Long-duration transient, gravitational-wave search pipeline
Adrian Macquet, Marie-Anne Bizouard, Nelson Christensen, Michael, Coughlin

TL;DR
This paper introduces a new gravitational-wave data analysis pipeline optimized for detecting long-duration, unmodeled transient signals, significantly improving sensitivity and reducing computational costs compared to previous methods.
Contribution
The paper presents a novel pipeline for long-duration gravitational-wave transients that enhances detection efficiency and computational speed, adaptable to multiple detector networks.
Findings
Detection efficiency increased depending on signal morphology
Computing time reduced by at least a factor of 10
Generalized to arbitrary detector networks
Abstract
As the sensitivity and observing time of gravitational-wave detectors increase, a more diverse range of signals is expected to be observed from a variety of sources. Especially, long-lived gravitational-wave transients have received interest in the last decade. Because most of long-duration signals are poorly modeled, detection must rely on generic search algorithms, which make few or no assumption on the nature of the signal. However, the computational cost of those searches remains a limiting factor, which leads to sub-optimal sensitivity. Several detection algorithms have been developed to cope with this issue. In this paper, we present a new data analysis pipeline to search for un-modeled long-lived transient gravitational-wave signals with duration between 10 and 1000 s, based on an excess cross-power statistic in a network of detectors. The pipeline implements several new features…
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