activity
20132025
most citedAll-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run

98 citations · 253 across the 9 of their papers we have counts for

collaborators

9 papers

gr-qc2025★ 2 cited

Decadal upgrade strategy for KAGRA toward post-O5 gravitational-wave astronomy

KAGRA Collaboration, T. Akutsu, M. Ando +150

The KAGRA Collaboration has investigated a ten-year upgrade strategy for the KAGRA gravitational wave detector, considering a total of 14 upgrade options that vary in mirror mass,…

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…

physics.ins-det2022★ 7 cited

Improving the stability of frequency dependent squeezing with bichromatic control of filter cavity length, alignment and incident beam pointing

Yuhang Zhao, Eleonora Capocasa, Marc Eisenmann +21

Frequency dependent squeezing is the main upgrade for achieving broadband quantum noise reduction in upcoming observation runs of gravitational wave detectors. The proper frequency…

physics.optics2020★ 50 cited

Gravitational wave detectors with broadband high frequency sensitivity

Michael A. Page, Maxim Goryachev, Haixing Miao +10

The binary neutron star coalescence GW170817 was observed by gravitational wave detectors during the inspiral phase but sensitivity in the 1-5 kHz band was insufficient to observe…

gr-qc2019★ 98 cited

All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run

The LIGO Scientific Collaboration, the Virgo Collaboration, B. P. Abbott +1186

We present the results of a search for short-duration gravitational-wave transients in the data from the second observing run of Advanced LIGO and Advanced Virgo. We search for gra…

astro-ph.IM2017★ 14 cited

Enhanced detection of high frequency gravitational waves using optically diluted optomechanical filters

Michael Page, Jiayi Qin, James La Fontaine +2

Detections of gravitational waves (GW) in the frequency band 35 Hz to 500 Hz have led to the birth of GW astronomy. Expected signals above 500 Hz, such as the quasinormal modes of…

physics.ins-det2016★ 29 cited

The next detectors for gravitational wave astronomy

David Blair, Li Ju, Chunnong Zhao +15

This paper focuses on the next detectors for gravitational wave astronomy which will be required after the current ground based detectors have completed their initial observations,…

physics.optics2016★ 10 cited

Towards thermal noise free optomechanics

Michael Page, Yiqiu Ma, Chunnong Zhao +6

Thermal noise generally greatly exceeds quantum noise in optomechanical devices unless the mechanical frequency is very high or the thermodynamic temperature is very low. This pape…

astro-ph.IM2013★ 43 cited

The Hot and Energetic Universe: The X-ray Integral Field Unit (X-IFU) for Athena+

D. Barret, J. W. den Herder, L. Piro +55

The Athena+ mission concept is designed to implement the Hot and Energetic Universe science theme submitted to the European Space Agency in response to the call for White Papers fo…