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Testing the performance of a blind burst statistic

A. Vicere'·G. Calamai·E. Campagna·G. Conforto·E. Cuoco·P. Dominici·I. Fiori·G. M. Guidi·G. Losurdo·F. Martelli·M. Mazzoni·B. Perniola·R. Stanga·F. Vetrano
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Abstract

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.

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A. Vicere', G. Calamai, E. Campagna, G. Conforto, E. Cuoco, P. Dominici, I. Fiori, G. M. Guidi, G. Losurdo, F. Martelli, M. Mazzoni, B. Perniola, R. Stanga, F. Vetrano. 2003-04-04. Testing the performance of a blind burst statistic. https://doi.org/10.1088/0264-9381%2F20%2F17%2F325

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