Comparison of the r-band absolute magnitude evolution with other type II LSNe and SN 1987A. The phase is with respect to the maximum brightness. The bumps of ASASSN-13dn are not seen in other objects. The adopted maximum light date in MJD, distance (Mpc), and A_V for each SN are, respectively: SN 1987A¹: 49849.8, 0.05, 0.206 (Hamuy & Suntzeff 1990); SN 2008es: 54599.3, 1013.2, 0.032 (Miller et al. 2009) SN 2013fc: 56530.8, 83.2, 2.914 (Kangas et al. 2016); ASASSN-15no: 57235.5, 153.5, 0.045 (Benetti et al. 2018); ASASSN-15nx: 57219.1, 127.25, 0.22 (Bose et al. 2018) SN 2016gsd: 57662.5, 311.6, 0.254 (Reynolds et al. 2020); ASASSN-18am: 58142.6, 140.5, 0.027 (Bose et al. 2021); SN 2017cfo: 57838.0, 178.2, 0.066; SN 2017hbj: 58031.0, 75.0, 0.095; SN 2017hxz: 58070.0, 330.6, 0.128; SN 2018aql: 58206.0, 321.4, 0.052; and SN 2018eph: 58342.0, 121.8, 0.066 (Pessi et al. 2023). For SN1987A and SN2008es we used the R-band photometry. Note that the phase reported for SN 1987A is relative to the explosion and not the maximum.