Mass discrepancy analysis for a select sample of Type II-Plateau supernovae

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Fig. A.1.

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Left: pre-SN model for each SN of our sample as a function of mass. Right: pre-SN model for each SN of our sample as a function of radius. These models come from double polytropic calculations (see Sect. 3). The values of the parameters for each model are shown in Table 3.

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