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Table 1:

Results of the time-resolved spectral analysis of GRB 060428C. Errors are at 90% c.l.

Name
$T_{\rm Start}$ $T_{\rm Stop}$ Spectral model Phot. index E0 (CPL) or kT (QT) $\chi^{2}_{\rm red}$ d.o.f.
  UTC UTC     keV    
Interval 1 02:30:35 02:30:40 PO $1.9 \pm 0.1$   1.4 28
      CPL $1.3 \pm 0.5$ $\rm 74^{-32}_{+155}$ 1.2 27
      QT $2.3 \pm 0.5$ $\rm 14^{-5}_{+5}$ 1.2 26
Interval 2 02:30:40 02:30:44 PO $1.46 \pm 0.07$   1.95 31
      CPL $0.5 \pm 0.3$ $\rm 64^{-16}_{+30}$ 1.25 30
      QT $1.4 \pm 0.3$ $\rm 17^{-3}_{+3}$ 1.15 29
Interval 3 02:30:45 02:30:48 PO $2.2 \pm 0.3$   1.29 21
      CPL Not constrained
      QT Not constrained

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