Fig. F.1.
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Spectrum fitting for the SLSN 2015bn. Left panel: position of SN 2015bn in the MUSE image of the observed field. Right panel: extracted spectrum for SN 2015bn, where the broad emission lines of the SN are still clearly present. Emission lines of Hα, Hβ, O[III]λ5007, and N[II]λ6583 belonging to the underlying H II region can be identified.
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