A power filter for the detection of burst sources of gravitational radiation in interferometric detectors

被引:19
作者
Anderson, WG
Brady, PR
Creighton, JDE
Flanagan, ÉÉ
机构
[1] Univ Wisconsin, Dept Phys, Milwaukee, WI 53201 USA
[2] Cornell Univ, Newman Lab, Ithaca, NY 14853 USA
来源
INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2000年 / 9卷 / 03期
基金
美国国家科学基金会;
关键词
D O I
10.1142/S0218271800000323
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a filter for detecting gravitational wave signals from burst sources. This filter requires only minimal advance knowledge of the expected signal: i.e. the signal's frequency band and time duration. It consists of a threshold on the total power in the data stream in the specified signal band during the specified time. This filter is optimal (in the Neyman-Pearson sense) for signal searches where only this minimal information is available.
引用
收藏
页码:303 / 307
页数:5
相关论文
共 10 条
[1]   Time-frequency detection of gravitational waves [J].
Anderson, WG ;
Balasubramanian, R .
PHYSICAL REVIEW D, 1999, 60 (10)
[2]  
ANDERSON WW, UNPUB
[3]   Detection of gravitational wave bursts by interferometric detectors [J].
Arnaud, N ;
Cavalier, F ;
Davier, M ;
Hello, P .
PHYSICAL REVIEW D, 1999, 59 (08) :1-9
[4]  
FEO M, 1996, E AMOLDI FDN SERIES, V2
[5]   OBSERVING BINARY INSPIRAL IN GRAVITATIONAL-RADIATION - ONE INTERFEROMETER [J].
FINN, LS ;
CHERNOFF, DF .
PHYSICAL REVIEW D, 1993, 47 (06) :2198-2219
[6]   Measuring gravitational waves from binary black hole coalescences. I. Signal to noise for inspiral, merger, and ringdown [J].
Flanagan, EE ;
Hughes, SA .
PHYSICAL REVIEW D, 1998, 57 (08) :4535-4565
[7]  
Kassam SA., 2012, SIGNAL DETECTION NON
[8]  
MOHANTY SD, GRQC9910027
[9]  
THORNE KS, 1995, P SNOWM 95 SUMM STUD
[10]  
Wainstein LA., 1962, Extraction of Signals from Noise. Dover Books on Physics and Mathematical Physics