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20092025
most citedKAGRA: 2.5 Generation Interferometric Gravitational Wave Detector

535 citations · 1.3k across the 31 of their papers we have counts for

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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…

gr-qc2023★ 1 cited

Searching for gravitational wave echoes from black hole binary events in the third observing run of LIGO, Virgo, and KAGRA collaborations

Nami Uchikata, Tatsuya Narikawa, Hiroyuki Nakano +3

Gravitational wave echo signals have been proposed as evidence for the modification of the spacetime structure near the classical event horizon. These signals are expected to occur…

gr-qc2023★ 13 cited

Multipole tidal effects in the post-Newtonian gravitational-wave phase of compact binary coalescences

Tatsuya Narikawa

We present the multipole component form of the gravitational wave tidal phase for compact binary coalescences (MultipoleTidal), which consists of the mass quadrupole, the current q…

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…

gr-qc2022★ 9 cited

Follow-up analyses of the binary-neutron-star signals GW170817 and GW190425 by using post-Newtonian waveform models

Tatsuya Narikawa, Nami Uchikata

We reanalyze the binary-neutron-star signals, GW170817 and GW190425, focusing on the inspiral regime to avoid uncertainties on waveform modeling in the postinspiral regime. We use…