Fig. 12.
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Temperature and radius of several LL SNe IIP, including SN 2020cxd (shown as black stars). Upper panel: evolution of their photospheric temperature estimated by fitting a blackbody to the SED in the optically thick phase. Bottom panel: evolution of their photospheric radius based on the same fits. We followed Jäger et al. (2020) in the methodology and the included SNe are also from that paper.
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