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19992014
most citedCharacterization of the LIGO detectors during their sixth science run

1.3k citations · 7.8k across the 53 of their papers we have counts for

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gr-qc2014★ 1.3k cited

Characterization of the LIGO detectors during their sixth science run

The LIGO Scientific Collaboration, The Virgo Collaboration, J. Aasi +867

In 2009-2010, the Laser Interferometer Gravitational-wave Observa- tory (LIGO) operated together with international partners Virgo and GEO600 as a network to search for gravitation…

gr-qc2014★ 58 cited

Searching for stochastic gravitational waves using data from the two co-located LIGO Hanford detectors

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +873

Searches for a stochastic gravitational-wave background (SGWB) using terrestrial detectors typically involve cross-correlating data from pairs of detectors. The sensitivity of such…

gr-qc2013★ 29 cited

Application of a Hough search for continuous gravitational waves on data from the 5th LIGO science run

The LIGO Scientific Collaboration, The Virgo Collaboration, J. Aasi +876

We report on an all-sky search for periodic gravitational waves in the frequency range with the first derivative of frequency in the range $-8.9 \times 10^{-1…

gr-qc2013★ 85 cited

Constraints on cosmic strings from the LIGO-Virgo gravitational-wave detectors

J. Aasi, J. Abadie, B. P. Abbott +873

Cosmic strings can give rise to a large variety of interesting astrophysical phenomena. Among them, powerful bursts of gravitational waves (GWs) produced by cusps are a promising o…

gr-qc2013★ 160 cited

Parameter estimation for compact binary coalescence signals with the first generation gravitational-wave detector network

the LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +801

Compact binary systems with neutron stars or black holes are one of the most promising sources for ground-based gravitational wave detectors. Gravitational radiation encodes rich i…

gr-qc2012★ 16 cited

Outlook for detection of GW inspirals by GRB-triggered searches in the Advanced detector era

Alexander Dietz, Nickolas Fotopoulos, Leo Singer +1

Short, hard gamma-ray bursts (GRBs) are believed to originate from the coalescence of two neutron stars (NSs) or a NS and a black hole (BH). If this scenario is correct, then short…

gr-qc2012★ 181 cited

Searching for gravitational waves from binary coalescence

S. Babak, R. Biswas, P. R. Brady +25

We describe the implementation of a search for gravitational waves from compact binary coalescences in LIGO and Virgo data. This all-sky, all-time, multi-detector search for binary…

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-qc2012★ 548 cited

Scientific Objectives of Einstein Telescope

B. Sathyaprakash, M. Abernathy, F. Acernese +222

The advanced interferometer network will herald a new era in observational astronomy. There is a very strong science case to go beyond the advanced detector network and build detec…

gr-qc2012★ 6 cited

Prospects for early localization of gravitational-wave signals from compact binary coalescences with advanced detectors

Alessandro Manzotti, Alexander Dietz

A leading candidate source of detectable gravitational waves is the inspiral and merger of pairs of stellar-mass compact objects. The advanced LIGO and advanced Virgo detectors wil…

gr-qc2012★ 92 cited

The characterization of Virgo data and its impact on gravitational-wave searches

J. Aasi, J. Abadie, B. P. Abbott +798

Between 2007 and 2010 Virgo collected data in coincidence with the LIGO and GEO gravitational-wave (GW) detectors. These data have been searched for GWs emitted by cataclysmic phen…

gr-qc2012★ 20 cited

Likelihood-ratio ranking of gravitational-wave candidates in a non-Gaussian background

Rahul Biswas, Patrick R. Brady, Jordi Burguet-Castell +9

We describe a general approach to detection of transient gravitational-wave signals in the presence of non-Gaussian background noise. We prove that under quite general conditions,…

gr-qc2012★ 13 cited

Detecting transient gravitational waves in non-Gaussian noise with partially redundant analysis methods

Rahul Biswas, Patrick R. Brady, Jordi Burguet-Castell +9

There is a broad class of astrophysical sources that produce detectable, transient, gravitational waves. Some searches for transient gravitational waves are tailored to known featu…

gr-qc2011★ 225 cited

Search for Gravitational Waves from Low Mass Compact Binary Coalescence in LIGO's Sixth Science Run and Virgo's Science Runs 2 and 3

the LIGO Scientific Collaboration, the Virgo Collaboration, J. Abadie +796

We report on a search for gravitational waves from coalescing compact binaries using LIGO and Virgo observations between July 7, 2009 and October 20, 2010. We searched for signals…

gr-qc2011★ 80 cited

All-sky Search for Periodic Gravitational Waves in the Full S5 LIGO Data

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

We report on an all-sky search for periodic gravitational waves in the frequency band 50-800 Hz and with the frequency time derivative in the range of 0 through -6e-9 Hz/s. Such a…

gr-qc2011

Characterization of the Virgo Seismic Environment

The Virgo Collaboration, T. Accadia, F. Acernese +180

The Virgo gravitational wave detector is an interferometer (ITF) with 3km arms located in Pisa, Italy. From July to October 2010, Virgo performed its third science run (VSR3) in co…

gr-qc2011

Search for gravitational waves from binary black hole inspiral, merger and ringdown

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Abadie +721

We present the first modeled search for gravitational waves using the complete binary black hole gravitational waveform from inspiral through the merger and ringdown for binaries w…

gr-qc2010★ 99 cited

Calibration and sensitivity of the Virgo detector during its second science run

The Virgo Collaboration, T. Accadia, F. Acernese +175

The Virgo detector is a kilometer-length interferometer for gravitational wave detection located near Pisa (Italy). During its second science run (VSR2) in 2009, six months of data…

gr-qc2010

Searches for inspiral gravitational waves associated with short gamma-ray bursts in LIGO's fifth and Virgo's first science run

Alexander Dietz

Mergers of two compact objects, like two neutron stars or a neutron star and a black hole, are the probable progenitor of short gamma-ray bursts. These events are also promising so…

gr-qc2010

Searches for inspiral gravitational waves associated with short gamma-ray bursts in LIGO's fifth and Virgo's first science run

Alexander Dietz

This brief report describes the search for gravitational-wave inspiral signals from short gamma-ray bursts. Since these events are probably created by the merger of two compact obj…

gr-qc2010★ 9 cited

Virgo calibration and reconstruction of the gravitational wave strain during VSR1

The Virgo collaboration, T. Accadia, F. Acernese +171

Virgo is a kilometer-length interferometer for gravitational waves detection located near Pisa. Its first science run, VSR1, occured from May to October 2007. The aims of the calib…

gr-qc2008★ 30 cited

First joint search for gravitational-wave bursts in LIGO and GEO600 data

LIGO Scientific Collaboration, B. Abbott

We present the results of the first joint search for gravitational-wave bursts by the LIGO and GEO600 detectors. We search for bursts with characteristic central frequencies in the…

gr-qc2008★ 4 cited

GRB-triggered searches for gravitational waves in LIGO data

Alexander Dietz

The LIGO gravitational wave detectors have recently reached their design sensitivity and finished a two-year science run. During this period one year of data with unprecedented sen…

gr-qc2007★ 1.2k cited

LIGO: The Laser Interferometer Gravitational-Wave Observatory

The LIGO Scientific Collaboration, B. Abbott

The goal of the Laser Interferometric Gravitational-Wave Observatory (LIGO) is to detect and study gravitational waves of astrophysical origin. Direct detection of gravitational wa…