Abstract
BATSE observed its most intense gamma-ray burst on 1993 January 31. The event reached count rates >~ 2 x 10^6 counts/s with most o fthe flux emitted in an extremely short ( 4 MeV in energy were recorded by BATSE during this first interval. The burst spectrum is best fitted by a broken power law with a break energy of 170 +/ 27 keV. The low-energy spectral index is -1.30 +/- 0.05, while a softer spectral index of -1.9 fits the spectrum between 170 keV and 2 MeV. Our data provide the only low-energy spectrum for this event; the combination of our spectrum with the one reported for GRB 930131 by the EGRET group extends the total energy spectrum of a GRB for the first time over five decades, up to the GeV range.
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CITATION STYLE
Kouveliotou, C., Preece, R., Bhat, N., Fishman, G. J., Meegan, C. A., Horack, J. M., … Norris, J. P. (1994). BATSE observations of the very intense gamma-ray burst GRB 930131. The Astrophysical Journal, 422, L59. https://doi.org/10.1086/187212
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