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Fig. A.1.

image

MUSE spectra (labeled on the top of each panel). Upper sub-panels: spectra extracted from each individual exposure (shifted up for clarity) and the average spectra of the object at its true flux level. The XSL spectra, when available, are plotted in red underneath the averaged MUSE spectrum. Bottom sub-panels: standard deviation of the average spectrum. The spectra of all stars are available at the CDS.

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