Fig. 9.
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Spectra of SN 2018xx and SN 2019gbx compared with spectra of the other NV SN 2004eo (Pastorello et al. 2007) and SN 2011fe (Zhang et al. 2016) at t ≈ −12, −7, 0, and +30 days (relative to B-band maximum). All the spectra have been corrected for redshift and reddening from their host galaxies and have been shifted vertically for clarity.
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