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19942022
most citedAdvanced Virgo: a 2nd generation interferometric gravitational wave detector

4.2k citations · 20.9k across the 175 of their papers we have counts for

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gr-qc2022★ 18 cited

Virgo Detector Characterization and Data Quality: tools

F. Acernese, M. Agathos, A. Ain +491

Detector characterization and data quality studies -- collectively referred to as {\em DetChar} activities in this article -- are paramount to the scientific exploitation of the jo…

gr-qc2022★ 60 cited

Virgo Detector Characterization and Data Quality: results from the O3 run

F. Acernese, M. Agathos, A. Ain +491

The Advanced Virgo detector has contributed with its data to the rapid growth of the number of detected gravitational-wave (GW) signals in the past few years, alongside the two Adv…

gr-qc2022★ 22 cited

The Virgo O3 run and the impact of the environment

F. Acernese, M. Agathos, A. Ain +486

Sources of geophysical noise (such as wind, sea waves and earthquakes) or of anthropogenic noise impact ground-based gravitational-wave interferometric detectors, causing transient…

gr-qc2021

The Next Generation Global Gravitational Wave Observatory: The Science Book

Vicky Kalogera, B. S. Sathyaprakash, Matthew Bailes +88

The next generation of ground-based gravitational-wave detectors will observe coalescences of black holes and neutron stars throughout the cosmos, thousands of them with exceptiona…

gr-qc2021

An Exploration of Possible Governance Models for the Future Global Gravitational-Wave Observatory Network

Stavros Katsanevas, Gary Sanders, Beverly Berger +17

The construction of a global network of detectors is the cornerstone to scientific success for 3rd generation gravitational wave astronomy. If carried out with a vision to the futu…

gr-qc2021

Future Ground-Based Gravitational-Wave Observatories: Synergies with Other Scientific Communities

Michele Punturo, David Reitze, Peter Couvares +10

Planning for the development of a 3rd generation global gravitational-wave detector array is a multifaceted and complex effort that will necessarily need a high level of community…

gr-qc2021

Gravitational Wave Data Analysis: Computing Challenges in the 3G Era

Peter Couvares, Ian Bird, Ed Porter +13

Cyber infrastructure will be a critical consideration in the development of next generation gravitational-wave detectors. The demand for data analysis computing in the 3G era will…

gr-qc2021

Expanding the Reach of Gravitational Wave Astronomy to the Edge of the Universe: The Gravitational-Wave International Committee Study Reports on Next Generation Ground-based Gravitational-Wave Observatories

David Reitze, Michele Punturo, Peter Couvares +10

The first direct detection of gravitational waves emitted from a pair of merging black holes in 2015 has been heralded as one of most significant scientific breakthroughs in physic…

gr-qc2018★ 58 cited

Calibration of Advanced Virgo and Reconstruction of the Gravitational Wave Signal h(t) during the Observing Run O2

Virgo Collaboration, F. Acernese, T. Adams +281

In August 2017, Advanced Virgo joined Advanced LIGO for the end of the O2 run, leading to the first gravitational waves detections with the three-detector network. This paper descr…

gr-qc2017★ 86 cited

Construction of KAGRA: an Underground Gravitational Wave Observatory

T. Akutsu, M. Ando, S. Araki +222

Major construction and initial-phase operation of a second-generation gravitational-wave detector KAGRA has been completed. The entire 3-km detector is installed underground in a m…

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…

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…

gr-qc2011★ 12 cited

Scientific Potential of Einstein Telescope

B. Sathyaprakash, M. Abernathy, F. Acernese +138

Einstein gravitational-wave Telescope (ET) is a design study funded by the European Commission to explore the technological challenges of and scientific benefits from building a th…

gr-qc2010★ 1.1k cited

Sensitivity Studies for Third-Generation Gravitational Wave Observatories

S. Hild, M. Abernathy, F. Acernese +136

Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a…

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★ 33 cited

Characterization of the seismic environment at the Sanford Underground Laboratory, South Dakota

Jan Harms, Fausto Acernese, Fabrizio Barone +18

An array of seismometers is being developed at the Sanford Underground Laboratory, the former Homestake mine, in South Dakota to study the properties of underground seismic fields…

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★ 24 cited

Gravitational wave burst search in the Virgo C7 data

The Virgo Collaboration, F. Acernese

A search for gravitational wave burst events has been performed with the Virgo C7 commissioning run data that have been acquired in September 2005 over five days. It focused on un-…