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.

A First Test of a Sine-Hough Method for Detection of Pulsars in Binary Systems using the E4 Virgo Test Run Data

ACERNESE, Fausto;BARONE, Fabrizio;
2004

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.
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11386/2501329
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