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

页码：S1679 / S1684

页数：6

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