학술논문
A first test of a sine-Hough method for the detection of pulsars in binary systems using the E4 Virgo engineering run data
Document Type
Article
Author
Yvert, Michel; Collaboration), (for the Virgo; Acernese, F; Amico, P; Arnaud, N; Babusci, D; Barillé, R; Barone, F; Barsotti, L; Barsuglia, M; Beauville, F; Bizouard, M A; Boccara, C; Bondu, F; Bosi, L; Bradaschia, C; Bracci, L; Braccini, S; Brillet, A; Brisson, V; Brocco, L; Buskulic, D; Calamai, G; Calloni, E; Campagna, E; Cavalier, F; Cella, G; Chassande-Mottin, E; Cleva, F; Cokelaer, T; Conforto, G; Corda, C; Coulon, J-P; Cuoco, E; Dattilo, V; Davier, M; Rosa, R De; Fiore, L Di; Virgilio, A Di; Dujardin, B; Eleuteri, A; Enar, D
Source
Classical and Quantum Gravity; March 2004, Vol. 21 Issue: 5 pS717-S727, 11p
Subject
Language
ISSN
02649381; 13616382
Abstract
Most of the known pulsars with frequencies lying in the best sensitivity range of the Virgo/LIGO/TAMA interferometers belong to binary systems. Accordingly their frequencies are Doppler shifted in an unknown way. We investigate a new method to search for and extract the parameters of such pulsars. A first preliminary test of this method, performed on the Virgo data recorded during the E4 engineering run, is presented.