535 citations · 653 across the 7 of their papers we have counts for
7 papers
Continuous Jets and Backflow Models for the Formation of W50/SS433 in Magnetohydrodynamics Simulations
Takumi Ohmura, Kojiro Ono, Haruka Sakemi +3
The formation mechanism of the W50/SS433 complex has long been a mystery. We propose a new scenario in which the SS433 jets themselves form the W50/SS433 system. We carry out magne…
KAGRA: 2.5 Generation Interferometric Gravitational Wave Detector
T. Akutsu, M. Ando, K. Arai +188
The recent detections of gravitational waves (GWs) reported by LIGO/Virgo collaborations have made significant impact on physics and astronomy. A global network of GW detectors wil…
Bias-free parameter estimation depending on sky region for targeted gravitational wave
Kenji Ono, Kazuhiro Hayama
Detection of gravitational waves(GW) involves using the network of GW telescopes to observe a large sky region. However, owing to the arrangement of the GW telescopes, even with aL…
Construction of KAGRA: an Underground Gravitational Wave Observatory
T. Akutsu, M. Ando, S. Araki +222
Major construction and initial-phase operation of a second-generation gravitational-wave detector KAGRA has been completed. The entire 3-km detector is installed underground in a m…
Determination of mass of an isolated neutron star using continuous gravitational waves with two frequency modes: an effect of a misalignment angle
Kazunari Eda, Kenji Ono, Yousuke Itoh
A rapidly spinning neutron star (NS) would emit a continuous gravitational wave (GW) detectable by the advanced LIGO, advanced Virgo, KAGRA and proposed third generation detectors…
A new estimation method for mass of an isolated neutron star using gravitational waves
Kenji Ono, Kazunari Eda, Yousuke Itoh
We investigate a possibility of estimating mass of an isolated rapidly rotating neutron star (NS) from a continuous gravitational wave (GW) signal emitted by the NS. When the GW pa…