activity
20172020
most citedAccelerating parameter inference with graphics processing units

70 citations · 95 across the 4 of their papers we have counts for

collaborators

7 papers

gr-qc202021 cited

Inferring the neutron star equation of state simultaneously with the population of merging neutron stars

Daniel Wysocki, Richard O'Shaughnessy, Leslie Wade +1

Observations of the properties of multiple coalescing neutron stars will simultaneously provide insight into neutron star mass and spin distribution, the neutron star merger rate,…

astro-ph.HE2019

Black Hole Coagulation: Modeling Hierarchical Mergers in Black Hole Populations

Zoheyr Doctor, Daniel Wysocki, Richard O'Shaughnessy +2

Data from the LIGO and Virgo detectors has confirmed that stellar-mass black holes can merge within a Hubble time, leaving behind massive remnant black holes. In some astrophysical…

gr-qc2019

Impact of subdominant modes on the interpretation of gravitational-wave signals from heavy binary black hole systems

Feroz H. Shaik, Jacob Lange, Scott E. Field +5

Over the past year, a handful of new gravitational wave models have been developed to include multiple harmonic modes thereby enabling for the first time fully Bayesian inference s…

astro-ph.HE2019

Monte-Carlo simulations of black hole mergers in AGN disks: Low mergers and predictions for LIGO

B. McKernan, K. E. S. Ford, R. O'Shaughnessy +1

Accretion disks around supermassive black holes are promising sites for stellar mass black hole mergers detectable with LIGO. Here we present the results of Monte-Carlo simulations…

astro-ph.IM201970 cited

Accelerating parameter inference with graphics processing units

D. Wysocki, R. O'Shaughnessy, Y-L. L. Fang +1

Gravitational wave Bayesian parameter inference involves repeated comparisons of GW data to generic candidate predictions. Even with algorithmically efficient methods like RIFT or…

astro-ph.CO20193 cited

Response to Cusin et al's comment on arXiv:1810.13435

Alexander C. Jenkins, Mairi Sakellariadou, Tania Regimbau +3

We offer a brief response to the criticisms put forward by Cusin et al in arXiv:1811.03582 about our work arXiv:1810.13435 and arXiv:1806.01718, emphasising that none of these crit…