GRB 050117: Simultaneous gamma-ray and X-ray observations with the swift satellite

Joanne E. Hill*, David C. Morris, Takanori Sakamoto, Goro Sato, David N. Burrows, Lorella Angelini, Claudio Pagani, Alberto Moretti, Antony F. Abbey, Scott Barthelmy, Andrew P. Beardmore, Vadim V. Biryukov, Sergio Campana, Milvia Capalbi, Giancarlo Cusumano, Paolo Giommi, Mansur A. Ibrahimov, Jamie Kennea, Shiho Kobayashi, Kunihito IokaCraig Markwardt, Peter Mész, Paul T. O'Brien, Julian P. Osborne, Alexei S. Pozanenko, Matteo Perri, Vasilij V. Rumyantsev, Patricia Schady, Dmitri A. Sharapov, Gianpiero Tagliaferri, Bing Zhang, Guido Chincarini, Neil Gehrels, Alan Wells, John A. Nousek

*この研究の対応する著者

研究成果: Article査読

18 被引用数 (Scopus)

抄録

The Swift Gamma-Ray Burst Explorer performed its first autonomous, X-ray follow-up to a newly detected GRB on 2005 January 17, within 193 s of the burst trigger by the Swift Burst Alert Telescope. While the burst was still in progress, the X-Ray Telescope (XRT) obtained a position and an image for an uncataloged X-ray source simultaneously with the gamma-ray observation. The XRT observed flux during the prompt emission was 1.1 × 10-8 ergs cm-2 s-1 in the 0.5-10 keV energy band. The emission in the X-ray band decreased by 3 orders of magnitude within 700 s, following the prompt emission. This is found to be consistent with the gamma-ray decay when extrapolated into the XRT energy band. During the following 6.3 hr, the XRT observed the afterglow in an automated sequence for an additional 947 s, until the burst became fully obscured by the Earth limb. A faint, extremely slowly decaying afterglow, α = -0.21, was detected. Finally, a break in the light curve occurred and the flux decayed with α < -1.2. The X-ray position triggered many follow-up observations: no optical afterglow could be confirmed, although a candidate was identified 3″ from the XRT position.

本文言語English
ページ(範囲)303-310
ページ数8
ジャーナルAstrophysical Journal
639
1 I
DOI
出版ステータスPublished - 2006 3月 1

ASJC Scopus subject areas

  • 宇宙惑星科学

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