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.
Testing the performance of a blind burst statistic
VICERE', ANDREA;CONFORTO, GIOVANNI;DOMINICI, PIETRO;GUIDI, GIANLUCA MARIA;MARTELLI, FILIPPO;PERNIOLA, BRUNA;VETRANO, FLAVIO
2003
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.File in questo prodotto:
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