Epeak estimator for gamma-ray bursts observed by the swift burst alert telescope

T. Sakamoto*, G. Sato, L. Barbier, S. D. Barthelmy, J. R. Cummings, E. E. Fenimore, N. Gehrels, D. Hullinger, H. A. Krimm, D. Q. Lamb, C. B. Markwardt, D. M. Palmer, A. M. Parsons, M. Stamatikos, J. Tueller, T. N. Ukwatta

*この研究の対応する著者

研究成果: Article査読

66 被引用数 (Scopus)

抄録

We report a correlation based on a spectral simulation study of the prompt emission spectra of gamma-ray bursts (GRBs) detected by the Swift Burst Alert Telescope (BAT). The correlation is between the Epeak energy, which is the peak energy in the νFν spectrum, and the photon index (Γ) derived from a simple power-law (PL) model. The Epeak- Γ relation, assuming the typical smoothly broken PL spectrum of GRBs, is log Epeak = 3.258-0.829 Γ (1.3 ≤ Γ ≤ 2.3). We take into account not only a range of Epeak energies and fluences, but also distributions for both the low-energy photon index and the high-energy photon index in the smoothly broken PL model. The distribution of burst durations in the BAT GRB sample is also included in the simulation. Our correlation is consistent with the index observed by BAT and Epeak measured by the BAT, and by other GRB instruments. Since about 85% of GRBs observed by the BAT are acceptably fit with the simple PL model because of the relatively narrow energy range of the BAT, this relationship can be used to estimate Epeak when it is located within the BAT energy range.

本文言語English
ページ(範囲)922-935
ページ数14
ジャーナルAstrophysical Journal
693
1
DOI
出版ステータスPublished - 2009 3月 1

ASJC Scopus subject areas

  • 宇宙惑星科学
  • 天文学と天体物理学

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