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- W2024709687 endingPage "114003" @default.
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- W2024709687 abstract "Binary black holes with total masses between ~20 and 200 M_⊙ require numerical relativity to describe the detectable signal in ground-based, gravitational-wave detectors. The time–frequency properties of the signals suggest that both modeled, matched filter searches and unmodeled, burst searches can expect to detect high mass binary signals. This paper presents a comparison of a matched filter pipeline and two unmodeled burst pipelines on the inspiral, merger and ring-down phases of compact binary coalescence by evaluating the sensitivity to binaries with total masses between 25 and 100 M_⊙ at a fixed false alarm rate. All three algorithms provided an average range of ~250 Mpc for a 50,50 M_⊙ binary at 10^(−7) Hz false alarm rate." @default.
- W2024709687 created "2016-06-24" @default.
- W2024709687 creator A5044522236 @default.
- W2024709687 date "2010-05-10" @default.
- W2024709687 modified "2023-09-25" @default.
- W2024709687 title "Gravitational-wave data analysis overview of compact binary searches using waveforms inspired by numerical relativity" @default.
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- W2024709687 doi "https://doi.org/10.1088/0264-9381/27/11/114003" @default.
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