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Fig. 14.

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Comparison of around-peak (purple) and late-time (green) spectra of SNe 2020nxt, 2020taz, 2021bbv, 2023utc, and 2024aej with other SNe Ibn at similar phases. All spectra have been corrected for redshift and extinction. Significant He I features are marked by blue dashed lines, while Balmer features by red dashed lines.

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