GW170814

E732408

GW170814 is a gravitational-wave signal detected in 2017 from the merger of two stellar-mass black holes, notable for being observed jointly by the LIGO and Virgo detectors.

All labels observed (1)

Label Occurrences
GW170814 canonical 1

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf astrophysical transient
binary black hole merger
gravitational-wave event
announcedOn 2017-09-27
belongsToObservingRun LIGO-Virgo O2 NERFINISHED
detectedBy LIGO NERFINISHED
Virgo NERFINISHED
detectedByInstrument Advanced LIGO NERFINISHED
Advanced Virgo NERFINISHED
hasCatalogInclusion GWTC-1 gravitational-wave transient catalog NERFINISHED
hasChirpMass ~24 solar masses
hasComponentSpinConstraint low effective spin
hasCosmologyAssumption standard Lambda-CDM cosmology
hasDataRelease strain time series publicly available
hasDeclinationUncertainty tens of square degrees
hasDetectionDate 2017-08-14
hasDetectionMethod gravitational-wave interferometry
hasDetectorSite LIGO Hanford Observatory NERFINISHED
LIGO Livingston Observatory NERFINISHED
Virgo detector at Cascina, Italy NERFINISHED
hasElectromagneticCounterpartDetected no
hasEventNameConvention date-based YYMMDD format
hasFalseAlarmRate less than 1 in 27,000 years
hasFinalBlackHoleMass 53.2 solar masses
hasFinalBlackHoleSpin dimensionless spin ~0.7
hasHostGalaxyIdentified no
hasLuminosityDistance 1.8 billion light-years
540 million parsecs
hasMassRatio ~1.2
hasNetworkSignificance >5 sigma
hasPolarizationMeasurement constrains tensor polarizations
hasPrimaryBlackHoleMass 30.5 solar masses
hasRadiatedEnergy about 3 solar masses c^2
hasRedshift 0.12
hasRightAscensionUncertainty tens of square degrees
hasSecondaryBlackHoleMass 25.3 solar masses
hasSignalToNoiseRatio ~15.9
hasSkyLocalizationArea about 60 square degrees
hasSkyLocalizationImprovementFactor about 10
hasSourceFrameTotalMass ~56 solar masses
hasSourceType stellar-mass black hole binary
hasWaveformType inspiral-merger-ringdown
isConsistentWithGeneralRelativity yes
isFirstOfType first LIGO-Virgo joint detection of a binary black hole merger
first binary black hole merger observed by three detectors
reportedInCollaborationPaper LIGO Scientific Collaboration and Virgo Collaboration NERFINISHED
testsGeneralRelativity yes

How these facts were elicited

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.