activity
20182026
most citedA standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart

239 citations · 678 across the 12 of their papers we have counts for

collaborators

12 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…

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…

physics.ins-det2024★ 9 cited

Development of ion-beam sputtered silicon nitride thin films for low-noise mirror coatings of gravitational-wave detectors

A. Amato, M. Bazzan, G. Cagnoli +32

Brownian thermal noise of thin-film coatings is a fundamental limit for high-precision experiments based on optical resonators such as gravitational-wave interferometers. Here we p…

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…

physics.ins-det2020★ 52 cited

Progress in the measurement and reduction of thermal noise in optical coatings for gravitational-wave detectors

Massimo Granata, Alex Amato, Gianpietro Cagnoli +8

Coating thermal noise is a fundamental limit for precision experiments based on optical and quantum transducers. In this review, after a brief overview of the techniques for coatin…

physics.ins-det2019★ 116 cited

Amorphous optical coatings of present gravitational-wave interferometers

Massimo Granata, Alex Amato, Laurent Balzarini +10

We report on the results of an extensive campaign of optical and mechanical characterization of the ion-beam sputtered oxide layers (TaO, TiO, TaO-TiO, SiO$…

astro-ph.CO2018★ 239 cited

A standard siren measurement of the Hubble constant from GW170817 without the electromagnetic counterpart

M. Fishbach, R. Gray, I. Magaña Hernandez +316

We perform a statistical standard siren analysis of GW170817. Our analysis does not utilize knowledge of NGC 4993 as the unique host galaxy of the optical counterpart to GW170817.…

gr-qc2018★ 58 cited

Calibration of Advanced Virgo and Reconstruction of the Gravitational Wave Signal h(t) during the Observing Run O2

Virgo Collaboration, F. Acernese, T. Adams +281

In August 2017, Advanced Virgo joined Advanced LIGO for the end of the O2 run, leading to the first gravitational waves detections with the three-detector network. This paper descr…