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dc.contributor.authorAbbott, B. P.
dc.contributor.authorDíaz García, Antonio Francisco 
dc.contributor.authorNavas Concha, Sergio 
dc.contributor.authorBueno Villar, Antonio 
dc.contributor.authorSánchez Lucas, Patricia
dc.date.accessioned2020-06-18T11:19:23Z
dc.date.available2020-06-18T11:19:23Z
dc.date.issued2017-10-20
dc.identifier.citationAbbott, B. P., Abbott, R., Abbott, T. D., Acernese, F., Ackley, K., Adams, C., ... & Affeldt, C. (2017). Multi-messenger Observations of a Binary Neutron Star Merger. The Astrophysical Journal, 848(2).. [https://doi.org/10.3847/2041-8213/aa91c9]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/62544
dc.descriptionLIGO Scientific Collaboration and Virgo Collaboration, Fermi GBM, INTEGRAL, IceCube Collaboration, AstroSat Cadmium Zinc Telluride Imager Team, IPN Collaboration, The Insight-HXMT Collaboration, ANTARES Collaboration, The Swift Collaboration, AGILE Team, The 1M2H Team, The Dark Energy Camera GW-EM Collaboration and the DES Collaboration, The DLT40 Collaboration, GRAWITA: GRAvitational Wave Inaf TeAm, The Fermi Large Area Telescope Collaboration, ATCA: Australia Telescope Compact Array, ASKAP: Australian SKA Pathfinder, Las Cumbres Observatory Group, OzGrav, DWF (Deeper, Wider, Faster Program), AST3, and CAASTRO Collaborations, The VINROUGE Collaboration, MASTER Collaboration, J-GEM, GROWTH, JAGWAR, CaltechNRAO, TTU-NRAO, and NuSTAR Collaborations, Pan-STARRS, The MAXI Team, TZAC Consortium, KU Collaboration, Nordic Optical Telescope, ePESSTO, GROND, Texas Tech University, SALT Group, TOROS: Transient Robotic Observatory of the South Collaboration, The BOOTES Collaboration, MWA: Murchison Widefield Array, The CALET Collaboration, IKI-GW Follow-up Collaboration, H.E.S.S. Collaboration, LOFAR Collaboration, LWA: Long Wavelength Array, HAWC Collaboration, The Pierre Auger Collaboration, ALMA Collaboration, Euro VLBI Team, Pi of the Sky Collaboration, The Chandra Team at McGill University, DFN: Desert Fireball Network, ATLAS, High Time Resolution Universe Survey, RIMAS and RATIR, and SKA South Africa/MeerKATes_ES
dc.description.abstractOn 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of $\sim 1.7\,{\rm{s}}$ with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of ${40}_{-8}^{+8}$ Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 $\,{M}_{\odot }$. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at $\sim 40\,{\rm{Mpc}}$) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient's position $\sim 9$ and $\sim 16$ days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta.es_ES
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dc.description.sponsorshipGerman INTEGRAL through DLR 50 OG 1101es_ES
dc.description.sponsorshipSpanish MINECO/FEDER ESP2015-65712-C5-1-Res_ES
dc.description.sponsorshipRussian Foundation for Basic Research (RFBR) 16-29-13009-ofi-mes_ES
dc.description.sponsorshipMinistry of Education, Culture, Sports, Science and Technology, Japan (MEXT) Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research (KAKENHI) JP16H02183 JP15H02075 JP15H02069 JP26800103 JP25800103es_ES
dc.description.sponsorshipInter-University Cooperation Program of the MEXTes_ES
dc.description.sponsorshipNINS programes_ES
dc.description.sponsorshipToyota Foundation D11-R-0830es_ES
dc.description.sponsorshipMitsubishi Foundationes_ES
dc.description.sponsorshipYamada Science Foundationes_ES
dc.description.sponsorshipInoue Foundation for Sciencees_ES
dc.description.sponsorshipNational Research Foundation - South Africaes_ES
dc.description.sponsorshipNRF 2017R1A3A3001362es_ES
dc.description.sponsorshipKASI 2017-1-830-03es_ES
dc.description.sponsorshipIsrael Science Foundation 541/17es_ES
dc.description.sponsorshipCouncil of Scientific & Industrial Research (CSIR) - Indiaes_ES
dc.description.sponsorshipDepartment of Science & Technology (India)es_ES
dc.description.sponsorshipScience AMP; Engineering Research Board (SERB), Indiaes_ES
