activity
20032023
most citedOn measuring the gravitational-wave background using Pulsar Timing Arrays

192 citations · 948 across the 32 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

9 papers · 1 filter

astro-ph.CO2022★ 1 cited

Constraining the Hubble constant and its lower limit from the proper motion of extragalactic radio jets

Tiger Yu-Yang Hsiao, Tomotsugu Goto, Tetsuya Hashimoto +11

The Hubble constant () is a measurement to describe the expansion rate of the Universe in the current era. However, there is a discrepancy between the measurements fr…

astro-ph.CO2021★ 27 cited

Revealing the cosmic reionisation history with fast radio bursts in the era of Square Kilometre Array

Tetsuya Hashimoto, Tomotsugu Goto, Ting-Yi Lu +7

Revealing the cosmic reionisation history is at the frontier of extragalactic astronomy. The power spectrum of the cosmic microwave background (CMB) polarisation can be used to con…

astro-ph.CO2020★ 7 cited

Subaru medium-resolution spectra of a QSO at z=6.62: Three reionization tests

Ting-Yi Lu, Tomotsugu Goto, Ji-Jia Tang +9

Investigating the Gunn-Peterson trough of high redshift quasars (QSOs) is a powerful way to reveal the cosmic reionization. As one of such attempts, we perform a series of analyses…

astro-ph.CO2011★ 37 cited

CFHT Legacy Ultraviolet Extension (CLUE): Witnessing Galaxy Transformations up to 7 Mpc from Rich Cluster Cores

Ting Lu, David Gilbank, Sean McGee +2

Using the optical data from the Wide component of the CFHT Legacy Survey, and new ultraviolet data from GALEX, we study the colours and specific star formation rates (SSFR) of ~100…

astro-ph.CO2010★ 2 cited

The stellar and hot gas content of low-mass galaxy clusters

Michael L. Balogh, Pasquale Mazzotta, Richard G. Bower +4

We analyse the stellar and hot gas content of 18 nearby, low-mass galaxy clusters, detected in redshift space and selected to have a dynamical mass 3E14<M/Msun<6E14, as measured fr…

astro-ph.CO2009★ 23 cited

Large-scale Structure and Dynamics of the Most X-ray Luminous Galaxy Cluster Known -- RX J1347-1145

Ting Lu, David G. Gilbank, Michael L. Balogh +6

We present photometric, spectroscopic and weak lensing analysis of the large-scale structure and dynamics of the most X-ray luminous galaxy cluster known, RX J1347-1145, at z=0.451…