Testing the performance of a blind burst statistic

A Viceré; 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

doi:10.1088/0264-9381/20/17/325

Classical and Quantum Gravity

Testing the performance of a blind burst statistic

A Viceré^1,2, G Calamai^2,3, E Campagna^2,4, G Conforto¹, E Cuoco², P Dominici¹, I Fiori^1,2, G M Guidi^1,2, G Losurdo², F Martelli^1,2, M Mazzoni^2,4, B Perniola^1,2, R Stanga^2,4 and F Vetrano^1,2

Published 18 August 2003 • Published under licence by IOP Publishing Ltd
Classical and Quantum Gravity, Volume 20, Number 17 Citation A Viceré et al 2003 Class. Quantum Grav. 20 S821 DOI 10.1088/0264-9381/20/17/325

Download Article PDF

Article metrics

25 Total downloads

Submit

Submit to this Journal

Permissions

Get permission to re-use this article

Author affiliations

¹ Istituto di Fisica, Università di Urbino, Italy

² Istituto Nazionale di Fisica Nucleare, Sez. Firenze/Urbino, Italy

³ Osservatorio Astrofisico di Arcetri, Firenze, Italy

⁴ Dipartimento di Astronomia, Università di Firenze, Italy

Dates

Received 7 April 2003
Published 18 August 2003

Buy this article in print

Journal RSS

Sign up for new issue notifications

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.

Export citation and abstract BibTeX RIS

Previous article in issue

Next article in issue

Please wait… references are loading.

Testing the performance of a blind burst statistic

Article metrics

Submit

Permissions

Share this article

Author affiliations

Dates

Abstract