Timing Analysis of Unusual GRB 090709A Observed by Suzaku Wide-band All sky Monitor
- Saitama University, 255 Shimo-Okubo, Sakura, Saitama, 338-8570 (Japan)
- ISAS/JAXA, 3-1-1 Yoshinodai, Sagamihara, Kanagawa, 229-8510 (Japan)
- Stanford Linear Accelerator Center, Menlo Park, CA 94025 (United States)
- Institute of Physical and Chemical Research (RIKEN), 2-1 Hirosawa, Wako, Saitama 351-0198 (Japan)
- Aoyama Gakuin University, 5-10-1 Fuchinobe, Sagamihara, 229-8558 (Japan)
- University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo, 113-0033 (Japan)
A result of a joint timing analysis is presented for prompt emission of long-duration (T90 = 81 s) GRB 090709A with Swift Burst Alert Telescope (Swift/BAT), Suzaku Wide-band All-sky Monitor (Suzaku/WAM) and Konus-Wind over an energy range from 15 keV to 5 MeV. It was reported that multi-peaked GRB 090709A exhibited a possible periodic behavior with a period of about 8 s which is comparable to typical time scale of soft gamma-ray repeaters. However, the periodicity is still marginal in detailed analysis with Swift/BAT and GRB090709A exhibited a typical afterglow[1][2]. To investigate significance of the periodicity more quantitatively, we performed a detailed timing analysis on all the lightcurves obtained with Suzaku/WAM, Swift/BAT, and Konus-Wind evaluating their underlying trend, red noise and white noise.
- OSTI ID:
- 21439608
- Journal Information:
- AIP Conference Proceedings, Vol. 1279, Issue 1; Conference: Conference on deciphering the ancient universe with gamma-ray bursts, Kyoto (Japan), 19-23 Apr 2010; Other Information: DOI: 10.1063/1.3509358; (c) 2010 American Institute of Physics; ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
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