A first comparison of search methods for gravitational wave bursts using LIGO and Virgo simulated data

被引：15
作者：
Beauville, F
Bizouard, MA
Blackburn, L
Bosi, L
Brady, P
Brocco, L
Brown, D
Buskulic, D
Chatterji, S
Christensen, N
Clapson, AC
Fairhurst, S
Grosjean, D
Guidi, G
Hello, P
Katsavounidis, E
Knight, M
Lazzarini, A
Marion, F
Mours, B
Ricci, F
Viceré, A
Zanolin, M
机构：
[1] Lab Annecy Le Vieux Phys Particules, F-74941 Annecy Le Vieux, France
[2] Univ Paris 11, LAL, IN2P3, CNRS, F-91898 Orsay, France
[3] MIT, LIGO, Cambridge, MA 02139 USA
[4] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy
[5] Univ Perugia, I-06123 Perugia, Italy
[6] Univ Wisconsin, Milwaukee, WI 53201 USA
[7] Ist Nazl Fis Nucl, Sez Roma, I-00185 Rome, Italy
[8] Univ Roma La Sapienza, I-00185 Rome, Italy
[9] CALTECH, LIGO, Pasadena, CA 91125 USA
[10] Carleton Coll, Northfield, MN 55057 USA
[11] Ist Nazl Fis Nucl, Sez Firenze Urbino, I-50019 Sesto Fiorentino, Italy
[12] Univ Urbino, I-61029 Urbino, Italy
来源：
CLASSICAL AND QUANTUM GRAVITY | 2005年 / 22卷 / 18期
关键词：
D O I：
10.1088/0264-9381/22/18/S43
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present. a comparative study of six search methods for gravitational wave bursts using simulated LIGO and Virgo noise data. The simulated data were generated according to the design sensitivity of the two 4 km LIGO interferometers and the 3 km Virgo interferometer. The searches were applied on replicas of the data sets to which eight different signals were injected. Three figures of merit were employed in this analysis: (a) receiver operator characteristic curves, (b) necessary signal-to-noise ratios for the searches to achieve 50% and 90% efficiencies and (c) variance and bias for the estimation of the arrival time of a gravitational wave burst.
引用
收藏
页码：S1293 / S1301
页数：9
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