Fig. 7.
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Spectra of SN 2022xlp, SN 2019muj (Barna et al. 2021), SN2012Z (Stritzinger et al. 2015), and SN 2022ywf (Barna et al. in prep.) measured 19 days after the explosion. Because of the order of magnitude difference in luminosity in the Iax subclass, we plot the logarithm of spectral luminosity density. The strong similarity between SN 2022xlp and SN 2019muj can be amply observed.
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