Fig. B.1.
Example Be star spectral classification of star 290. The MUSE spectrum of the star that has to be classified is shown in black. Overplotted and shifted vertically for clarity are a set of standard star spectra (as described in Sect. 4.1) of spectral types B1 to B9, degraded to the MUSE resolution. While the continuous line shows the observed standard star spectrum, the dash-dotted line is rotationally broadened by 200 km s−1.
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