activity
20182026
most citedDirect constraints on ultra-light boson mass from searches for continuous gravitational waves

134 citations · 501 across the 18 of their papers we have counts for

collaborators

18 papers

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…

astro-ph.IM2026

Advanced Virgo Plus for O5 -- Design Report Overview

F. Acernese, A. Agapito, D. Agarwal +578

This document presents an overview of the design, implementation, and expected performance of the Advanced Virgo Plus (AdV+) upgrades in view of the O5 observing run. Following the…

astro-ph.IM2026

py5vec: a modular Python package for the 5-vector method to search for continuous gravitational waves

Luca D'Onofrio, Federico Muciaccia, Lorenzo Mirasola +7

We present \texttt{py5vec}, a Python package for implementing and extending the 5-vector method, used to search for continuous gravitational wave (CW) signals. We also provide a co…

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…

gr-qc2025★ 5 cited

A directed continuous-wave search from Scorpius X-1 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…

gr-qc2024★ 1 cited

Doppler correlation-driven vetoes for the Frequency Hough analysis in continuous gravitational-wave searches

Matteo Di Giovanni, Paola Leaci, Pia Astone +8

We present an improved method for vetoing candidates of continuous gravitational-wave sources during all-sky searches utilizing the Frequency Hough pipeline. This approach leverage…

astro-ph.IM2024

Neural network method to search for long transient gravitational waves

Francesca Attadio, Leonardo Ricca, Marco Serra +11

We present a new method to search for long transient gravitational waves signals, like those expected from fast spinning newborn magnetars, in interferometric detector data. Standa…

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★ 6 cited

Impact of signal clusters in wide-band searches for continuous gravitational waves

Lorenzo Pierini, Pia Astone, Cristiano Palomba +9

In this paper we present a study of some relevant steps of the hierarchical frequency-Hough (FH) pipeline, used within the LIGO and Virgo Collaborations for wide-parameter space se…

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…

astro-ph.HE2019★ 134 cited

Direct constraints on ultra-light boson mass from searches for continuous gravitational waves

Cristiano Palomba, Sabrina D'Antonio, Pia Astone +10

\textit{Superradiance} can trigger the formation of an ultra-light boson cloud around a spinning black hole. Once formed, the boson cloud is expected to emit a nearly periodic, lon…

astro-ph.IM2019★ 71 cited

How effective is machine learning to detect long transient gravitational waves from neutron stars in a real search?

Andrew L. Miller, Pia Astone, Sabrina D'Antonio +12

We present a comprehensive study of the effectiveness of Convolution Neural Networks (CNNs) to detect long duration transient gravitational-wave signals lasting fro…

astro-ph.IM2018★ 72 cited

A New Method to Observe Gravitational Waves emitted by Core Collapse Supernovae

P. Astone, P. Cerda-Duran, I. Di Palma +4

While gravitational waves have been detected from mergers of binary black holes and binary neutron stars, signals from core collapse supernovae, the most energetic explosions in th…

astro-ph.IM2018★ 47 cited

A method to search for long duration gravitational wave transients from isolated neutron stars using the generalized FrequencyHough

Andrew Miller, Pia Astone, Sabrina D'Antonio +10

We describe a method to detect gravitational waves lasting emitted by young, isolated neutron stars, such as those that could form after a supernova or a binary neu…

gr-qc2018★ 54 cited

A semi-coherent analysis method to search for continuous gravitational waves emitted by ultra-light boson clouds around spinning black holes

S. D'Antonio, C. Palomba, S. Frasca +8

As a consequence of superradiant instability induced in Kerr black holes, ultra-light boson clouds can be a source of persistent gravitational waves, potentially detectable by curr…

gr-qc2018★ 4 cited

Phase decomposition of the template metric for continuous gravitational-wave searches

S. Mastrogiovanni, P. Astone, S. D Antonio +9

A type of gravitational-wave signals in the LIGO-Virgo sensitivity band are expected to be emitted by spinning asymmetric neutron stars, with rotational frequencies that could plau…