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Published July 5, 2012 | Published
Journal Article Open

Summed parallel infinite impulse response filters for low-latency detection of chirping gravitational waves

Abstract

With the upgrade of current gravitational wave detectors, the first detection of gravitational wave signals is expected to occur in the next decade. Low-latency gravitational wave triggers will be necessary to make fast follow-up electromagnetic observations of events related to their source, e.g., prompt optical emission associated with short gamma-ray bursts. In this paper we present a new time-domain low-latency algorithm for identifying the presence of gravitational waves produced by compact binary coalescence events in noisy detector data. Our method calculates the signal to noise ratio from the summation of a bank of parallel infinite impulse response filters. We show that our summed parallel infinite impulse response method can retrieve the signal to noise ratio to greater than 99% of that produced from the optimal matched filter.

Additional Information

© 2012 American Physical Society. Received 16 August 2011; published 5 July 2012. We would like to thank Kipp Cannon, Drew Keppel and Chad Hanna for detailed discussion on the design and implementation of low-latency detection algorithms. This work was done in part during the LIGO Visiting Student Researcher program, which was partially funded by the 2009 UWA Research Collaboration Award. This research was supported by the Australian Research Council. S. H. gratefully acknowledges the support of an Australian Postgraduate Award. L.W. acknowledges the support of the Australian Research Council Discovery Grants and Future Fellow program.

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August 19, 2023
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October 18, 2023