Fig. A.1.

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Comparison of the observations (MUSE spectrum, red line) with BPASS models (black line). The left column shows three BPASS models with an IMF up to 100 M⊙, ages of 1.5 Myr, 2 Myr, and 2.5 Myr and an added number of 236.56 150 M⊙ VMS. The right column shows a BPASS model with an IMF up to 100 M⊙ at same ages (as shown in previous column), but with an added number of 236.56 and 60.30 VMS of 150 M⊙ and 200 M⊙.
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