activity
20092026
most citedMeasurement and correction of variations in interstellar dispersion in high-precision pulsar timing

224 citations · 766 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.CO2026

Constraints on Ultralight Scalar and Dark Photon Dark Matter from PPTA-DR3 and EPTA-DR2

Xiao-Song Hu, Siyuan Chen, Kuo Liu +18

The cold dark matter model successfully describes the Universe on large scales, yet faces challenges at sub-galactic scales. Ultralight dark matter (ULDM), with particle masses aro…

astro-ph.GA2025★ 1 cited

Mapping the Spatial Distribution of Fast Radio Bursts within their Host Galaxies

Alexa C. Gordon, Wen-fai Fong, Adam T. Deller +23

We present deep optical and near-infrared observations of the host galaxies of 34 fast radio bursts (FRBs) detected by the Commensal Real-time ASKAP Fast Transient (CRAFT) survey o…

astro-ph.HE2024★ 4 cited

Pulsar Polarization Array Limits on Ultralight Axion-like Dark Matter

Xiao Xue, Shi Dai, Hoang Nhan Luu +20

We conduct the first-ever Pulsar Polarization Array (PPA) analysis to detect the ultralight Axion-Like Dark Matter (ALDM) using the polarization data of 22 millisecond pulsars from…

astro-ph.IM2020★ 127 cited

The Parkes Pulsar Timing Array Project: Second data release

M. Kerr, D. J. Reardon, G. Hobbs +27

We describe 14 years of public data from the Parkes Pulsar Timing Array (PPTA), an ongoing project that is producing precise measurements of pulse times of arrival from 26 millisec…

astro-ph.HE2017★ 29 cited

Comparison of Pulsar Positions from Timing and Very Long Baseline Astrometry

J. B. Wang, W. A. Coles, G. Hobbs +22

Pulsar positions can be measured with high precision using both pulsar timing methods and very-long-baseline interferometry (VLBI). Pulsar timing positions are referenced to a sola…

astro-ph.CO2013★ 173 cited

Gravitational-wave Limits from Pulsar Timing Constrain Supermassive Black Hole Evolution

R. M. Shannon, V. Ravi, W. A. Coles +14

The formation and growth processes of supermassive black holes (SMBHs) are not well constrained. SMBH population models, however, provide specific predictions for the properties of…