Current Status of TAMA300 Online Search for Inspiraling Binaries

Details Current Status of TAMA300 Online Search for Inspiraling Binaries Current Status of TAMA300 Online Search for Inspiraling Binaries

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....5.3063t&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

A gravitational wave detector of TAMA300 was pioneer in development of interferometric one with over one hundred meter scale. We archived long-term observations over one hundred hours with sufficient sensitivity to monitor within our galaxy [1, 2]. This was marvelous step to the first and direct detection of gravitational wave signals. In such long-term observations, online processes are important for the detector operation and for the signal search. By fo cusing on the most promising source of neutron star binaries, we make a brief intro duction to the online processes.

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