Considerations on coincidence experiments between two gravitational wave detectors for sources in the Galactic Centre

Details Considerations on coincidence experiments between two gravitational wave detectors for sources in the Galactic Centre Considerations on coincidence experiments between two gravitational wave detectors for sources in the Galactic Centre

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26a...421..811b&link_type=abstract

Astronomy and Astrophysics, v.421, p.811-813 (2004)

Astronomy and Astrophysics

Astrophysics

2

Gravitational Waves, Methods: Data Analysis, Methods: Numerical

Scientific paper

In a coincidence experiment between gravitational wave detectors, the sidereal time analysis can provide very useful and powerful indications. We studied, with the help of a MonteCarlo simulation, the sidereal time pattern to be expected in such an experiment in the particular case of the resonant bars NAUTILUS and EXPLORER and for sources located in the Galactic Centre. It is shown that for linearly polarized gravitational waves the sidereal time pattern exhibits just a large peak at hour 3.5 and only a small peak at about hour 12.

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