Author(s): Gregory Ashton, Ann-Kristin Malz, and Nicolo Colombo
Gravitational-wave data from advanced-era interferometric detectors consists of background Gaussian noise, frequent transient artifacts, and rare astrophysical signals. Multiple search algorithms exist to detect the signals from compact binary coalescences, but their varying performance complicates … [Phys. Rev. Lett. 136, 011402] Published Thu Jan 08, 2026
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