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Fig. A.6

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Night-to-night changes demonstrated on the spectra taken at CFHT on 2012-08-13 and 2012-08-14. Significant changes are shown only in the hydrogen and oxygen lines. Also shown to be slightly different is the blue wing of the Fe II lines 4 924, and 5 018 Å lines. Other lines do not show night-to-night variations. The spectra are corrected on the system radial velocity. The laboratory wavelength connected with the system is plotted by the vertical grey line and its thickness corresponds to its error.

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