82 citations · 224 across the 7 of their papers we have counts for
7 papers
On Statistical Independence and No-Correlation for a Pair of Random Variables Taking Two Values: Classical and Quantum
Toru Ohira
It is well known that when a pair of random variables is statistically independent, it has no-correlation (zero covariance, ), and that the converse is not tr…
Results of the search for inspiraling compact star binaries from TAMA300's observation in 2000-2004
TAMA Collaboration, T. Akutsu
We analyze the data of TAMA300 detector to search for gravitational waves from inspiraling compact star binaries with masses of the component stars in the range 1-3Msolar. In this…
Observation results by the TAMA300 detector on gravitational wave bursts from stellar-core collapses
Masaki Ando, Koji Arai, Youichi Aso +19
We present data-analysis schemes and results of observations with the TAMA300 gravitational-wave detector, targeting burst signals from stellar-core collapse events. In analyses fo…
Coincidence analysis to search for inspiraling compact binaries using TAMA300 and LISM data
Hirotaka Takahashi, Hideyuki Tagoshi
Japanese laser interferometric gravitational wave detectors, TAMA300 and LISM, performed a coincident observation during 2001. We perform a coincidence analysis to search for inspi…
The First Search for Gravitational Waves from Inspiraling Compact Binaries using TAMA300 data
Hideyuki Tagoshi, Nobuyuki Kanda, Takahiro Tanaka +2
We analyzed 6 hours of data from the TAMA300 detector by matched filtering, searching for gravitational waves from inspiraling compact binaries. We incorporated a two-step hierarch…
Detection of Dark Matter Concentrations in the Field of Cl 1604+4304 from Weak Lensing Analysis
Keiichi Umetsu, Toshifumi Futamase
We present a weak-lensing analysis of a region around the galaxy cluster Cl 1604+4304 (z=0.897) on the basis of the deep observations with the HST/WFPC2. We apply a variant of Schn…
Post-Newtonian Approximation
Hideki Asada, Toshifumi Futamase
We discuss various aspects of the post-Newtonian approximation in general relativity. After presenting the foundation based on the Newtonian limit, we use the (3+1) formalism to fo…