Open Data from LIGO, Virgo, and KAGRA through the First Part of the Fourth Observing Run
gr-qc, astro-ph.HE
Submitted: 2025-08-25
Updated: 2026-09-16
Comments: 26 pages. The version updates Table 3, updates the author list, removes one figure, and updates some text for clarity and grammar
Journal ref: The Astrophysical Journal, 2026, Volume 1004, Number 2, Page 232
Code: https://github.com/gwosc-tutorial/introduction_gwosc_
Project page: https://gwosc.org
License: http://creativecommons.org/licenses/by/4.0/
The gist: LIGO, Virgo, and KAGRA form a network of gravitational-wave observatories.
Terminology
Abstract
LIGO, Virgo, and KAGRA form a network of gravitational-wave observatories. Data and analysis results from this network are made publicly available through the Gravitational Wave Open Science Center. This paper describes open data from this network, including the addition of data from the first part of the fourth observing run and selected periods from the preceding engineering run, collected from 2023 May to 2024 January. The public dataset includes calibrated strain time series for each instrument, data from additional channels used for noise subtraction and detector characterization, and analysis data products from version 4.0 of the Gravitational-Wave Transient Catalog.
Sources
- GWTC-4.0: An Introduction to Version 4.0 of the Gravitational-Wave Transient Catalog
- GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
- GWTC-4.0: Methods for Identifying and Characterizing Gravitational-wave Transients
- All-sky search for short gravitational-wave bursts in the first part of the fourth LIGO-Virgo-KAGRA observing run
- Photon Calibration Performance of KAGRA during the 4th Joint Observing Run (O4)
- GW231123: a Binary Black Hole Merger with Total Mass 190-265 $M_{\odot}$
- Performance of iDQ ahead of LIGO, Virgo, and KAGRA's fourth observing run
- Characterization of systematic error in Advanced LIGO calibration in the second half of O3
- Toward Low-Latency, High-Fidelity Calibration of the LIGO Detectors with Enhanced Monitoring Tools
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