activity
20092019
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations · 11k across the 15 of their papers we have counts for

collaborators
Showing gr-qcShow all

11 papers · 1 filter

gr-qc2019★ 84 cited

Narrow-band search for gravitational waves from known pulsars using the second LIGO observing run

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1135

Isolated spinning neutron stars, asymmetric with respect to their rotation axis, are expected to be sources of continuous gravitational waves. The most sensitive searches for these…

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…

gr-qc2014★ 55 cited

A directed search for gravitational waves from Scorpius X-1 with initial LIGO

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +891

We present results of a search for continuously-emitted gravitational radiation, directed at the brightest low-mass X-ray binary, Scorpius X-1. Our semi-coherent analysis covers 10…

gr-qc2014★ 123 cited

Improved Upper Limits on the Stochastic Gravitational-Wave Background from 2009-2010 LIGO and Virgo Data

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +846

Gravitational waves from a variety of sources are predicted to superpose to create a stochastic background. This background is expected to contain unique information from throughou…

gr-qc2014★ 69 cited

First all-sky search for continuous gravitational waves from unknown sources in binary systems

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +849

We present the first results of an all-sky search for continuous gravitational waves from unknown spinning neutron stars in binary systems using LIGO and Virgo data. Using a specia…

gr-qc2012★ 120 cited

Search for Gravitational Waves from Binary Black Hole Inspiral, Merger and Ringdown in LIGO-Virgo Data from 2009-2010

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +800

We report a search for gravitational waves from the inspiral, merger and ringdown of binary black holes (BBH) with total mass between 25 and 100 solar masses, in data taken at the…

gr-qc2012★ 110 cited

Einstein@Home all-sky search for periodic gravitational waves in LIGO S5 data

J. Aasi, J. Abadie, B. P. Abbott +794

This paper presents results of an all-sky searches for periodic gravitational waves in the frequency range [50, 1190] Hz and with frequency derivative ranges of [-2 x 10^-9, 1.1 x…

gr-qc2010★ 143 cited

Calibration of the LIGO Gravitational Wave Detectors in the Fifth Science Run

LIGO Scientific Collaboration, J. Abadie, B. P. Abbott +538

The Laser Interferometer Gravitational Wave Observatory (LIGO) is a network of three detectors built to detect local perturbations in the space-time metric from astrophysical sourc…

gr-qc2009★ 48 cited

Search for gravitational wave ringdowns from perturbed black holes in LIGO S4 data

The LIGO Scientific Collaboration, B. Abbott

According to general relativity a perturbed black hole will settle to a stationary configuration by the emission of gravitational radiation. Such a perturbation will occur, for exa…

gr-qc2009★ 146 cited

Search for Gravitational Waves from Low Mass Binary Coalescences in the First Year of LIGO's S5 Data

LIGO Scientific Collaboration, B. Abbott

We have searched for gravitational waves from coalescing low mass compact binary systems with a total mass between 2 and 35 Msun and a minimum component mass of 1 Msun using data f…