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- W2030602716 abstract "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." @default.
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- W2030602716 date "2003-08-11" @default.
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- W2030602716 title "Methods to characterize non-Gaussian noise in TAMA" @default.
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- W2030602716 doi "https://doi.org/10.1088/0264-9381/20/17/313" @default.
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