activity
20162026
most citedKAGRA: 2.5 Generation Interferometric Gravitational Wave Detector

535 citations · 2.2k across the 67 of their papers we have counts for

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Showing 2025Show all

11 papers · 1 filter

gr-qc2025

Efficient Reconstruction of Matched-Filter Signal-to-Noise Ratio Time Series from Nearby Templates for Compact Binary Coalescences Searches

Yasuhiro Murakami, Tathagata Ghosh, Soichiro Morisaki

We present a method for efficiently searching long-duration gravitational wave signals from compact binary coalescences (CBCs). The approach exploits the smooth frequency-domain be…

gr-qc2025

Jiggled interferometer: Ground-based gravitational wave detector using rapidly-repeated free-falling test masses

Shoki Iwaguchi, Bin Wu, Kurumi Umemura +10

We propose the Jiggled Interferometer (JIGI), a novel ground-based gravitational wave detector employing low-frequency noise mitigation similar to that of space-based detectors. Us…

astro-ph.HE2025★ 2 cited

GW231109_235456: A Sub-threshold Binary Neutron Star Merger in the LIGO-Virgo-KAGRA O4a Observing Run?

Wanting Niu, Carl-Johan Haster, Jolien D. E. Creighton +25

We present a sub-threshold search for gravitational-wave inspirals from binary neutron stars using data from the first part of the fourth LIGO--Virgo--KAGRA observing run. To enhan…

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★ 3 cited

Analyzing black-hole ringdowns with orthonormal modes

Soichiro Morisaki, Hayato Motohashi, Motoki Suzuki +1

The ringdown signal following a black hole (BH) merger can be modeled as a superposition of BH quasinormal modes (QNMs), offering a clean setup for testing gravitational theories.…

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-qc2025

New Methods for Offline GstLAL Analyses

Prathamesh Joshi, Leo Tsukada, Chad Hanna +38

In this work, we present new methods implemented in the GstLAL offline gravitational wave search. These include a technique to reuse the matched filtering data products from a GstL…

gr-qc2025

How Many Times Should We Matched Filter Gravitational Wave Data? A Comparison of GstLAL's Online and Offline Performance

Prathamesh Joshi, Wanting Niu, Chad Hanna +34

Searches for gravitational waves from compact binary coalescences employ a process called matched filtering, in which gravitational wave strain data is cross-correlated against a b…

hep-ph2025

Enhancing the sensitivity to ultralight bosonic dark matter using signal correlations

Soichiro Morisaki, Jun'ya Kume, Takumi Fujimori +1

In recent years, numerous experiments have been proposed and conducted to search for ultralight bosonic dark matter (ULBDM). Signals from ULBDM in such experiments are characterize…

astro-ph.IM2025

Parameter estimation of gravitational-wave signals with frequency-dependent antenna responses and higher modes

Pratyusava Baral, Soichiro Morisaki, Ish Gupta +1

We implement frequency-dependent antenna responses and develop likelihood classes (standard likelihood, multibanded likelihood, and the relative binning (RB) likelihood) capable of…

hep-ph2025

Searches for ultralight vector and axion dark matter with KAGRA

Yuta Michimura, Takumi Fujimori, Hiroki Fujimoto +10

We have proposed using laser interferometric gravitational wave detectors to search for ultralight vector and axion dark matter. Vector dark matter can be probed through oscillatin…