Abstract
In this work we propose a new strategy for gravitational waves detection from coalescing binaries, using Adaptive Line Enhancer filters. An analysis of the filters performance is shown in terms of the tracking capability and determination of filter parameters. Furthermore, receiver operating characteristics are derived, by extensive Monte Carlo simulation studies. Some tests have been performed on simulated Virgo noise, demonstrating that adaptive filters are promising both for the small computational power needed (with respect to the matched filter) and for the statistical robustness of the algorithms used.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
