The E-peak distribution of the GRBs detected by HETE FREGATE instrument

Details The E-peak distribution of the GRBs detected by HETE FREGATE instrument The E-peak distribution of the GRBs detected by HETE FREGATE instrument

2002-04-24

arxiv.org/abs/astro-ph/0204407v1

AIP Conf.Proc. 662 (2003) 59-62

Astronomy and Astrophysics

Astrophysics

3 pages, Woods Hole Proceedings

Scientific paper

10.1063/1.1579300

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.

Affiliated with

Also associated with

No associations

Rating

The E-peak distribution of the GRBs detected by HETE FREGATE instrument does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The E-peak distribution of the GRBs detected by HETE FREGATE instrument, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The E-peak distribution of the GRBs detected by HETE FREGATE instrument will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-646