dc.description.sponsorshipMinistry of Higher Education & Scientific Research (MHESR)es_ES
dc.description.sponsorshipSpanish Agencia Estatal de Investigaciones_ES
dc.description.sponsorshipVicepresidencia i Conselleria d'Innovacio Recerca i Turismees_ES
dc.description.sponsorshipConselleria d'Educacio i Universitat del Govern de les Illes Balearses_ES
dc.description.sponsorshipConselleria d'Educacio Investigacio Cultura i Esport de la Generalitat Valencianaes_ES
dc.description.sponsorshipNational Science Centre of Polandes_ES
dc.description.sponsorshipSwiss National Science Foundation (SNSF)es_ES
dc.description.sponsorshipRussian Foundation for Basic Research (RFBR)es_ES
dc.description.sponsorshipRussian Science Foundation (RSF)es_ES
dc.description.sponsorshipEuropean Commission Joint Research Centrees_ES
dc.description.sponsorshipEuropean Union (EU)es_ES
dc.description.sponsorshipRoyal Society of Londones_ES
dc.description.sponsorshipScottish Funding Counciles_ES
dc.description.sponsorshipScottish Universities Physics Alliancees_ES
dc.description.sponsorshipOrszagos Tudomanyos Kutatasi Alapprogramok (OTKA)es_ES
dc.description.sponsorshipLyon Institute of Origins (LIO)es_ES
dc.description.sponsorshipNational Research, Development and Innovation Office Hungary (NKFI)es_ES
dc.description.sponsorshipNational Research Foundation of Koreaes_ES
dc.description.sponsorshipIndustry Canada and Province of Ontario through Ministry of Economic Development and Innovationes_ES
dc.description.sponsorshipNatural Sciences and Engineering Research Council of Canadaes_ES
dc.description.sponsorshipCanadian Institute for Advanced Research (CIFAR)es_ES
dc.description.sponsorshipBrazilian Ministry of Science, Technology, Innovations, and Communicationses_ES
dc.description.sponsorshipInternational Center for Theoretical Physics South American Institute for Fundamental Research (ICTP-SAIFR)es_ES
dc.description.sponsorshipHong Kong Research Grants Counciles_ES
dc.description.sponsorshipNational Natural Science Foundation of Chinaes_ES
dc.description.sponsorshipChinese Academy of Scienceses_ES
dc.description.sponsorshipMinistry of Science and Technology, Chinaes_ES
dc.description.sponsorshipLeverhulme Trustes_ES
dc.description.sponsorshipResearch Corporation for Science Advancementes_ES
dc.description.sponsorshipMinistry of Science and Technology, Taiwanes_ES
dc.description.sponsorshipRIKENes_ES
dc.description.sponsorshipMinistry of Education, Culture, Sports, Science and Technology, Japan (MEXT) Japan Society for the Promotion of Science Grants-in-Aid for Scientific Research (KAKENHI) JP 17H06362es_ES
dc.description.sponsorshipEVN RP029es_ES
dc.description.sponsorshipEuropean Union's Horizon 2020 research and innovation programme 653477es_ES
dc.description.sponsorshipEuropean Research Council (ERC) 647208es_ES
dc.description.sponsorshipNetherlands Organization for Scientific Research through NWO VIDI 639.042.612-Nissankees_ES
dc.description.sponsorshipNetherlands Organization for Scientific Research (NWO) 62002444-Nissankees_ES
dc.description.sponsorshipVISIR 60.A-9392es_ES
dc.description.sponsorshipMOST104-2923-M-008-004-MY5es_ES
dc.description.sponsorshipMOST106-2112-M-008-007es_ES
dc.language.isoenges_ES
dc.publisherIOP Publishing; American Astronomical Societyes_ES
dc.relationEC/FP7/PEOPLE-2012-IEF-328826es_ES
dc.relationEC/H2020/646623es_ES
dc.relationEU/FP7/PIRSES-2009-GA-246806es_ES
dc.relationEU/H2020/653477es_ES
dc.relationERC/647208es_ES
dc.rightsAtribución 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.subjectGravitational waveses_ES
dc.subjectStars: neutrones_ES
dc.titleMulti-messenger Observations of a Binary Neutron Star Mergeres_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.identifier.doi10.3847/2041-8213/aa91c9


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Atribución 3.0 España
Except where otherwise noted, this item's license is described as Atribución 3.0 España