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20012026
most citedObservation of the rare decay from the combined analysis of CMS and LHCb data

508 citations · 8.5k across the 167 of their papers we have counts for

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Showing 2022Show all

10 papers · 1 filter

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★ 26 cited

ETpathfinder: a cryogenic testbed for interferometric gravitational-wave detectors

A. Utina, A. Amato, J. Arends +112

The third-generation of gravitational wave observatories, such as the Einstein Telescope (ET) and Cosmic Explorer (CE), aim for an improvement in sensitivity of at least a factor o…

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…