Fig. 4.
Observed solar spectrum from HARPS (R = 115 000, asteroid reflection) around the line 5711.09 Å. The adopted wavelength domain where the abundance is measured is delimited by blue vertical lines (ΔλAbund ∼ 0.5 Å). Two different local normalisation intervals of 1 Å (Δλ1) and 4 Å (Δλ2) are shown with red and orange dashed vertical lines, respectively.
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