1999/01/19 by M. S. Briggs, D. L. Band, Briggs, M. S. +8
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9901224
To appear in the Proceedings of the 3rd INTEGRAL Workshop, "The Extreme Universe". Four pages
arxiv created 1999/01/19 · openalex publication_date 1999/01/19 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
A 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.