Analysis methods for burst gravitational waves with TAMA data

被引：8
|
作者：
Ando, M
Arai, K
Nagano, S
Takahashi, R
Sato, S
Tatsumi, D
Tsunesada, Y
Kanda, N
Kawamura, S
Beyersdorf, P
Zhu, ZH
Numata, K
Iida, Y
Aso, Y
Mio, N
Moriwaki, S
Somiya, K
Miyoki, S
Kondo, K
Takahashi, H
Hayama, K
Tagoshi, H
Fujimoto, MK
Tsubono, K
Kuroda, K
机构：
[1] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan
[2] Natl Astron Observ Japan, TAMA project, Tokyo, Japan
[3] Osaka City Univ, Dept Phys, Osaka 558, Japan
[4] Univ Tokyo, Dept Adv Mat Sci, Tokyo, Japan
[5] Univ Tokyo, Inst Cosm Ray Res, Tokyo, Japan
[6] Niigata Univ, Dept Phys, Niigata 95021, Japan
[7] Univ Tokyo, Dept Astron, Tokyo 113, Japan
[8] Osaka Univ, Dept Earth & Space Sci, Osaka, Japan
来源：
CLASSICAL AND QUANTUM GRAVITY | 2004年 / 21卷 / 20期
关键词：
D O I：
10.1088/0264-9381/21/20/010
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We describe analysis methods and results for burst gravitational waves with data obtained in the eighth observation run by the TAMA300 detector. In this analysis, we used an excess-power filter for signal detection, and two types of veto for fake-event rejection; one is a time-scale selection of events and the other is a veto with auxiliary information recorded together with the main signal. We generated an event-candidate list with this analysis procedure, which will be used for coincidence analysis with the other detectors.
引用
收藏
页码：S1679 / S1684
页数：6
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