Methods to characterize non-Gaussian noise in TAMA

Details Methods to characterize non-Gaussian noise in TAMA Methods to characterize non-Gaussian noise in TAMA

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cqgra..20s.697a&link_type=abstract

Classical and Quantum Gravity, Volume 20, Issue 17, pp. S697-S709 (2003).

Physics

9

Scientific paper

We present a data characterization method for the main output signal of the interferometric gravitational-wave detector, in particular targetting at effective detection of burst gravitational waves from stellar core collapse. The time scale of non-Gaussian events is evaluated in this method, and events with longer time scale than real signals are rejected as non-Gaussian noises. As a result of data analysis using 1000 h of real data with the interferometric gravitational-wave detector TAMA300, the false-alarm rate was improved 103 times with this non-Gaussian noise evaluation and rejection method.

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