most citedAn Updated Galactic Double Neutron Star Merger Rate Based on Radio Pulsar Populations

18 citations · 23 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.HE20201 cited

Modeling the Galactic Compact Binary Neutron Star Population and Studying the Double Pulsar System

Nihan Pol

In this dissertation, we estimate the population of different classes of BNS systems that are visible to gravitational-wave observatories. Given that no ultra-compact BNS systems h…

astro-ph.GA20204 cited

Multi-Messenger Gravitational Wave Searches with Pulsar Timing Arrays: Application to 3C66B Using the NANOGrav 11-year Data Set

Zaven Arzoumanian, Paul T. Baker, Adam Brazier +56

When galaxies merge, the supermassive black holes in their centers may form binaries and, during the process of merger, emit low-frequency gravitational radiation in the process. I…

astro-ph.HE202018 cited

An Updated Galactic Double Neutron Star Merger Rate Based on Radio Pulsar Populations

Nihan Pol, Maura McLaughlin, Duncan Lorimer

Following the procedure described in Pol et al., we update the Galactic double neutron star (DNS) merger rate by including the new, highly eccentric DNS system J0509+3801 (Lynch et…

astro-ph.HE2020

Modeling the uncertainties of solar-system ephemerides for robust gravitational-wave searches with pulsar timing arrays

M. Vallisneri, S. R. Taylor, J. Simon +61

The regularity of pulsar emissions becomes apparent once we reference the pulses' times of arrivals to the inertial rest frame of the solar system. It follows that errors in the de…

astro-ph.HE2019

The NANOGrav 11-Year Data Set: Evolution of Gravitational Wave Background Statistics

J. S. Hazboun, J. Simon, S. R. Taylor +60

An ensemble of inspiraling supermassive black hole binaries should produce a stochastic background of very low frequency gravitational waves. This stochastic background is predicte…