Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run.
Sushant Sharma ChaudharyAndrew ToivonenGaurav WaratkarGeoffrey MoDeep ChatterjeeSarah AntierPatrick BrockillMichael W CoughlinReed EssickShaon GhoshSoichiro MorisakiPratyusava BaralAmanda BaylorNaresh AdhikariPatrick BradyGareth Cabourn DaviesTito Dal CantonMarco CavagliaJolien CreightonSunil ChoudharyYu-Kuang ChuPatrick ClearwaterLuke DavisThomas DentMarco DragoBecca EwingPatrick GodwinWeichangfeng GuoChad HannaRachael HuxfordIan HarryErik KatsavounidisManoj KovalamAlvin K Y LiRyan MageeEthan MarxDuncan MeacherCody MessickXan Morice-AtkinsonAlexander PaceRoberto De PietriBrandon PiotrzkowskiSoumen RoySurabhi SachdevLeo P SingerDivya SinghMarek SzczepanczykDaniel TangMax TrevorLeo TsukadaVerónica Villa-OrtegaLinqing WenDaniel WysockiPublished in: Proceedings of the National Academy of Sciences of the United States of America (2024)
Multimessenger searches for binary neutron star (BNS) and neutron star-black hole (NSBH) mergers are currently one of the most exciting areas of astronomy. The search for joint electromagnetic and neutrino counterparts to gravitational wave (GW)s has resumed with ALIGO's, AdVirgo's and KAGRA's fourth observing run (O4). To support this effort, public semiautomated data products are sent in near real-time and include localization and source properties to guide complementary observations. In preparation for O4, we have conducted a study using a simulated population of compact binaries and a mock data challenge (MDC) in the form of a real-time replay to optimize and profile the software infrastructure and scientific deliverables. End-toend performance was tested, including data ingestion, running online search pipelines, performing annotations, and issuing alerts to the astrophysics community. We present an overview of the low-latency infrastructure and the performance of the data products that are now being released during O4 based on the MDC. We report the expected median latency for the preliminary alert of full bandwidth searches (29.5 s) and show consistency and accuracy of released data products using the MDC. We report the expected median latency for triggers from early warning searches (-3.1 s), which are new in O4 and target neutron star mergers during inspiral phase. This paper provides a performance overview for LIGO-Virgo-KAGRA (LVK) low-latency alert infrastructure and data products using theMDCand serves as a useful reference for the interpretation of O4 detections.