Search method for unmodeled transient gravitational waves associated with SGR flares

被引：18

作者：

Kalmus, P. ^{[1
]}

Khan, R. ^{[1
]}

Matone, L. ^{[1
]}

Marka, S. ^{[1
]}

机构：

[1] Columbia Univ, New York, NY 10027 USA

来源：

CLASSICAL AND QUANTUM GRAVITY | 2007年 / 24卷 / 19期

关键词：

D O I：

10.1088/0264-9381/24/19/S28

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We describe a method for searching for transient gravitational waves associated with soft gamma-ray repeater (SGR) flares or other burst-like events using data collected by interferometric gravitational wave detectors. The method can be used to analyze data from either a single detector or from two detectors coherently. The excess power-type algorithm creates event sets from conditioned detector data which may be compared to signal simulations of known strength based on plausible waveform classes. Estimated search sensitivities obtained by performing two-detector searches on the simulated data are presented. In the case of 22 ms duration white noise bursts in the 100-200 Hz band injected into simulated noise, we find a characteristic strain sensitivity h(rss)(90%) = 3.0 x 10(-22) Hz(-1/2).

引用

页码：S659 / S669

页数：11

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