activity
20142018
most citedAdvanced Virgo: a 2nd generation interferometric gravitational wave detector

4.2k citations · 5.9k across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2018★ 239 cited

A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart

M. Fishbach, R. Gray, I. Magaña Hernandez +316

We perform a statistical standard siren analysis of GW170817. Our analysis does not utilize knowledge of NGC 4993 as the unique host galaxy of the optical counterpart to GW170817.…

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-qc2018★ 98 cited

Empirical tests of the black hole no-hair conjecture using gravitational-wave observations

Gregorio Carullo, Laura van der Schaaf, Lionel London +10

We show that second-generation gravitational-wave detectors at their design sensitivity will allow us to directly probe the ringdown phase of binary black hole coalescences. This o…

gr-qc2017★ 80 cited

Parameterized tests of the strong-field dynamics of general relativity using gravitational wave signals from coalescing binary black holes: Fast likelihood calculations and sensitivity of the method

Jeroen Meidam, Ka Wa Tsang, Janna Goldstein +15

Thanks to the recent discoveries of gravitational wave signals from binary black hole mergers by Advanced Laser Interferometer Gravitational Wave Observatory and Advanced Virgo, th…

gr-qc2016★ 76 cited

Effective-one-body waveforms for binary neutron stars using surrogate models

Benjamin D. Lackey, Sebastiano Bernuzzi, Chad R. Galley +2

Gravitational-wave observations of binary neutron star systems can provide information about the masses, spins, and structure of neutron stars. However, this requires accurate and…

astro-ph.HE2016★ 21 cited

Search for transient gravitational waves in coincidence with short duration radio transients during 2007-2013

The LIGO Scientific Collaboration, the Virgo Collaboration, others +999

We present an archival search for transient gravitational-wave bursts in coincidence with 27 single pulse triggers from Green Bank Telescope pulsar surveys, using the LIGO, Virgo a…

gr-qc2016★ 754 cited

GW150914: The Advanced LIGO Detectors in the Era of First Discoveries

The LIGO Scientific Collaboration, The Virgo Collaboration

Following a major upgrade, the two advanced detectors of the Laser Interferometer Gravitational-wave Observatory (LIGO) held their first observation run between September 2015 and…

gr-qc2015★ 232 cited

Constraining the neutron star equation of state with gravitational wave signals from coalescing binary neutron stars

Michalis Agathos, Jeroen Meidam, Walter Del Pozzo +5

Recently exploratory studies were performed on the possibility of constraining the neutron star equation of state (EOS) using signals from coalescing binary neutron stars, or neutr…

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★ 148 cited

Testing the no-hair theorem with black hole ringdowns using TIGER

J. Meidam, M. Agathos, C. Van Den Broeck +2

The Einstein Telescope (ET), a proposed third-generation gravitational wave observatory, would enable tests of the no-hair theorem by looking at the characteristic frequencies and…

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…