activity
20012022
most citedCharacterization of the LIGO detectors during their sixth science run

1.3k citations · 7k across the 62 of their papers we have counts for

collaborators

64 papers

gr-qc2022

Input optics systems of the KAGRA detector during O3GK

T. Akutsu, M. Ando, K. Arai +246

KAGRA, the underground and cryogenic gravitational-wave detector, was operated for its solo observation from February 25th to March 10th, 2020, and its first joint observation with…

astro-ph.IM2022★ 30 cited

Performance of the KAGRA detector during the first joint observation with GEO 600 (O3GK)

KAGRA Collaboration, H. Abe, R. X. Adhikari +212

KAGRA, the kilometer-scale underground gravitational-wave detector, is located at Kamioka, Japan. In April 2020, an astrophysics observation was performed at the KAGRA detector in…

gr-qc2021★ 5 cited

Gravitational Wave Physics and Astronomy in the nascent era

Makoto Arimoto, Hideki Asada, Michael L. Cherry +50

The detections of gravitational waves (GW) by LIGO/Virgo collaborations provide various possibilities to physics and astronomy. We are quite sure that GW observations will develop…

gr-qc2020★ 9 cited

Overview of KAGRA : KAGRA science

KAGRA Collaboration, T. Akutsu, M. Ando +240

KAGRA is a newly build gravitational-wave observatory, a laser interferometer with 3 km arm length, located in Kamioka, Gifu, Japan. In this paper in the series of KAGRA-featured a…

astro-ph.HE2020★ 4 cited

Estimate of the Detectability of the Circular Polarisation Signature of Supernova Gravitational Waves Using the Stokes Parameters

Man Leong Chan, Kazuhiro Hayama

The circular polarisation of gravitational waves from core collapse supernovae has been proposed as a probe to investigate the rotation and physical features inside the core of the…

gr-qc2020★ 23 cited

Prospects for improving the sensitivity of the cryogenic gravitational wave detector KAGRA

Yuta Michimura, Kentaro Komori, Yutaro Enomoto +18

Upgrades to improve the sensitivity of gravitational wave detectors enable more frequent detections and more precise source parameter estimation. Unlike other advanced interferomet…