GstLAL O4 Online Results Paper
Shomik Adhicary, Pratyusava Baral, Amanda Baylor, Becca Ewing, Yun-Jing Huang, Rachael Huxford, Prathamesh Joshi, James Kennington, Ryan Magee, Cody Messick, Wanting Niu, Cort Posnansky, Surabhi Sachdev, Shio Sakon, Urja Shah, Divya Singh, Leo Tsukada, Zach Yarbrough, Noah Zhang

TL;DR
The paper reports on the performance and results of the GstLAL real-time gravitational-wave analysis during LIGO-Virgo-KAGRA's O4 run, highlighting low latency detection and high operational uptime.
Contribution
It provides the first comprehensive report on GstLAL's real-time detection capabilities and its role in the O4 gravitational-wave observing run.
Findings
Median latency of 15.8 seconds for candidate uploads
98% operational uptime during the run
88% of significant events identified in low latency
Abstract
Gravitational-wave observations of merging binary neutron stars and black holes are now routinely made by detectors in the Advanced LIGO-Virgo-KAGRA network. Neutron star binary systems may also produce detectable electromagnetic and particle emission over times scales ranging from seconds to years. Real-time gravitational-wave searches play a central role in enabling time-critical electromagnetic and/or neutrino follow-up observations. During the fourth observing run (O4) of the Advanced LIGO-Virgo-KAGRA network, multiple real-time searches operated continuously to identify candidate gravitational-wave events and publicly disseminate information about these discoveries. Here, the performance and results of the GstLAL real-time analysis are reported. The analysis is designed to identify candidates with low latency, high detection efficiency, and sustained operational uptime over long…
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