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Fig. 14.

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Bolometric LC of SN 2021aatd (black circles) with the best-fit two-component Model I curves (red line). The left and right panels show the results of our model fitting assuming a recombination temperature of Trec = 6500 and 7000 K, respectively. The contributions of the core and the shell parts of the ejecta are plotted as blue and green lines, respectively. The light blue and magenta lines represent respectively the contribution of the radioactive decay and magnetar energy input to the luminosity evolution of the core component. Details and parameter values can be found in the text and in Table 4.

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