Light-curve rise and decline timescales against absolute magnitude. Left: Rise time against the Gall et al. (2015) sample measured from the r band. The P23 sample does not have explosion constraints, and is therefore not included here. Right: Decline rate of SN 2022lxg (filled marker in g band, open marker in V band), compared to other luminous Type II SNe from the P23 sample (V band), the Type IIP/IIL sample of Faran et al. (2014) (V band), and several unusual transitional and/or interacting Type II SNe; SN 1996al (Benetti et al. 2016) (B band), SN 1998S (Leonard et al. 2000; Fassia et al. 2000) (V band), SN 2016gsd (Reynolds et al. 2020) (B band), SN 2017ivv (Gutiérrez et al. 2020) (V band), SN 2018ivc (Bostroem et al. 2020; Maeda et al. 2023a; Reguitti et al. 2024) (B band), and the fast and faint Type IIb SN SN 2020ikq (Ho et al. 2023) (g band).