Plans for the LIGO-TAMA joint search for gravitational wave bursts

被引：5

作者：

Sutton, PJ ^{[1
]}

Ando, M

Brady, P

Cadonati, L

Di Credico, A

Fairhurst, S

Finn, LS

Kanda, N

Katsavounidis, E

Klimenko, S

Lazzarini, A

Marka, S

McNabb, JWC

Majumder, SR

Saulson, PR

Tagoshi, H

Takabashi, H

Takahashi, R

Tatsumi, D

Tsunesada, Y

Whitcomb, SE

机构：

[1] CALTECH, LIGO Lab, Pasadena, CA 91125 USA

[2] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan

[3] Univ Wisconsin, Dept Phys, Milwaukee, WI 53201 USA

[4] MIT, LIGO Lab, Cambridge, MA 02139 USA

[5] Syracuse Univ, Dept Phys, Syracuse, NY 13244 USA

[6] Penn State Univ, Dept Phys, Ctr Gravitat Wave Phys, University Pk, PA 16802 USA

[7] Osaka City Univ, Grad Sch Sci, Dept Phys, Sumiyoshi Ku, Osaka 5588585, Japan

[8] Univ Florida, Dept Phys, Gainesville, FL 32611 USA

[9] Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Toyonaka, Osaka 5600043, Japan

[10] Niigata Univ, Grad Sch Sci & Technol, Niigata 9502181, Japan

[11] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan

[12] Natl Astron Observ, Mitaka, Tokyo 1818588, Japan

来源：

CLASSICAL AND QUANTUM GRAVITY | 2004年 / 21卷 / 20期

关键词：

D O I：

10.1088/0264-9381/21/20/023

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We describe the plans for a joint search for unmodelled gravitational wave bursts being carried out by the LIGO and TAMA Collaborations using data collected during February-April 2003. We take a conservative approach to detection, requiring candidate gravitational wave bursts to be seen in coincidence by all four interferometers. We focus on some of the complications of performing this coincidence analysis, in particular the effects of the different alignments and noise spectra of the interferometers.

引用

页码：S1801 / S1807

页数：7

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