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Fig. D.1

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HARPS IP models in velocity space for orders 89 through 122. Each panel shows the IP in 16 segments of one order, whose central wavelength is printed above it. Line colour within the panel changes from blue to red with increasing wavelength. The same plots with background reference grids (which make it easier to see the profile changes) can be found on the arXiv version of this manuscript https://doi.org/10.48550/arXiv.2311.05240.

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