Abstract
We present preliminary results of systematic temporal and spectral analysis of the Konus-Wind observational data on short and intermediate SGR bursts. We conclude that the burst energy spectra are equally well described, in the 20 − 200 keV range, by both power-law with an exponential cutoff, and double black-body functions. We also discuss energetics and durations of the bursts, distributions of the spectral parameters and correlations between them.
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