Published in

Società Italiana di Fisica, Nuovo Cimento B, 10011(121), p. 1117-1121

DOI: 10.1393/ncb/i2007-10072-9

Links

Tools

Export citation

Search in Google Scholar

Spectral Analysis of GRBs Measured by RHESSI

Journal article published in 2007 by Claudia Wigger, Wojtek Hajdas, Alex Zehnder, Kevin Hurley, Eric Bellm ORCID, Steven Boggs, Mark Bandstra, David M. Smith
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Red circle
Preprint: archiving forbidden
Orange circle
Postprint: archiving restricted
Upload
Red circle
Published version: archiving forbidden
Policy details
Data provided by SHERPA/RoMEO

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. Comment: 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