New Methods for Offline GstLAL Analyses
Prathamesh Joshi, Leo Tsukada, Chad Hanna, Shomik Adhicary, Debnandini Mukherjee, Wanting Niu, Shio Sakon, Divya Singh, Pratyusava Baral, Amanda Baylor, Kipp Cannon, Sarah Caudill, Bryce Cousins, Jolien D. E. Creighton, Becca Ewing, Heather Fong, Richard N. George

TL;DR
This paper introduces new computational and analytical methods for offline GstLAL gravitational wave searches, significantly improving sensitivity, reliability, and efficiency during the O4 observing run.
Contribution
The paper presents novel techniques for data reuse, combined searches, likelihood adjustments, and background estimation that enhance GstLAL's offline analysis capabilities.
Findings
50%-100% increase in sensitivity for high-mass sources
More reliable significance estimation of gravitational wave candidates
Reduced computational resources and improved reusability of analysis results
Abstract
In this work, we present new methods implemented in the GstLAL offline gravitational wave search. These include a technique to reuse the matched filtering data products from a GstLAL online analysis, which hugely reduces the time and computational resources required to obtain offline results; a technique to combine these results with a separate search for heavier black hole mergers, enabling detections from a larger set of gravitational wave sources; changes to the likelihood ratio which increases the sensitivity of the analysis; and two separate changes to the background estimation, allowing more precise significance estimation of gravitational wave candidates. Some of these methods increase the sensitivity of the analysis, whereas others correct previous mis-estimations of sensitivity by eliminating false positives. These methods have been adopted for GstLAL's offline results during…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
