2005/04/13 by L. Blackburn, F. Beauville, M. -A. Bizouard +20
Physics and Astronomy · #gr-qc
published as Class.Quant.Grav. 22 (2005) S1293-S1302 · GWDAW9 proceedings
arxiv created 2005/04/13 · arxiv updated 2009/12/01
We present a comparative study of 6 search methods for gravitational wave bursts using simulated LIGO and Virgo noise data. The data's spectra were chosen to follow the design sensitivity of the two 4km LIGO interferometers and the 3km Virgo interferometer. The searches were applied on replicas of the data sets to which 8 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 percent and 90 percent efficiencies, and (c) variance and bias for the estimation of the arrival time of a gravitational wave burst.