Fig. 13.
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X-ray luminosity evolution at 0.3–10 keV of SN 2024iss compared with that of SNe 1993J (Chandra et al. 2009), 2011dh (Soderberg et al. 2012), 2013df (Kamble et al. 2016), 2016gkg (Dwarkadas 2025), and 2024abfo (Reguitti et al. 2025). While most of the comparison data are in the 0.3–10 keV band, the fluxes of SNe 1993J and 2013df were measured in the 0.3–8 keV band.
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