most citedGW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors

2 citations · 2 across the 4 of their papers we have counts for

collaborators

8 papers

gr-qc2026

GWTC-5.0: Tests of General Relativity

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1822

The signals from the LIGO-Virgo-KAGRA network of gravitational-wave (GW) detectors allow us to perform sensitive tests of general relativity (GR) in the dynamical and strong-field…

astro-ph.IM2026

GFH-v2 Pipeline for Searches of Long-Transient Gravitational Waves from Newborn Magnetars

Sandhya Sajith Menon, Lorenzo Pierini, Pia Astone +11

This paper presents an enhanced methodology for searching long transient gravitational waves associated with a newborn magnetar, with particular focus on the regime in which the ea…

gr-qc2026

Impact of coalescence signals on the search for continuous gravitational waves with Einstein Telescope

Elena Codazzo, Lorenzo Mirasola, Matteo Di Giovanni +7

The current network of gravitational wave detectors has already revealed hundreds of compact binary coalescences (CBCs), including binary neutron stars, binary black holes, and bla…

gr-qc20262 cited

GW240925 and GW250207: Astrophysical Calibration of Gravitational-wave Detectors

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1878

GW240925 and GW250207 are two loud gravitational-wave signals from binary black hole coalescences observed with network signal-to-noise ratios and , respectively…

gr-qc2025

Search for continuous gravitational wave signals from luminous dark photon superradiance clouds with LVK O3 observations

Lorenzo Mirasola, Cristina Mondino, Francesco Amicucci +10

Superradiance clouds of kinetically-mixed dark photons around spinning black holes can produce observable multi-messenger electromagnetic and gravitational wave signals. The cloud…

gr-qc2025

A directed continuous-wave search from neutron stars in binary systems with the five-vector resampling technique

Francesco Amicucci, Paola Leaci, Pia Astone +8

Continuous gravitational-wave signals (CWs), which are typically emitted by rapidly rotating neutron stars with non-axisymmetric deformations, represent particularly intriguing tar…