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Fig. 6.

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Comparison of the absolute magnitude r-band light-curve of SN 2022lxg to three LSNe from the P23 sample in the V band (SN 2017cfo, SN 2017hbj, SN 2017hxz) and to other fast declining transients of various subtypes: SN 1998S, SN 2016gsd, SN 2018ivc in V band, and SN 1996al, SN 2020ikq, and two more Type IIb SNe (SN 2011dh; Arcavi et al. 2011; Bersten et al. 2012, SN 2011hs; Bufano et al. 2014) in the r/R band. Visual extinctions (for both MW and host galaxies) and distance moduli are retrieved from the referenced works (see also Fig. 5 for the references). There is a remarkable similarity in the decline rate (and luminosity) with SN 2017hxz of the P23 sample.

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