Fig. 6.
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Best-fit values from the fa model, TBabs × (bbodyrad + fa × nthcomp), and 1σ uncertainties of two X-ray burst spectra. From top to bottom: burst flux, Fburst, the blackbody temperature, kTbb, and radius, Rbb, the enhanced persistent emission flux, Fper, and the goodness of fit per degree of freedom, , for bursts #4 (left panel) and #5 (right panel). The blue dashed-dot lines represent the flux of the persistent emissions before the bursts. The grey data are fitted by the blackbody model for comparisons.
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