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Spectra of cosmic gamma-ray bursts in the hard X-ray rangeHard X-ray measurements of six gamma-ray bursts observed by detectors on the OGO-5 and OSO-6 satellites during the period Oct. 1969 to Apr. 1971 are presented. Spectra for five of the six bursts were determined using measurements from both satellites in order to reduce ambiguities due to uncertain source locations. A significant fraction, 20 to 60%, of the energy of the bursts fall in the hard X-ray range (20 to 130 keV). The time-integrated spectra were fitted by power-law, exponential, and thermal bremsstrahlung functions. They are consistent with power-laws which steepen at energies approx. above 150 keV, as reported earlier for two other bursts. Evidence for spectral variability from event to event in the hard X-ray region is presented. The hard X-ray spectra of the gamma-ray bursts differ from those of the recently discovered 1 to 15 keV bursts.
Document ID
19780004007
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Share, G. H.
(Naval Research Lab. Washington, DC, United States)
Kane, S. R.
(Calif. Univ. Berkeley, United States)
Date Acquired
August 9, 2013
Publication Date
July 1, 1977
Publication Information
Publication: in ESA Recent Advan. in Gamma-Ray Astronomy
Subject Category
Space Radiation
Accession Number
78N11950
Funding Number(s)
CONTRACT_GRANT: NGL-05-003-017
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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