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.
Vicere A, Calamai G, Campagna E, Conforto G, Cuoco E, Dominici P, et al. (2003). Testing the performance of a blind burst statistic. CLASSICAL AND QUANTUM GRAVITY, 20(17), 821-828 [10.1088/0264-9381/20/17/325].
Testing the performance of a blind burst statistic
Cuoco E;
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:
Eventuali allegati, non sono esposti
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
