A weakly-modeled search for compact binary coalescences in Einstein Telescope
Adrian Macquet, Tito Dal Canton, Tania Regimbau

TL;DR
This paper evaluates an unmodelled gravitational wave search pipeline for the Einstein Telescope, demonstrating its ability to detect a significant fraction of compact binary coalescence signals with low computational cost, suitable for real-time analysis.
Contribution
It presents a performance assessment of a low-cost, unmodelled GW search pipeline tailored for the Einstein Telescope, highlighting its detection capabilities for CBC signals.
Findings
Recovers 38% of injected CBC signals, including 89% of high-mass systems.
Accurately estimates BNS chirp mass with 1.3% precision.
Sensitivity to other long-duration signals is only marginally affected.
Abstract
Einstein Telescope (ET) is a project of third generation gravitational wave (GW) detector with a planned sensitivity 10 times better than current detectors such as Advanced LIGO and Advanced Virgo. The high rate of GW signals expected in the data will pose several data analysis challenges, like the ability to disentangle overlapping signals or the need to dimension the computational resources required to treat all the candidate events. We explore the behaviour and the performances of a data analysis pipeline designed to search for unmodelled GW signals with duration 1 to 1000 s on a mock dataset that consists of 1 month of data following ET design sensitivity on top of which is added a realistic distribution of compact binary coalescence (CBC) signals. Unmodelled searches are intrinsically less sensitive to CBC signals than template-based searches, but are computationally cheaper and…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Astronomical Observations and Instrumentation
