activity
20172025
most citedReading signatures of supermassive binary black holes in pulsar timing array observations

6 citations · 12 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2025

Detecting Intermediate-mass Black Holes Using Miniature Pulsar Timing Arrays in Globular Clusters

Xian Chen, Verónica Vázquez-Aceves, Siyuan Chen +3

Theoretical models predict that intermediate-mass black holes (IMBHs) exist in globular clusters (GCs), but observational evidence remains elusive. Millisecond pulsars (MSPs), whic…

astro-ph.HE2024★ 6 cited

Reading signatures of supermassive binary black holes in pulsar timing array observations

Boris Goncharov, Shubhit Sardana, A. Sesana +10

We find the inferred properties of the putative gravitational wave background in the second data release of the European Pulsar Timing Array to be in better agreement with theoreti…

astro-ph.HE2024

Quasars can Signpost Supermassive Black Hole Binaries

J. Andrew Casey-Clyde, Chiara M. F. Mingarelli, Jenny E. Greene +3

Supermassive black holes (SMBHs) are found in the centers of massive galaxies, and galaxy mergers should eventually lead to SMBH mergers. Quasar activity has long been associated w…

astro-ph.HE2024

A Gaussian-processes approach to fitting for time-variable spherical solar wind in pulsar timing data

Iuliana C. Niţu, Michael J. Keith, Caterina Tiburzi +26

Propagation effects are one of the main sources of noise in high-precision pulsar timing. For pulsars below an ecliptic latitude of , the ionised plasma in the solar wind…

physics.data-an2020★ 4 cited

Applying clock comparison methods to pulsar timing observations

Siyuan Chen, Francois Vernotte, Enrico Rubiola

Frequency metrology outperforms any other branch of metrology in accuracy (parts in ) and small fluctuations (). In turn, among celestial bodies, the rotation…

physics.data-an2020★ 1 cited

Response and Uncertainty of the Parabolic Variance PVAR to Non-Integer Exponents of the Power Law

François Vernotte, Siyuan Chen, Enrico Rubiola

Oscillator fluctuations are described as the phase or frequency noise spectrum, or in terms of a wavelet variance as a function of the measurement time. The spectrum is generally a…

astro-ph.HE2017★ 1 cited

Pulsar science with data from the Large European Array for Pulsars

J. W. McKee, C. G. Bassa, S. Chen +12

The Large European Array for Pulsars (LEAP) is a European Pulsar Timing Array project that combines the Lovell, Effelsberg, Nançay, Sardinia, and Westerbork radio telescopes into a…