Fig. 6
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Average isolated spectrum, F*,N, calculated from three real HARPS transits (orange) and its corresponding best-fit spectrum (purple) with Teff and log g fixed to parameters from Lendl et al. (2020). The shaded green region in the inset indicates ±0.2 variations in metallicity, [Fe/H]. The dotted green line indicates the spectrum with solar metallicity, [Fe/H] = 0.
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