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An efficient Matched Filtering Algorithm for the Detection of Continuous Gravitational Wave Signals
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We describe an efficient method of matched filtering over long (greater than 1 day) time baselines starting from Fourier transforms of short durations (roughly 30 minutes) of the data stream. This method plays a crucial role in the search algorithm developed by Schutz and Papa for the detection of continuous gravitational waves from pulsars. Also, we discuss the computational cost--saving approximations used in this method, and the resultant performance of the search algorithm.
Forward citations
Cited by 2 Pith papers
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One-stop strategy to search for long-duration gravitational-wave signals
A generic GPU search engine plus a fast semianalytic sensitivity estimator could make blind continuous gravitational-wave searches much cheaper to run and characterize.
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The WDM Time-Frequency Transform in Gravitational-Wave Data Analysis I: Formalism
Derives and documents the WDM basis properties, forward/inverse transforms, and time-frequency likelihood for gravitational-wave data analysis.
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