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Fig. 6.

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Time-resolved spectroscopy using the NS atmosphere model for burst #4. Results for other bursts are shown in Fig. A.3. Panel a shows the estimated bolometric flux, panel b shows the time evolution of the ratio of luminosity to the Eddington luminosity, panel c shows the time evolution of the normalization, and panel d gives the reduced χ2 fit statistic. Time is relative to the burst onset (t0).

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