Comparison of SN2023ixf bolometric light curve with Type-II population from Carnegie Supernova project (Martinez et al. 2022). The features are those reported in Martinez et al. (2022): M_bol_end is the bolometric magnitude measured 30 d before t_PT (midpoint of the plateau–tail transition). If t_PT is not defined, this is the magnitude of the last observation during the optically thick phase; M_bol_tail is the bolometric magnitude 30 d after t_PT. If the transition is not well defined but the tail is observed, this is the magnitude at the closest point after the transition; s1 is the decline rate (mag/100 d) of the early cooling phase, obtained from a linear fit; s2 is the decline rate of the plateau phase, obtained from a linear fit; s3 is the decline rate of the radioactive tail, obtained from a linear fit with at least three data points; Cd is the cooling phase duration, from t_explosion to t_trans; pd is the plateau duration, t_PT − t_trans; optd is the optically thick phase duration, t_PT (if t_explosion is known). When possible, we estimated the parameters following the formalism in Martinez et al. (2022). The values are within the distributions for each of the parameters; the only value we could not estimate is s1, due to the lack of data in the time range defined to infer this parameter.