activity
20162024
most citedThe International Pulsar Timing Array second data release: Search for an isotropic Gravitational Wave Background

344 citations · 435 across the 8 of their papers we have counts for

collaborators

23 papers

gr-qc20242 cited

CMB and energy conservation limits on nanohertz gravitational waves

David Wright, John T. Giblin, Jeffrey Hazboun

The recent evidence for a stochastic gravitational wave background (GWB) in the nanohertz band, announced by pulsar timing array (PTA) collaborations around the world, has been pos…

astro-ph.HE2022344 cited

The International Pulsar Timing Array second data release: Search for an isotropic Gravitational Wave Background

J. Antoniadis, Z. Arzoumanian, S. Babak +123

We searched for an isotropic stochastic gravitational wave background in the second data release of the International Pulsar Timing Array, a global collaboration synthesizing decad…

astro-ph.GA2021

The NANOGrav 11yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500Mpc

Zaven Arzoumanian, Paul T. Baker, Adam Brazier +54

Supermassive black hole binaries (SMBHBs) should form frequently in galactic nuclei as a result of galaxy mergers. At sub-parsec separations, binaries become strong sources of low-…

gr-qc202047 cited

Common-spectrum process versus cross-correlation for gravitational-wave searches using pulsar timing arrays

Joseph D. Romano, Jeffrey S. Hazboun, Xavier Siemens +1

The North American Nanohertz Observatory for Gravitational Waves (NANOGrav) has recently reported strong statistical evidence for a common-spectrum red-noise process for all pulsar…

astro-ph.HE2020

A Study in Frequency-Dependent Effects on Precision Pulsar Timing Parameters with the Pulsar Signal Simulator

Brent J. Shapiro-Albert, Jeffrey S. Hazboun, Maura A. McLaughlin +1

In this paper we introduce a new Python package, the Pulsar Signal Simulator, or PsrSigSim, which is designed to simulate a pulsar signal from emission at the pulsar, through the i…

astro-ph.IM2020

Model Dependence of Bayesian Gravitational-Wave Background Statistics for Pulsar Timing Arrays

Jeffrey S. Hazboun, Joseph Simon, Xavier Siemens +1

Pulsar timing array (PTA) searches for a gravitational-wave background (GWB) typically include time-correlated "red" noise models intrinsic to each pulsar. Using a simple simulated…