Fig. 7.

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Time-resolved spectroscopy using the NS atmosphere model in addition to the fa correction for burst #4. Results for other bursts are shown in Fig. A.4. Blue markers are used for the first fa case, constant*(diskbb+comptt) and light green markers for the second fa case, constant*diskbb+comptt. Since their behavior is similar, the blue markers overlap the green ones. Panel a shows the estimated bolometric flux, panel b shows the time evolution of the ratio of luminosity to Eddington luminosity, panel c shows the evolution of the fa factor, and panel d gives the reduced χ2 fit statistic.
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