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Nine years of gravitational waves

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Every detection LIGO, Virgo and KAGRA have published masses for — 282 since September 2015 — placed by the two objects that collided: the heavier one across, the lighter one up, both measured in Suns. Press play to run the nine years a quarter at a time; between observing runs the detectors are dark and nothing arrives. Almost everything crowds the diagonal, because these things pair up with something close to their own size. The strip underneath counts every object on the same scale, and it has a hole in it: of 564 masses here, one falls between 3 and 5 Suns. Tap or hover any detection.

Observing run
Data & source

Data: Gravitational Wave Open Science Center, cumulative Gravitational-Wave Transient Catalog (GWTC-1 through GWTC-5.0), LIGO Scientific / Virgo / KAGRA collaborations — open data, CC BY 4.0 · fetched —. Scope: the 282 catalog entries that carry a published pair of source-frame masses, out of 391 entries in all. The most recent release also lists candidates whose parameters have not been published yet; those are left out rather than guessed, so this is the detections whose masses are known, not every detection. Every event drawn clears the catalogs' own confident threshold (probability of astrophysical origin above 0.5), and a few sit only just above it. Each mass is the median of a probability distribution, not a measurement: the cross through every dot is the 90% credible interval, and on the faintest signals it is wider than the dot is far from its neighbours. Masses are source-frame (the redshift is divided out). Dot size is the network signal-to-noise ratio — how loudly the signal arrived, which depends as much on distance and on which detectors were running as on the collision itself. Distance is luminosity distance in megaparsecs. The catalog is detection-limited by construction: loud, nearby, heavy mergers are easy to hear and quiet ones are not, so this is what the instruments could reach, not what the universe contains.