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Fig. 8.

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Late time spectra of NGC 300 OT and AT 2019ahd. A shift in flux has been applied to superimpose the two spectra. The broad features described in the text are highlighted with grey shaded regions. The lower panels show the temporal evolution of these broad features in NGC 300 OT, starting from their first detection. Dashed vertical lines mark the positions of their peaks estimated through a Gaussian fit.

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