Testing the performance of a blind burst statistic

Preprint

4 April 2003

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.gr-qc/0304022

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.

Keywords

INTERFEROMETRIC GRAVITATIONAL
WAVEFORMS EMITTED
SPECTRAL DENSITY
DENSITY EXPECTED
BURST STATISTIC
SIGNALS TAKEN
II SUPERNOVAE
BLIND BURST
RECEIVER

All Related Versions

Version 1, 2003-04-04, ArXiv
Published version: Classical and Quantum Gravity, 20 (17), S821.

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