Spectral Analysis of GRBs Measured by RHESSI

A. Zehnder; C. Wigger; D.M. Smith; E. Bellm; K. Hurley; M. Bandstra; S. Boggs; W. Hajdas

arxiv: 0704.3038 · v1 · pith:QUQNAY3Fnew · submitted 2007-04-23 · 🌌 astro-ph

Spectral Analysis of GRBs Measured by RHESSI

C. Wigger , W. Hajdas , A. Zehnder , K. Hurley , E. Bellm , S. Boggs , M. Bandstra , D.M. Smith This is my paper

classification 🌌 astro-ph

keywords rhessigrbsresultsspectralswiftaboveanalysisbursts

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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.

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Spectral Analysis of GRBs Measured by RHESSI

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