Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run
Open Access
- 23 April 2024
- journal article
- research article
- Published by National Academy of Sciences in Proceedings of the National Academy of Sciences
- Vol. 121 (18)
Abstract
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.Keywords
All Related Versions
Funding Information
- National Science Foundation (PHY-2010970 OAC-2117997)
- National Science Foundation (PHY-2010970 OAC-2117997)
- National Science Foundation (PHY-2011334 PHY-2308693)
- National Science Foundation (PHY-2011334 PHY-2308693 PHY-2219212)
- National Science Foundation (OAC-2117997 PHY-1764464)
- National Science Foundation (PHY-1764464)
- National Science Foundation (PHY-1764464)
- National Science Foundation (PHY-1764464)
- MEXT | Japan Society for the Promotion of Science (No.~23H04891 No.~23H04893)
- National Science Foundation (PHY-2110576)
- National Science Foundation (PHY-2207728)
- National Science Foundation (PHY-2207728)
- National Science Foundation (PHY-2207728)
- National Science Foundation (PHY-2207728)
- National Science Foundation (PHY-2207728)
- National Science Foundation (PHY-2207728)
- National Science Foundation (PHY-2207728)
This publication has 74 references indexed in Scilit:
- LIGO and Virgo detector characterization and data quality: Contributions to the O3 run and preparation for O4Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2022
- Constraining neutron-star matter with microscopic and macroscopic collisionsNature, 2022
- coherent WaveBurst, a pipeline for unmodeled gravitational-wave data analysisSoftwareX, 2021
- Measuring the Hubble constant with a sample of kilonovaeNature Communications, 2020
- Identification of strontium in the merger of two neutron starsNature, 2019
- A Hubble constant measurement from superluminal motion of the jet in GW170817Nature Astronomy, 2019
- The PyCBC search for gravitational waves from compact binary coalescenceClassical and Quantum Gravity, 2016
- A coherent method for detection of gravitational wave burstsClassical and Quantum Gravity, 2008
- HEALPix: A Framework for High‐Resolution Discretization and Fast Analysis of Data Distributed on the SphereThe Astrophysical Journal, 2005
- A Skyrme parametrization from subnuclear to neutron star densities Part II. Nuclei far from stabilitiesNuclear Physics A, 1998