Spectral Analysis of GRBs Measured by RHESSI
Astrophysics
2010-11-11 v1
Abstract
The Ge spectrometer of the RHESSI satellite is sensitive to Gamma Ray Bursts (GRBs) from about 40 keV up to 17 MeV, thus ideally complementing the Swift/BAT instrument whose sensitivity decreases above 150 keV. We present preliminary results of spectral fits of RHESSI GRB data. After describing our method, the RHESSI results are discussed and compared with Swift and Konus.
Keywords
Cite
@article{arxiv.0704.3038,
title = {Spectral Analysis of GRBs Measured by RHESSI},
author = {C. Wigger and W. Hajdas and A. Zehnder and K. Hurley and E. Bellm and S. Boggs and M. Bandstra and D. M. Smith},
journal= {arXiv preprint arXiv:0704.3038},
year = {2010}
}
Comments
4 pages, 4 figures, conference proceedings, 'Swift and GRBs: Unveiling the Relativistic Universe', San Servolo, Venice, 5-9 June 2006, to appear in Il Nouvo Cimento