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20102025
most citedFirst higher-multipole model of gravitational waves from spinning and coalescing black-hole binaries

253 citations · 2k across the 30 of their papers we have counts for

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29 papers · 1 filter

gr-qc2025★ 2 cited

Testing general relativity with amplitudes of subdominant gravitational-wave modes

Ish Gupta, Purnima Narayan, Lionel London +2

We present an improved subdominant-mode amplitude (SMA) test of general relativity (GR), which probes amplitude-level deviations in the higher-order modes of gravitational-wave (GW…

gr-qc2025

PhenomXPNR: An improved gravitational wave model linking precessing inspirals and NR-calibrated merger-ringdown

Eleanor Hamilton, Marta Colleoni, Jonathan E. Thompson +10

We present the frequency-domain quasi-circular precessing binary-black-hole model PhenomXPNR. This model combines the most precise available post-Newtonian description of the evolu…

gr-qc2025★ 3 cited

Black hole spectroscopy: from theory to experiment

Emanuele Berti, Vitor Cardoso, Gregorio Carullo +65

The "ringdown" radiation emitted by oscillating black holes has great scientific potential. By carefully predicting the frequencies and amplitudes of black hole quasinormal modes a…

gr-qc2023★ 81 cited

PhenomXO4a: a phenomenological gravitational-wave model for precessing black-hole binaries with higher multipoles and asymmetries

Jonathan E. Thompson, Eleanor Hamilton, Lionel London +4

In this work we introduce PhenomXO4a, the first phenomenological, frequency-domain gravitational waveform model to incorporate multipole asymmetries and precession angles tuned to…

gr-qc2023★ 8 cited

A catalogue of precessing black-hole-binary numerical-relativity simulations

Eleanor Hamilton, Edward Fauchon-Jones, Mark Hannam +9

We present a public catalogue of numerical-relativity binary-black-hole simulations. The catalogue contains datasets from 80 distinct configurations of precessing binary-black-hole…

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★ 7 cited

Virgo Detector Characterization and Data Quality during 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 signals in the past few years, alongside the two LIGO ins…

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★ 87 cited

The final twist: A model of gravitational waves from precessing black-hole binaries through merger and ringdown

Eleanor Hamilton, Lionel London, Jonathan E. Thompson +6

We present PhenomPNR, a frequency-domain phenomenological model of the gravitational-wave (GW) signal from binary-black-hole mergers that is tuned to numerical relativity (NR) simu…

gr-qc2019★ 105 cited

On the properties of the massive binary black hole merger GW170729

Katerina Chatziioannou, Roberto Cotesta, Sudarshan Ghonge +53

We present a detailed investigation into the properties of GW170729, the gravitational wave with the most massive and distant source confirmed to date. We employ an extensive set o…

gr-qc2018★ 39 cited

On modeling for Kerr black holes: Basis learning, QNM frequencies, and spherical-spheroidal mixing coefficients

L. London, E. Fauchon-Jones

Models of black hole properties play an important role in the ongoing direct detection of gravitational waves from black hole binaries. One important aspect of model based gravitat…

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-qc2018★ 61 cited

Modeling ringdown II: non-precessing binary black holes

L. London

The aftermath of binary black hole coalescence is a perturbed remnant whose gravitational radiation rings down, encoding information about the new black hole's recent history and c…

gr-qc2017★ 253 cited

First higher-multipole model of gravitational waves from spinning and coalescing black-hole binaries

Lionel London, Sebastian Khan, Edward Fauchon-Jones +7

Gravitational-wave observations of binary black holes currently rely on theoretical models that predict the dominant multipoles (l,m) of the radiation during inspiral, merger and r…

gr-qc2017★ 134 cited

Testing general relativity using gravitational wave signals from the inspiral, merger and ringdown of binary black holes

Abhirup Ghosh, Nathan K. Johnson-McDaniel, Archisman Ghosh +6

Advanced LIGO's recent observations of gravitational waves (GWs) from merging binary black holes have opened up a unique laboratory to test general relativity (GR) in the highly re…

gr-qc2016★ 42 cited

The most powerful astrophysical events: Gravitational-wave peak luminosity of binary black holes as predicted by numerical relativity

David Keitel, Xisco Jiménez Forteza, Sascha Husa +9

For a brief moment, a binary black hole (BBH) merger can be the most powerful astrophysical event in the visible universe. Here we present a model fit for this gravitational-wave p…

gr-qc2016★ 25 cited

Search for continuous gravitational waves from neutron stars in globular cluster NGC 6544

B. P. Abbott, R. Abbott, T. D. Abbott +953

We describe a directed search for continuous gravitational waves in data from the sixth LIGO science run. The target was the nearby globular cluster NGC 6544 at a distance of 2.7 k…

gr-qc2016★ 35 cited

Results of the deepest all-sky survey for continuous gravitational waves on LIGO S6 data running on the Einstein@Home volunteer distributed computing project

The LIGO Scientific Collaboration, The Virgo Collaboration

We report results of a deep all-sky search for periodic gravitational waves from isolated neutron stars in data from the S6 LIGO science run. The search was possible thanks to the…

gr-qc2016★ 202 cited

Georgia Tech Catalog of Gravitational Waveforms

Karan Jani, James Healy, James A. Clark +3

This paper introduces a catalog of gravitational waveforms from the bank of simulations by the numerical relativity effort at Georgia Tech. Currently, the catalog consists of 452 d…

gr-qc2016★ 150 cited

Testing general relativity using golden black-hole binaries

Abhirup Ghosh, Archisman Ghosh, Nathan K. Johnson-McDaniel +8

The coalescences of stellar-mass black-hole binaries through their inspiral, merger, and ringdown are among the most promising sources for ground-based gravitational-wave (GW) dete…

gr-qc2015★ 2 cited

Connecting Numerical Relativity and Data Analysis of Gravitational Wave Detectors

Deirdre Shoemaker, Karan Jani, Lionel London +1

Gravitational waves deliver information in exquisite detail about astrophysical phenomena, among them the collision of two black holes, a system completely invisible to the eyes of…

gr-qc2014★ 2 cited

Investigating Binary Black Hole Mergers with Principal Component Analysis

James Clark, Laura Cadonati, James Healy +6

Despite recent progress in numerical simulations of the coalescence of binary black hole systems, highly asymmetric spinning systems and the construction of accurate physical templ…

gr-qc2014★ 219 cited

Modeling Ringdown: Beyond the Fundamental Quasi-Normal Modes

Lionel London, James Healy, Deirdre Shoemaker

While black hole perturbation theory predicts a rich quasi-normal mode structure, technical challenges have limited the numerical study of excitations to the fundamental, lowest or…