Fig. 2.
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PRE phase spectra and residuals for burst # 9. Top panel: PRE phase spectra from the burst # 9. The best-fit model, Tbabs × (bbodyrad+gaussion+bbodyrad) × gabs × gabs, is represented by the solid red line. The 1 keV emission line are clearly shown in the spectra and a pair of absorption lines are indicated near 1.6 and 3 keV. The two middle panels are the residuals of the spectra fitted with 3c50 and SCORPEON backgrounds, respectively. The bottom panel shows the residuals of the best-fit model to the spectra.
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