using iSpec (Blanco-Cuaresma et al. 2014; Blanco-Cuaresma 2019) is shown in orange. The gray regions were used to fit the observed spectra to obtain chemical abundances of different elements.
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