activity
20242026
most citedParameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang transform

5 citations · 8 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.IM2026

Wavelet-Based Extraction of Transient Noise in Gravitational-Wave Interferometers using a Saliency-Guided Learning Architecture

Christopher Allene, Dhruv Kumar, Yusuke Sakai +2

Gravitational-wave interferometers exhibit a wide variety of short-duration non-Gaussian transients, commonly referred to as glitches, that complicate the detection of astrophysica…

gr-qc2025

Glitch noise classification in KAGRA O3GK observing data using unsupervised machine learning

Shoichi Oshino, Yusuke Sakai, Marco Meyer-Conde +5

Gravitational wave interferometers are disrupted by various types of nonstationary noise, referred to as glitch noise, that affect data analysis and interferometer sensitivity. The…

gr-qc2025

Regression of Suspension Violin Modes in KAGRA O3GK Data with Kalman Filters

Lucas Moisset, Marco Meyer-Conde, Christopher Allene +4

Suspension thermal modes in interferometric gravitational-wave detectors produce narrow, high-Q spectral lines that can contaminate gravitational searches and bias parameter estima…

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…

astro-ph.IM2025

Computing the Wave: Where the Gravitational Wave Community benefits from High-Energy Physics, and where it differs ?

Marco Meyer-Conde, Nobuyuki Kanda, Hirotaka Takahashi +2

High-Energy Physics (HEP) and Gravitational Wave (GW) communities serve different scientific purposes. However, their methodologies might potentially offer mutual enrichment throug…

hep-ph2025

Probing Pion Valence Quark Distribution with Beam-charge Asymmetry of Pion-induced Production

Wen-Chen Chang, Marco Meyer-Conde, Jen-Chieh Peng +2

We consider the beam-charge asymmetry of the production cross sections in - versus -induced reactions on proton or nuclear targets. We show that the productio…

astro-ph.HE2025★ 1 cited

Gravitational Wave Memory from Accelerating Relativistic Jets in Multiple Thick Shell Scenarios

Yusuke Sakai, Ryo Yamazaki, Yoshihiro Okutani +4

Gravitational wave (GW) memory, a permanent distortion of the space-time metric, is anticipated during the acceleration of relativistic jets in gamma-ray bursts (GRBs). While the p…

gr-qc2024★ 5 cited

Parameter estimation of protoneutron stars from gravitational wave signals using the Hilbert-Huang transform

Seiya Sasaoka, Yusuke Sakai, Diego Dominguez +5

Core-collapse supernovae (CCSNe) are potential multimessenger events detectable by current and future gravitational wave (GW) detectors. The GW signals emitted during these events…