Fig. A.2

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Line shape evolution of various lines as indicated in each panel for the second observing season. Top left: RV shift over time of the individual spectra. We show all taken spectra in grey and the colour coding of the spectra shown in the other panels. All other panels: Line centre marked with the vertical dashed broad line, while the narrow dashed vertical lines mark velocities of ± 10 km s−1 and ± 20 km s−1.
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