Fig. 19.
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Comparison of the first CO overtone region of SN 2022jli at +139, +190 and +224 days with the with nebular phase CO emission from the type Ic SNe 2013ge (Drout et al. 2016) and SN 2016adj (Stritzinger et al. 2024), and the type II SNe 1987A (Bouchet et al. 1991), 2017eaw (Rho et al. 2018) and 2020ocz (Cartier et al. 2021). The phase and the SN colour are indicated in the inset.
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