In this paper, we describe the analysis performed in the data of C6 and C7 commissioning runs of Virgo for the search of periodic sources of gravitational waves. The analysis is all-sky, covers the frequency range between 50 Hz and 1050 Hz an d neutron star spin-down rate below 1.58 x 10(-8) Hz s(-1). Coincidences in the source parameter space between candidates found in the two data sets are required to reduce the false alarm probability. The procedure used to estimate the detection efficienc y of the analysis pipeline, through the injection of simulated signals in the data, is also described.

Acernese, F., Amico, P., Alshourbagy, M., Antonucci, F., Aoudia, S., Astone, P., et al. (2007). Coincidence analysis between periodic source candidates in C6 and C7 Virgo data. CLASSICAL AND QUANTUM GRAVITY, 24(19), S491-S499 [10.1088/0264-9381/24/19/S12].

Coincidence analysis between periodic source candidates in C6 and C7 Virgo data

Cuoco E;
2007

Abstract

In this paper, we describe the analysis performed in the data of C6 and C7 commissioning runs of Virgo for the search of periodic sources of gravitational waves. The analysis is all-sky, covers the frequency range between 50 Hz and 1050 Hz an d neutron star spin-down rate below 1.58 x 10(-8) Hz s(-1). Coincidences in the source parameter space between candidates found in the two data sets are required to reduce the false alarm probability. The procedure used to estimate the detection efficienc y of the analysis pipeline, through the injection of simulated signals in the data, is also described.
2007
Acernese, F., Amico, P., Alshourbagy, M., Antonucci, F., Aoudia, S., Astone, P., et al. (2007). Coincidence analysis between periodic source candidates in C6 and C7 Virgo data. CLASSICAL AND QUANTUM GRAVITY, 24(19), S491-S499 [10.1088/0264-9381/24/19/S12].
Acernese, F; Amico, P; Alshourbagy, M; Antonucci, F; Aoudia, S; Astone, P; Avino, S; Babusci, D; Ballardin, G; Barone, F; Barsotti, L; Barsuglia, M; B...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/998601
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