67 citations · 1.3k across the 70 of their papers we have counts for
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Search for Compact Binary Coalescences with Sub-solar Mass Components in Data from the Second Part of LIGO-Virgo-KAGRA's Fourth Observing Run
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1816
We report on a gravitational wave search for compact binary coalescences with secondary mass between 0.2 M and 1 M and primary mass between 0.2 M and 10 M, restricting the componen…
Updated Upper Limits on the Isotropic Gravitational-Wave Background from LIGO, Virgo, and KAGRA Data through April 2025
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1805
We report results from a search for an isotropic stochastic gravitational-wave background using data collected by the LIGO--Virgo--KAGRA Collaboration. The analysis uses data from…
Constraints on ultralight bosons from merging binary and remnant black holes observed during the second and third parts of the fourth LIGO-Virgo-KAGRA observing run
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1808
We present constraints on ultralight bosons using binary black hole mergers observed in the second and third parts of the fourth LIGO-Virgo-KAGRA observing run. Directed searches a…
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…
Open Data from LIGO, Virgo, and KAGRA through the Second Part of the Fourth Observing Run
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1809
LIGO, Virgo, KAGRA, and GEO 600 form a network of gravitational-wave observatories. Data and analysis results from this network are made publicly available through the Gravitationa…
Numerical-relativity simulations of long-lived remnants of binary neutron star mergers
Roberto De Pietri, Alessandra Feo, José A. Font +3
We analyze the properties of the gravitational wave signal emitted after the merger of a binary neutron star system when the remnant survives for more than a 80 ms (and up to 140ms…
Convective Excitation of Inertial Modes in Binary Neutron Star Mergers
Roberto De Pietri, Alessandra Feo, José A. Font +4
We present the first very long-term simulations (extending up to ~140 ms after merger) of binary neutron star mergers with piecewise polytropic equations of state and in full gener…
Spectral analysis of gravitational waves from binary neutron star merger remnants
Francesco Maione, Roberto De Pietri, Alessandra Feo +1
In this work we analyze the gravitational wave signal from hypermassive neutron stars formed after the merger of binary neutron star systems, focusing on its spectral features. The…
Modeling Mergers of Known Galactic Systems of Binary Neutron Stars
Alessandra Feo, Roberto De Pietri, Francesco Maione +1
We present a study of the merger of six different known galactic systems of binary neutron stars (BNS) of unequal mass with a mass ratio between and . Specifically, th…
Binary neutron star merger simulations with different initial orbital frequency and equation of state
Francesco Maione, Roberto De Pietri, Alessandra Feo +1
We present results from three-dimensional general relativistic simulations of binary neutron star coalescences and mergers using public codes. We considered equal mass models where…
Modeling Equal and Unequal Mass Binary Neutron Star Mergers Using Public Codes
Roberto De Pietri, Alessandra Feo, Francesco Maione +1
We present three-dimensional simulations of the dynamics of binary neutron star (BNS) mergers from the late stage of the inspiral process up to ms after the system has me…
Stiffness effects on the dynamics of the bar-mode instability of Neutron Stars in full General Relativity
Frank Löffler, Roberto De Pietri, Alessandra Feo +2
We present results on the effect of the stiffness of the equation of state on the dynamical bar-mode instability in rapidly rotating polytropic models of neutron stars in full Gene…
Neutron Star instabilities in full General Relativity using a ideal fluid
Roberto De Pietri, Alessandra Feo, Luca Franci +1
We present results about the effect of the use of a stiffer equation of state, namely the ideal-fluid ones, on the dynamical bar-mode instability in rapidly rotating polyt…