Best-fit C-statistic of the spectrum of Fig. C.1 when fitted with a simple blackbody. We subtract here the expected value of C-stat and scale by its expected root-mean-square value, so that it is expressed in equivalent number of σ. The dotted lines indicate the ± 3σ range; when the best fit is outside this ± 3σ range, most investigators would reject the model (in this case a simple blackbody). The FWHM used in this figure is the FWHM of the additional Gaussian component in the spectrum (1 Å).
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