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@ARTICLE{Abbott:395658,
      author       = {Abbott, B. P. and others},
      title        = {{M}ulti-messenger {O}bservations of a {B}inary {N}eutron
                      {S}tar {M}erger},
      journal      = {The astrophysical journal / 2},
      volume       = {848},
      number       = {2},
      issn         = {2041-8213},
      address      = {London},
      publisher    = {IOP Publ.},
      reportid     = {PUBDB-2017-12237, LIGO-P1700294. VIR-0802A-17.
                      arXiv:1710.05833},
      pages        = {L12},
      year         = {2017},
      note         = {This is a reproduction of the article published in the
                      Astrophysical Journal Letters, under the terms of the
                      Creative Commons Attribution 3.0 licence},
      abstract     = {On 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$1.7 s with
                      respect to the merger time. From the gravitational-wave
                      signal, the source was initially localized to a sky region
                      of 31 deg$^2$ 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 Msun. 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 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 $\sim$10 days. Following early non-detections, X-ray
                      and radio emission were discovered at the transient's
                      position $\sim$9 and $\sim$16 days, respectively, after the
                      merger. Both the X-ray and radio emission likely arise from
                      a physical process that is distinct from the one that
                      generates the UV/optical/near-infrared emission. No
                      ultra-high-energy gamma-rays and no neutrino candidates
                      consistent with the source were found in follow-up searches.
                      (Abridged)},
      cin          = {ZEU-EXP/AT},
      ddc          = {520},
      cid          = {$I:(DE-H253)ZEU-EXP_AT-20120731$},
      pnm          = {613 - Matter and Radiation from the Universe (POF3-613)},
      pid          = {G:(DE-HGF)POF3-613},
      experiment   = {EXP:(DE-H253)HESS-20170101 / EXP:(DE-H253)IceCube-20150101},
      typ          = {PUB:(DE-HGF)29 / PUB:(DE-HGF)16},
      eprint       = {1710.05833},
      howpublished = {arXiv:1710.05833},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1710.05833;\%\%$},
      UT           = {WOS:000413211000001},
      doi          = {10.3847/2041-8213/aa91c9},
      url          = {https://bib-pubdb1.desy.de/record/395658},
}