activity
19962026
most citedPossibility of Direct Measurement of the Acceleration of the Universe Using 0.1 Hz Band Laser Interferometer Gravitational Wave Antenna in Space

955 citations · 3.9k across the 84 of their papers we have counts for

collaborators
Showing 2005 · astro-phShow all

6 papers · 2 filters

astro-ph2005★ 10 cited

Prospects of LIGO for constraining inclination of merging compact binaries associated with three-dimensionally localized short-hard GRBs

Naoki Seto

We study prospects of a method to constrain the inclination of a coalescing compact binary by detecting its gravitational waves associated with a three-dimensionally localized (dir…

astro-ph2005★ 34 cited

Did WMAP see Moving Local Structures?

Asantha Cooray, Naoki Seto

The divergence of the momentum density field of the large scale structure generates a secondary anisotropy contribution to the Cosmic Microwave Background (CMB). While the effect i…

astro-ph2005★ 10 cited

Gravitational Wave Astrometry for Rapidly Rotating Neutron Stars and Estimation of Their Distances

Naoki Seto

We discuss an astrometric timing effect on data analysis of continuous gravitational waves from rapidly rotating isolated neutron stars. Special attention is directed to the possib…

astro-ph2005★ 6 cited

Can LISA Resolve Distance to the Large Magellanic Cloud?

Asantha Cooray, Naoki Seto

The Laser Interferometer Space Antenna (LISA) is expected to detect N ~ 22 [x10^(+/- 1)] close white dwarf binaries in the Large Magellanic Cloud (LMC) through their gravitational…

astro-ph2005★ 9 cited

Cosmological Constraints on the Very Low Frequency Gravitational-Wave Background

Naoki Seto, Asantha Cooray

While there are no strong observational constraints on the gravitational wave background across six or more orders of magnitude between 10^{-16} Hz and 10^{-10} Hz and it is diffic…

astro-ph2005★ 18 cited

Probing the largest scale structure in the universe with polarization map of galaxy clusters

Naoki Seto, Elena Pierpaoli

We introduce a new formalism to describe the polarization signal of galaxy clusters on the whole sky. We show that a sparsely sampled, half-sky map of the cluster polarization sign…