Observing Run

The term Observing Run is currently used for surveys carried out by gravitational-wave detectors to detect gravitational waves (GW detections). They typically run for a few months, the time between used for maintenance and upgrades. Currently, the different GW detection efforts coordinate, attempting to operate over the same such time-periods: a number of detections of each detected event offers considerable value: simultaneous detections provide clearer confirmation that the event truly occurred (i.e., the detection wasn't merely noise), and offers data regarding to the direction of the source, increasing the chances of establishing a counterpart transient such as an optical transient or gamma-ray burst. The Observing Runs so far have been numbered 1 through 4, with letter suffixes to indicate subdivisions of the run (e.g., 4a, 4b), typically separated by periods of a few weeks for maintenance and minor upgrades. Between the full runs are longer outages, typically for substantial upgrades, which require on the order of a year or more. Observing Runs:

Note that in some of these, Virgo and KAGRA did not operate for the run's entire time interval.

Initial development and testing of these detectors lasted for years, including successive upgrades and some pilot operation. Among LIGO's pilot runs were six labeled Science Runs (1 through 6), during which there were no detections.