Fig. 8.
Normalised observed spectrum of a particular metal-rich star ([M/H] = +0.31 dex) in the abundance estimation window of the non-saturated line 4730.04 Å. Different line profile depending on the applied local continuum intervals (Δλnorm = 1.35 (blue), 4.35 (red), 68 Å (black)), along with the derived [Mg/Fe] abundance for each case.
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