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Table 2:

Spectral analysis of the Swift-XRT data.

Mode
$N_{\rm H}$ $N_{\rm H}$ Photon index $\chi^2$/d.o.f.
    (rest frame)    
  (1021 cm-2) (1021 cm-2)    
WT $\rm 7.2_{-4.6}^{+5.2}$ - $\rm 2.32_{-0.29}^{+0.33}$ 17.9/17 = 1.05
PC $\rm 14.1_{-6.0}^{+7.0}$ - $\rm 2.32_{-0.20}^{+0.20}$ 11.9/17 = 0.70
WT 0.23 $\rm 3.6_{-3.0}^{+3.6}$ $\rm 2.28_{-0.17}^{+0.20}$ 17.7/17 = 1.03
PC 0.23 $\rm 8.3_{-3.7}^{+5.7}$ $\rm 2.17_{-0.22}^{+0.25}$ 12.9/17 = 0.76

Notes. The switch from WT to PC mode occurred at $\sim $180 s after the burst. Analysis of data later than about 2000 s gave results comparable to those for the PC mode but with lower statistical significance.


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