activity
20212024
most citedScience with the Einstein Telescope: a comparison of different designs

402 citations · 934 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.IM2024★ 60 cited

LIGO Detector Characterization in the first half of the fourth Observing run

S. Soni, B. K. Berger, D. Davis +232

Progress in gravitational-wave astronomy depends upon having sensitive detectors with good data quality. Since the end of the LIGO-Virgo-KAGRA third Observing run in March 2020, de…

gr-qc2023

Prospects for an isotropic gravitational wave background detection with Earth-based interferometric detectors and the threat of correlated noise

Kamiel Janssens

In this overview we discuss the prospects for a first detection of an isotropic gravitational wave background with earth-based interferometric detectors. Furthermore, we focus on h…

gr-qc2023★ 29 cited

pygwb: Python-based library for gravitational-wave background searches

Arianna I. Renzini, Alba Romero-Rodrguez, Colm Talbot +31

The collection of gravitational waves (GWs) that are either too weak or too numerous to be individually resolved is commonly referred to as the gravitational-wave background (GWB).…

gr-qc2023★ 402 cited

Science with the Einstein Telescope: a comparison of different designs

Marica Branchesi, Michele Maggiore, David Alonso +73

The Einstein Telescope (ET), the European project for a third-generation gravitational-wave detector, has a reference configuration based on a triangular shape consisting of three…

gr-qc2022★ 36 cited

Stochastic gravitational wave background: methods and Implications

Nick van Remortel, Kamiel Janssens, Kevin Turbang

Beyond individually resolvable gravitational wave events such as binary black hole and binary neutron star mergers, the superposition of many more weak signals coming from a multit…

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★ 23 cited

Correlated 1-1000 Hz magnetic field fluctuations from lightning over earth-scale distances and their impact on gravitational wave searches

Kamiel Janssens, Matthew Ball, Robert M. S. Schofield +9

We report Earth-scale distance magnetic correlations from lightning strokes in the frequency range 1-1000 Hz at several distances ranging from 1100 to 9000 km. Noise sources which…

astro-ph.IM2022

Impact of correlated seismic and correlated Newtonian noise on the Einstein Telescope

Kamiel Janssens, Guillaume Boileau, Nelson Christensen +2

Correlated noise could impact the search for the gravitational wave background at future Earth-based gravitational-wave detectors. Due to the small distance ( 400 m) between…

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★ 11 cited

Formalism for power spectral density estimation for non-identical and correlated noise using the null channel in Einstein Telescope

Kamiel Janssens, Guillaume Boileau, Marie-Anne Bizouard +3

Several proposed gravitational wave interferometers have a triangular configuration, such as the Einstein Telescope and the Laser Interferometer Space Antenna. For such a configura…

gr-qc2022

External environmental noise influences on Virgo during O3

Nicolas Arnaud, Rosario De Rosa, Francesco Di Renzo +8

Sources of geophysical noise, such as wind, sea waves and earthquakes, can have an impact on gravitational wave interferometers causing sensitivity worsening and gaps in data takin…

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…

gr-qc2021

Gravitational-Wave Geodesy: Defining False Alarm Probabilities with Respect to Correlated Noise

Kamiel Janssens, Thomas A. Callister, Nelson Christensen +4

Future searches for a gravitational-wave background using Earth-based gravitational-wave detectors might be impacted by correlated noise sources. A well known example are the Schum…

gr-qc2021★ 33 cited

Impact of Schumann resonances on the Einstein Telescope and projections for the magnetic coupling function

Kamiel Janssens, Katarina Martinovic, Nelson Christensen +2

Correlated magnetic noise in the form of Schumann resonances could introduce limitations to the gravitational-wave background searches of future Earth-based gravitational-wave dete…

astro-ph.IM2021★ 233 cited

LIGO Detector Characterization in the Second and Third Observing Runs

D. Davis, J. S. Areeda, B. K. Berger +284

The characterization of the Advanced LIGO detectors in the second and third observing runs has increased the sensitivity of the instruments, allowing for a higher number of detecta…