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Fig. 14


Evolution of the integrated luminosity of the most prominent Balmer lines (Hα and Hβ) compared to those inferred for SN 2010jl. Insets in the upper panel show representative spectra during the different phases of the evolution of SN 2015da. The inset in the bottom panel shows the evolution of the Hα/Hβ ratio compared to that computed for SN 2010jl.

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