NASA NTRS · 19930056086
Hardness/intensity correlations among BATSE bursts
Abstract
Conclusions about the nature of gamma-ray bursts derived from the size-frequency distribution may be altered if a significant correlation exists between burst intensity and spectral shape. Moreover, if gamma-ray bursts have a cosmological origin, such a correlation may be expected to result from the expansion of the universe. We have performed a rudimentary search of the BATSE bursts for hardness/intensity correlations. The range of spectral shapes was determined for each burst by computing the ratio of the intensity in the range 100-300 keV to that in 55-300 keV. We find weak evidence for the existence of a correlation, the strongest effect being present when comparing the maximum hardness ratio for each burst with its maximum rate.
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Paciesas, William S., Pendleton, Geoffrey N., Kouveliotou, Chryssa, Fishman, Gerald J., Meegan, Charles A., Wilson, Robert B.. 1992-01-01. Hardness/intensity correlations among BATSE bursts. https://ntrs.nasa.gov/citations/19930056086
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