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19992026
most citedAdvanced Virgo: a 2nd generation interferometric gravitational wave detector

4.2k citations · 45.2k across the 160 of their papers we have counts for

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16 papers · 1 filter

physics.ins-det2014★ 26 cited

Measurement of the atmospheric muon depth intensity relation with the NEMO Phase-2 tower

S. Aiello, F. Ameli, M. Anghinolfi +90

The results of the analysis of the data collected with the NEMO Phase-2 tower, deployed at 3500 m depth about 80 km off-shore Capo Passero (Italy), are presented. Cherenkov photons…

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★ 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…

astro-ph.IM2014★ 50 cited

Narrow-band search of continuous gravitational-wave signals from Crab and Vela pulsars in Virgo VSR4 data

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +894

In this paper we present the results of a coherent narrow-band search for continuous gravitational-wave signals from the Crab and Vela pulsars conducted on Virgo VSR4 data. In orde…

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-qc2014★ 4.2k cited

Advanced Virgo: a 2nd generation interferometric gravitational wave detector

F. Acernese, M. Agathos, K. Agatsuma +231

Advanced Virgo is the project to upgrade the Virgo interferometric detector of gravitational waves, with the aim of increasing the number of observable galaxies (and thus the detec…

astro-ph.HE2014★ 45 cited

Methods and results of a search for gravitational waves associated with gamma-ray bursts using the GEO600, LIGO, and Virgo detectors

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +889

In this paper we report on a search for short-duration gravitational wave bursts in the frequency range 64 Hz-1792 Hz associated with gamma-ray bursts (GRBs), using data from GEO60…

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…

astro-ph.IM2014★ 76 cited

Deep sea tests of a prototype of the KM3NeT digital optical module

S. Adrián-Martínez, M. Ageron, F. Aharonian +247

The first prototype of a photo-detection unit of the future KM3NeT neutrino telescope has been deployed in the deep waters of the Mediterranean Sea. This digital optical module has…

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…

astro-ph.HE2014★ 43 cited

Search for gravitational waves associated with gamma-ray bursts detected by the InterPlanetary Network

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +901

We present the results of a search for gravitational waves associated with 223 gamma-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth…

gr-qc2014★ 45 cited

Search for gravitational radiation from intermediate mass black hole binaries in data from the second LIGO-Virgo joint science run

The LIGO Scientific Collaboration, the Virgo Collaboration, J. Aasi +847

This paper reports on an unmodeled, all-sky search for gravitational waves from merging intermediate mass black hole binaries (IMBHB). The search was performed on data from the sec…

gr-qc2014★ 33 cited

Search for gravitational wave ringdowns from perturbed intermediate mass black holes in LIGO-Virgo data from 2005-2010

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

We report results from a search for gravitational waves produced by perturbed intermediate mass black holes (IMBH) in data collected by LIGO and Virgo between 2005 and 2010. The se…

gr-qc2014★ 61 cited

The NINJA-2 project: Detecting and characterizing gravitational waveforms modelled using numerical binary black hole simulations

The LIGO Scientific Collaboration, the Virgo Collaboration, 2 Collaboration +888

The Numerical INJection Analysis (NINJA) project is a collaborative effort between members of the numerical relativity and gravitational-wave astrophysics communities. The purpose…

gr-qc2014★ 31 cited

Towards weighing the condensation energy to ascertain the Archimedes force of vacuum

Enrico Calloni, Martina De Laurentis, Rosario De Rosa +7

The force exerted by the gravitational field on a Casimir cavity in terms of Archimedes force of vacuum is discussed, the force that can be tested against observation is identified…

gr-qc2014★ 11 cited

Reconstruction of the gravitational wave signal during the Virgo science runs and independent validation with a photon calibrator

Virgo collaboration, T. Accadia, F. Acernese +193

The Virgo detector is a kilometer-scale interferometer for gravitational wave detection located near Pisa (Italy). About 13 months of data were accumulated during four science runs…