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20142020
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations · 22.3k across the 18 of their papers we have counts for

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Showing 2017Show all

5 papers · 1 filter

astro-ph.HE2017★ 1.3k cited

GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1101

On June 8, 2017 at 02:01:16.49 UTC, a gravitational-wave signal from the merger of two stellar-mass black holes was observed by the two Advanced LIGO detectors with a network signa…

astro-ph.HE2017★ 3.6k cited

Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

LIGO Scientific Collaboration, Virgo Collaboration, Fermi Gamma-Ray Burst Monitor +1

On 2017 August 17, the gravitational-wave event GW170817 was observed by the Advanced LIGO and Virgo detectors, and the gamma-ray burst (GRB) GRB 170817A was observed independently…

astro-ph.HE2017★ 266 cited

Search for post-merger gravitational waves from the remnant of the binary neutron star merger GW170817

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1105

The first observation of a binary neutron star coalescence by the Advanced LIGO and Advanced Virgo gravitational-wave detectors offers an unprecedented opportunity to study matter…

gr-qc2017★ 9.8k cited

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

The LIGO Scientific Collaboration, The Virgo Collaboration

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, GW1…

gr-qc2017★ 63 cited

First narrow-band search for continuous gravitational waves from known pulsars in advanced detector data

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1096

Spinning neutron stars asymmetric with respect to their rotation axis are potential sources of continuous gravitational waves for ground-based interferometric detectors. In the cas…