Improved ranking statistics of the GstLAL inspiral search for compact binary coalescences
Leo Tsukada, Prathamesh Joshi, Shomik Adhicary, Richard George, Andre, Guimaraes, Chad Hanna, Ryan Magee, Aaron Zimmerman, Pratyusava Baral, Amanda, Baylor, Kipp Cannon, Sarah Caudill, Bryce Cousins, Jolien D. E. Creighton,, Becca Ewing, Heather Fong, Patrick Godwin

TL;DR
This paper introduces new features for the GstLAL inspiral search pipeline, significantly enhancing its sensitivity to gravitational waves from compact binary coalescences for upcoming observing runs.
Contribution
The paper presents novel ranking statistic features, including contamination removal and model upgrades, tailored for the expanded detector network and improved sensitivities.
Findings
Sensitivity improved by 15-20% with new features
Enhanced detection capabilities for upcoming observing runs
Integration of KAGRA detector into the pipeline
Abstract
Starting from May 2023, the LIGO Scientific, Virgo and KAGRA Collaboration is planning to conduct the fourth observing run with improved detector sensitivities and an expanded detector network including KAGRA. Accordingly, it is vital to optimize the detection algorithm of low-latency search pipelines, increasing their sensitivities to gravitational waves from compact binary coalescences. In this work, we discuss several new features developed for ranking statistics of GstLAL-based inspiral pipeline, which mainly consist of: the signal contamination removal, the bank- incorporation, the upgraded signal model and the integration of KAGRA. An injection study demonstrates that these new features improve the pipeline's sensitivity by approximately 15% to 20%, paving the way to further multi-messenger observations during the upcoming observing run.
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Taxonomy
TopicsScientific Research and Discoveries · Astronomical Observations and Instrumentation · Astronomy and Astrophysical Research
