Fig. 12.
Spectra of SN 2019lqo compared to those of Type IIb SNe 2011dh (Ergon et al. 2014) and 1993J (Matheson et al. 2000). The most prominent SN lines are indicated based on Ergon et al. (2014). The spectra have been extinction and redshift corrected, and shifted vertically for clarity. The main telluric band wavelengths for SN 2019lqo are indicated with a circled plus sign (⊕).
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