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Fig. C.2


Same data as Fig. C.1 but rebinned by a factor of 100 (diamonds). The same best-fit model of Fig. C.1 using a simple blackbody with a temperature of 50 eV is indicated with the red line. The blue line indicates the model for the source that entered the simulation: the sum of a blackbody spectrum and a weak Gaussian line at 30 Å.

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