activity
20132026
most citedGravitational-wave Limits from Pulsar Timing Constrain Supermassive Black Hole Evolution

173 citations · 626 across the 10 of their papers we have counts for

collaborators

10 papers

gr-qc2026

Searching for a waveform-agnostic gravitational wave signal in pulsar timing arrays

Heling Deng, Bence Becsy, Yuri Levin +2

Pulsar timing arrays have recently provided compelling evidence for a nanohertz stochastic gravitational wave background, motivating searches for gravitational waves from localized…

gr-qc2017★ 48 cited

Challenges testing the no-hair theorem with gravitational waves

Eric Thrane, Paul Lasky, Yuri Levin

General relativity's no-hair theorem states that isolated astrophysical black holes are described by only two numbers: mass and spin. As a consequence, there are strict relationshi…

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.IM2016★ 27 cited

Wide-band Profile Domain Pulsar Timing Analysis

L. Lentati, M. Kerr, S. Dai +22

We extend profile domain pulsar timing to incorporate wide-band effects such as frequency-dependent profile evolution and broadband shape variation in the pulse profile. We also in…

astro-ph.IM2015★ 40 cited

Versatile Directional Searches for Gravitational Waves with Pulsar Timing Arrays

D. R. Madison, X. -J. Zhu, G. Hobbs +23

By regularly monitoring the most stable millisecond pulsars over many years, pulsar timing arrays (PTAs) are positioned to detect and study correlations in the timing behaviour of…

astro-ph.HE2015★ 4 cited

Timing analysis for 20 millisecond pulsars in the Parkes Pulsar Timing Array

D. J. Reardon, G. Hobbs, W. Coles +18

We present timing models for 20 millisecond pulsars in the Parkes Pulsar Timing Array. The precision of the parameter measurements in these models has been improved over earlier re…