Deblending of stellar spectra on MUSE data. The top left panel shows a white light image of the central MUSE datacube in NGC 6397. A zoom into the area indicated with a red square is shown in the top middle panel. In the top right panel, the same field of view is shown as seen with HST. All stars for which spectra were extracted are shown with crosses. Spectra extracted from the stars indicated with the red and green crosses are shown in the bottom panel and show clearly distinct features without any contamination from each other. The star indicated in red was determined to be a late-type G star, while the star in green is type A. The spectra are continuum subtracted and normalised and the areas dominated by telluric absorption are indicated in grey for clarity.