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LIGO Scientific Collaboration

United States

105 papers here33.8k citations across 105
fields
  • gr-qc61
  • astro-ph.HE17
  • astro-ph.IM12
  • astro-ph6
  • physics.ins-det4
  • astro-ph.CO1
  • astro-ph.GA1
  • cs.LG1
ROR 0518wrr32OpenAlex

affiliations via OpenAlex

output
20032026
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations

researchers with a paper here
  • I. W. Harry66
  • P. Schmidt59
  • R. L. Savage58
  • D. J. Ottaway57
  • A. M. Sintes56
  • B. J. J. Slagmolen56
  • D. H. Shoemaker56
  • B. Willke55
  • D. E. McClelland55
  • D. Sigg55
  • J. T. Whelan55
  • A. L. Stuver54
collaborating institutions
  • California Institute of TechnologyUS84 papers
  • Massachusetts Institute of TechnologyUS77 papers
  • University of FloridaUS76 papers
  • Louisiana State UniversityUS71 papers
  • Syracuse UniversityUS71 papers
  • Max Planck Institute for Gravitational PhysicsDE70 papers
  • Australian National UniversityAU69 papers
  • Leibniz University HannoverDE68 papers
  • Stanford UniversityUS68 papers
  • The University of AdelaideAU67 papers
  • The University of Western AustraliaAU67 papers
  • University of GlasgowGB67 papers
Showing astro-ph.GAShow all

1 paper · 1 filter

astro-ph.GA2025★ 1 cited

Black Hole - Neutron Star and Binary Neutron Star Mergers from Population III and II stars

Benedetta Mestichelli, Michela Mapelli, Filippo Santoliquido +9

Population III (Pop. III) stars are expected to be massive and to undergo minimal mass loss due to their lack of metals, making them ideal progenitors of black holes and neutron…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.