In this work we estimate the performance of a method for the detection of burst events in the data produced by interferometric gravitational wave detectors. We compute the receiver operating characteristics in the specific case of a simulated noise having the spectral density expected for Virgo, using test signals taken from a library of possible waveforms emitted during the collapse of the core of Type II Supernovae.
@article{arxiv.gr-qc/0304022,
title = {Testing the performance of a blind burst statistic},
author = {A. Vicere' and G. Calamai and E. Campagna and G. Conforto and E. Cuoco and P. Dominici and I. Fiori and G. M. Guidi and G. Losurdo and F. Martelli and M. Mazzoni and B. Perniola and R. Stanga and F. Vetrano},
journal= {arXiv preprint arXiv:gr-qc/0304022},
year = {2009}
}
Comments
8 pages, 6 figures, Talk given at the GWDAW2002 workshop