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Fig. 6


P analysis: relative flux difference, (fλ,o − fλ,S)/fλ,o, smoothed to a resolution corresponding to Δλ = 50 Å, for a subset of the grid with [M/H] = 0.0 around the best-fit parameters for Star 1 are shown in gray-scale. The best-fit model (Teff/log g/[M/H]  =  3940/2.0/0.0) is overplotted with a thicker line style.

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