Fig. 10.

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Corner plot presenting the posterior distributions of the SW17 shock-cooling light-curve model of SN 2024iss. The fit to the early light curves was restricted to five days after the estimated time of the SN explosion. The best-fit parameters are listed at the top of the figure. The upper-right inset presents the model light curves that best fit the multiband photometry, as displayed by color coded curves and symbols, respectively.
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