{"work":{"id":"a19136e8-99c2-49be-b029-60af2e20c6ee","openalex_id":null,"doi":"10.1103/physrevlett.119.161106","arxiv_id":"1710.05832","raw_key":null,"title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","authors":null,"authors_text":"The LIGO Scientific Collaboration, The Virgo Collaboration","year":2017,"venue":"gr-qc","abstract":"On August 17, 2017 at 12:41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per $8.0\\times10^4$ years. We infer the component masses of the binary to be between 0.86 and 2.26 $M_\\odot$, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17 to 1.60 $M_\\odot$, with the total mass of the system $2.74^{+0.04}_{-0.01}\\,M_\\odot$. The source was localized within a sky region of 28 deg$^2$ (90% probability) and had a luminosity distance of $40^{+8}_{-14}$ Mpc, the closest and most precisely localized gravitational-wave signal yet. The association with the gamma-ray burst GRB 170817A, detected by Fermi-GBM 1.7 s after the coalescence, corroborates the hypothesis of a neutron star merger and provides the first direct evidence of a link between these mergers and short gamma-ray bursts. Subsequent identification of transient counterparts across the electromagnetic spectrum in the same location further supports the interpretation of this event as a neutron star merger. This unprecedented joint gravitational and electromagnetic observation provides insight into astrophysics, dense matter, gravitation and cosmology.","external_url":"https://arxiv.org/abs/1710.05832","cited_by_count":null,"metadata_source":"pith","metadata_fetched_at":"2026-07-10T15:07:19.424958+00:00","pith_arxiv_id":"1710.05832","created_at":"2026-05-09T06:19:13.991649+00:00","updated_at":"2026-07-11T11:50:26.030339+00:00","title_quality_ok":true,"display_title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","render_title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral"},"hub":{"state":{"work_id":"a19136e8-99c2-49be-b029-60af2e20c6ee","tier":"super_hub","tier_reason":"100+ Pith inbound or 10,000+ external citations","pith_inbound_count":158,"external_cited_by_count":null,"distinct_field_count":12,"first_pith_cited_at":"2013-10-06T02:23:37+00:00","last_pith_cited_at":"2026-07-08T21:42:21+00:00","author_build_status":"needed","summary_status":"needed","contexts_status":"needed","graph_status":"needed","ask_index_status":"needed","reader_status":"not_needed","recognition_status":"not_needed","updated_at":"2026-08-21T23:49:19.415402+00:00","tier_text":"super_hub"},"tier":"super_hub","role_counts":[{"context_role":"background","n":52},{"context_role":"dataset","n":1},{"context_role":"method","n":1}],"polarity_counts":[{"context_polarity":"background","n":48},{"context_polarity":"support","n":3},{"context_polarity":"unclear","n":1},{"context_polarity":"use_dataset","n":1},{"context_polarity":"use_method","n":1}],"runs":{"ask_index":{"job_type":"ask_index","status":"succeeded","result":{"title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","claims":[{"claim_text":"On August 17, 2017 at 12:41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per $8.0\\times10^4$ years. We infer the component masses of the binary to be between 0.86 and 2.26 $M_\\odot$, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17 to 1.60 $M_\\od","claim_type":"abstract","evidence_strength":"source_metadata"},{"claim_text":"Introduction- The direct detection of gravitational wave (GW) signals, with the first detection of a black- hole (BH) binary GW150914 by the LIGO-Virgo col- laboration in 2015 [1], has established GW astronomy as a new pathway for exploring the physics of our uni- verse in the strong-gravity regime. 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In addition to the gravitational- wave signal, GW170817 showed a prompt short-duration g","claim_type":"background","confidence":0.95,"evidence_strength":"citation_context"},{"claim_text":"primordial sound waves ringing in the early Universe, from an epoch prior to the formation of the CMB. Recently, the first detection of gravitational waves (GWs) [107,108] by the LIGO collab- oration [109-111] has opened an unprecedented window onto the Universe, and has inaugu- rated the era of multi-messenger astronomy thanks to the first coincident detection of GW and electromagnetic signal with the GW170817 and GRB170817A events [112-114]. 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The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per $8.0\\times10^4$ years. We infer the component masses of the binary to be between 0.86 and 2.26 $M_\\odot$, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17 to 1.60 $M_\\od","claim_type":"abstract","evidence_strength":"source_metadata"},{"claim_text":"Introduction- The direct detection of gravitational wave (GW) signals, with the first detection of a black- hole (BH) binary GW150914 by the LIGO-Virgo col- laboration in 2015 [1], has established GW astronomy as a new pathway for exploring the physics of our uni- verse in the strong-gravity regime. 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In addition to the gravitational- wave signal, GW170817 showed a prompt short-duration g","claim_type":"background","confidence":0.95,"evidence_strength":"citation_context"},{"claim_text":"primordial sound waves ringing in the early Universe, from an epoch prior to the formation of the CMB. Recently, the first detection of gravitational waves (GWs) [107,108] by the LIGO collab- oration [109-111] has opened an unprecedented window onto the Universe, and has inaugu- rated the era of multi-messenger astronomy thanks to the first coincident detection of GW and electromagnetic signal with the GW170817 and GRB170817A events [112-114]. 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