Computer Science
Scientific paper
Jun 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010cqgra..27k4003h&link_type=abstract
Classical and Quantum Gravity, Volume 27, Issue 11, pp. 114003 (2010).
Computer Science
1
Scientific paper
Binary black holes with total masses between ~20 and 200 Modot 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 Modot at a fixed false alarm rate. All three algorithms provided an average range of ~250 Mpc for a 50,50 Modot binary at 10-7 Hz false alarm rate.
Hanna Chad
LIGO the
Virgo Scientific Collaborations
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