Image Details
Caption: Figure 7.
SED of KN2-B with best-fit models from Robitaille (2017), overlaid with Herschel 100–350 μm photometry and corresponding error bars. The best-fit model (with ﹩{\chi }^{2}/\mathrm{datapoint}﹩<3) with a stellar temperature of ∼18,500 K is shown as a solid black line. Other models with ﹩{\chi }^{2}/\mathrm{datapoint}﹩<5 are also shown as solid gray lines.
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