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Figure 1:
Top: light curve of simulated noise signal.
Bottom: diffusion entropy as a function of the temporal window ![]() ![]() ![]() |
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Figure 2: Light curve of the GRB 910429 ( top) and GRB 910601 ( bottom). Data represents the counts as function of time in four different energy channels. From top to bottom: 20-50 keV, 50-100 keV, 100-300 keV, and 300-1000 keV. |
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Figure 3:
Diffusion Entropy of GRB 910429 ( top) and GRB 910601 ( bottom), four different channels. Numerical data (dots). Lines: data fits using functions
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Figure 4: Distribution of the Diffusion Entropy index over a sample of 1224 Long GRB calculated considering the first 2 T90 portion of the light curves. Different panels correspond to different energy channels: 20-50 keV ( top-left), 50-100 keV ( top-right), 100-300 keV ( bottom-left), 300-1000 keV ( bottom-right). DE indices mean and RMS values are shown in legends. |
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Figure 5:
Power-complexity relation: the scaling index ![]() ![]() ![]() ![]() ![]() |
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Figure 6:
Light curves for two simulated burst.
The light curves have been scaled in the four channels in order to take into account the different count rate in the different channels. Background noise has been added to the light curve.
Top panel: the light curve is obtained using the peak shape of Eq. (5) with
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Figure 7:
Simulated power-complexity relation. The synthetic light
curves are obtained using a fred-like exponential peak shape. In the
plot various relations have been obtained by varying the number of the peaks
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Figure 8: Diffusion Entropy as a function of time of GRB 910429 ( top), and GRB 910601 ( bottom). W = 32 s (500 points) and M=0.64 s (10 points). Channel 1: 20-50 keV, Channel 2: 50-100 keV, Channel 3: 100-300 keV, and Channel 4: 300-1000 keV. Curves are averaged over L=10 realizations to smooth statistical fluctuations. The arrows indicate the end of the burst given by the T90 parameters. |
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