Analysis of Line Candidates in Gamma-Ray Bursts Observed by BATSE

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dc.creatorBriggs, M. S.
dc.creatorBand, D. L.
dc.creatorPreece, R. D.
dc.creatorPaciesas, W. S.
dc.creatorPendleton, G. N.
dc.date1999-01-19
dc.date.accessioned2026-07-25T13:27:57Z
dc.descriptionA comprehensive search of BATSE Spectroscopy Detector data from 117 GRBs has uncovered 13 statistically significant line candidates. The case of a candidate in GRB 930916 is discussed. In the data of SD 2 there appears to be a emission line at 46 keV, however the line is not seen in the data of SD 7. Simulations indicate that the lack of agreement between the results from SD 2 and SD 7 is implausible but not impossible.
dc.descriptionTo appear in the Proceedings of the 3rd INTEGRAL Workshop, "The Extreme Universe". Four pages
dc.identifierhttps://arxiv.org/abs/astro-ph/9901224
dc.identifierhttp://arxiv.org/abs/astro-ph/9901224
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/17515
dc.subjectAstrophysics
dc.titleAnalysis of Line Candidates in Gamma-Ray Bursts Observed by BATSE
dc.typetext

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