Confirmation of the E peak src-E iso (Amati) relation from the X-ray flash XRF 050416A observed by Swift/BAT

T. Sakamoto*, L. Barbier, S. Barthelmy, J. Cummings, E. Fenimore, N. Gehrels, D. Hullinger, H. Krimm, C. Markwardt, D. Palmer, A. Parsons, G. Sato, J. Tueller

*この研究の対応する著者

研究成果: Conference contribution

抄録

We report Swift Burst Alert Telescope (BAT) observations of the X-ray Flash (XRF) XRF 050416A. The fluence ratio between the 15-25 and 25-50 keV bands of this event is 1.1, thus making it the softest gamma-ray burst (GRB) observed by BAT so far. The spectrum is well fitted by the Band function with E peak obs of 15.6 -2.7 +2.3keV. Assuming the redshift of the host galaxy (z=0.6535), the isotropic-equivalent energy E iso and the E peak energy at the GRB rest frame (E peak src) of XRF 050416A are not only consistent with the correlation found by Amati et al. and extended to XRFs by Sakamoto et al., but also fill-in the gap of this relation around 30-80 keV range of E peak src. This result tightens the validity of the E peak src-E iso relation form XRFs to GRBs.

本文言語English
ホスト出版物のタイトルAIP Conference Proceedings
ページ578-581
ページ数4
836
DOI
出版ステータスPublished - 2006 5 19
イベントGAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference - Washington, D.C.
継続期間: 2005 11 292005 12 2

Other

OtherGAMMA-RAY BURSTS IN THE SWIFT ERA: 16th Maryland Astrophysics Conference
CityWashington, D.C.
Period05/11/2905/12/2

ASJC Scopus subject areas

  • 物理学および天文学(全般)

フィンガープリント

「Confirmation of the E <sub>peak</sub> <sup>src</sup>-E <sub>iso</sub> (Amati) relation from the X-ray flash XRF 050416A observed by Swift/BAT」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。

引用スタイル