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20172026
most citedGW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole with a 2.6 M Compact Object

1.8k citations · 6k across the 16 of their papers we have counts for

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gr-qc2026

Advanced Virgo during the LIGO-Virgo-KAGRA fourth observing run

Virgo Collaboration, F Acernese, A Agapito +546

From April 10, 2024 to November 18, 2025 Advanced Virgo participated in the fourth observing run of the network of gravitational-wave detectors, together with Advanced LIGO and KAG…

gr-qc2025★ 10 cited

Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession

Soumen Roy, Maria Haney, Geraint Pratten +2

When testing general relativity (GR) with gravitational wave observations, parametrized tests of deviations from the expected strong-field source dynamics are one of the most widel…

gr-qc2025★ 97 cited

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

gr-qc2024★ 8 cited

Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object

Elise M. Sänger, Soumen Roy, Michalis Agathos +16

On May 29, 2023, the LIGO Livingston observatory detected the gravitational-wave signal GW230529_181500 from the merger of a neutron star with a lower mass-gap compact object. Its…

gr-qc2024★ 1 cited

Detectability of eccentric binary black holes with PyCBC and cWB pipelines during the third observing run of LIGO-Virgo-KAGRA

Bhooshan Gadre, Kanchan Soni, Shubhanshu Tiwari +3

Detecting binary black hole (BBH) mergers with quantifiable orbital eccentricity would confirm the existence of a dynamical formation channel for these binaries. The current state-…

gr-qc2023★ 16 cited

New gravitational waveform model for precessing binary neutron stars with double-spin effects

Marta Colleoni, Felip A. Ramis Vidal, Nathan K. Johnson-McDaniel +3

We present two new frequency-domain gravitational waveform models for the analysis of signals emitted by binary neutron star coalescences: IMRPhenomXAS_NRTidalv2 and IMRPhenomXP_NR…