Fig. 11
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Top two panels: CCF weights for each night of data, for cases 1 and 2 (top panel) and for cases 3 and 4 (second panel). Third panel: S/N per order, for each night of data. The S/N increases towards the red showing the sensitivity of both HARPS detectors. Bottom panel: number of stellar lines per order, which is the same for each night of data.
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