activity
20192025
most citedAGN Disks Harden the Mass Distribution of Stellar-mass Binary Black Hole Mergers

166 citations · 662 across the 11 of their papers we have counts for

collaborators

11 papers

gr-qc2025

Identification of Noise-Associated Glitches in KAGRA O3GK with Hveto

T. Akutsu, M. Ando, M. Aoumi +148

Transient noise ("glitches") in gravitational wave detectors can mimic or obscure true signals, significantly reducing detection sensitivity. Identifying and excluding glitch-conta…

gr-qc2023★ 21 cited

Gravitational wave source populations: Disentangling an AGN component

V. Gayathri, Daniel Wysocki, Y. Yang +4

The astrophysical origin of the over 90 compact binary mergers discovered by the LIGO and Virgo gravitational wave observatories is an open question. While the unusual mass and spi…

physics.acc-ph2022★ 3 cited

A Work Proposal for a Collaborative Study of Magnet Technology for a Future Muon Collider

L. Bottura, D. Aguglia, B. Auchmann +30

In this paper we elaborate on the nature and challenges for the magnet systems of a muon collider as presently considered within the scope of the International Muon Collider Collab…

astro-ph.HE2021★ 27 cited

Micro Tidal Disruption Events in Active Galactic Nuclei

Y. Yang, I. Bartos, G. Fragione +5

Active galactic nuclei (AGNs) can act as black hole assembly lines, funneling some of the stellar-mass black holes from the vicinity of the galactic center into the inner plane of…

gr-qc2021★ 60 cited

Black hole mergers of AGN origin in LIGO/Virgo's O1-O3a observing periods

V. Gayathri, Y. Yang, H. Tagawa +2

The origin of the black hole mergers detected by LIGO and Virgo remains an open question. While the unusual mass and spin of a few events constrain their possible astrophysical for…

gr-qc2020★ 71 cited

All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems

The LIGO Scientific Collaboration, the Virgo Collaboration, R. Abbott +1369

Rapidly spinning neutron stars are promising sources of persistent, continuous gravitational waves. Detecting such a signal would allow probing of the physical properties of matter…