A first test of a sine-Hough method for the detection of pulsars in binary systems using the E4 Virgo engineering run data

Details A first test of a sine-Hough method for the detection of pulsars in binary systems using the E4 Virgo engineering run data A first test of a sine-Hough method for the detection of pulsars in binary systems using the E4 Virgo engineering run data

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004cqgra..21s.717y&link_type=abstract

Classical and Quantum Gravity, Volume 21, Issue 5, pp. S717-S727 (2004).

Physics

Scientific paper

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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