arXiv · astro-ph/0204407
The E-peak distribution of the GRBs detected by HETE FREGATE instrument
Abstract
The FREGATE gamma ray detector of HETE-2 is sensitive to photons between 6 and 400 keV. This sensitivity range, extended towards low energies, allows us to explore the emission of GRBs in hard X-rays. We fit the spectra of 23 GRBs with Band's spectral function in order to derive the distribution of their peak energies (E-peak). This distribution is then compared with the E-peak distributions measured by BATSE and GINGA.
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C. Barraud, J. L. Atteia, J. F. Olive, J. P. Dezalay. 2002-04-24. The E-peak distribution of the GRBs detected by HETE FREGATE instrument. https://doi.org/10.1063/1.1579300
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