(15 September 2022 update; next update by 15 November 2022)

LIGO, Virgo, and KAGRA are closely coordinating to start the O4 Observing run together. As a result of the most recent evaluation of the schedule for O4 readiness, we project to start the O4 Observing Run in March 2023, with an Engineering Run to start one month before the observing run begins; low-latency alerts for candidate events identified during engineering time may be released, both to exercise the system and to exploit their scientific value.

The run is planned to start with LIGO Hanford, LIGO Livingston, Virgo, and KAGRA. While the commissioning of the detectors is progressing, the plan towards readiness continues to be reviewed. The updated O4 start date is driven by further unanticipated delays in the detectors’ upgrade and commissioning programs. O5 plans are still in formulation; we note that based on experience during previous observing runs, we anticipate the need in O5 for one or more commissioning breaks of a few months duration each to address issues and make improvements based on observing experience.

The projected sensitivity of the detectors remains unchanged: LIGO projects a sensitivity goal of 160-190 Mpc for binary neutron stars. Virgo projects a target sensitivity of 80-115 Mpc. KAGRA should be running with greater than 1 Mpc sensitivity at the beginning of O4, and will work to improve the sensitivity toward the end of O4.

Please check the OpenLVKEM pages for the timing and coordinates for telemeetings. We plan a call on Sep 22, 2022. After that, we will hold calls on the third Thursday of each month through the end of the year. The schedule of calls is posted at the OpenLVKEM wiki (see below), along with Agenda and pointers to materials.

Reference Material:


The gravitational-wave observing schedule is divided into Observing Runs of operation at a given sensitivity of roughly a year duration, down time for construction and commissioning, and transitional Engineering Runs between commissioning and observing runs. The current best understanding of the long-term observing schedule is shown below. Since BNS (Binary Neutron Star) mergers are a well-studied class of gravitational-wave signals, this figure gives the BNS range for each observing run.

Long-term observing schedule

During O4, we expect that four facilities (LIGO Hanford (LHO) and Livingston (LLO), KAGRA and Virgo) will observe for one year with a month break in the middle. KAGRA is expected to start with Virgo and LIGO, and then step away for commissioning and return to observing with a greater sensitivity toward the end of the O4 run.

The O5 start dates, duration, and sensitivities are current best guesses, and will likely be adjusted as we approach that run.

Live Status

There are a handful of public web pages that report live status of the LIGO/Virgo detectors and alert infrastructure.