As the field of gravitational wave astronomy strides rapidly towards its rst
direct detection, developing e cient data analysis strategies become crucial
due to the low signal to noise ratio in the data. The noise level ...
The interferometric data from gravitational wave detectors is neither Gaussian nor stationary
and contains noise transients or glitches. These glitches interfere with the search algorithms
by producing high SNR triggers. ...
The LIGO and VIRGO Detectors have conducted two observation runs, in which a total of ten
binary black-hole mergers and neutron star mergers have been detected. The third observation run has already seen several potential ...
The analysis of stochastic gravitational wave background involves the cross-correlation of signals detected by the two detectors at short time intervals augmented by a filter to optimize the signal to noise ratio. The ...