Comparison of SN 2022jli with other SE SNe during the SN re-brightening. On the left panel, the SN is compared at the time of its second maximum with the SLSNe-I SN 2019stc (Gomez et al. 2021) and SN 2015bn (Nicholl et al. 2016b), the Ic SN 2013ge (Drout et al. 2016), the Ib SN 2007Y (Stritzinger et al. 2009, 2023) and the IIb SN 2011dh (Ergon et al. 2014) at a similar phase relative to the first maximum. Similarly, on the right panel, SN 2022jli is compared with SN 2019stc, SN 2013ge and SN 2011dh (Ergon et al. 2015) at about +149 days relative to the first maximum. We indicate the rest-frame wavelength of the main spectral features. All the spectra have been corrected for reddening assuming R_V = 3.1 and values from the literature, in the case of SN 2022jli we assume E(B − V)_tot = 0.27 mag.