Prospects for gravitational-wave detection and supermassive black hole astrophysics with pulsar timing arrays

Grants

Funding Acknowledgements

The authors thank Alberto Sesana for useful discussions and Justin Ellis for sharing results on predicted sensitivity curves. The authors also acknowledge the comments of the anonymous referee, which helped to significantly improve the manuscript. VR is a recipient of a John Stocker Postgraduate Scholarship from the Science and Industry Endowment Fund and JSBW acknowledges an Australian Research Council Laureate Fellowship. GH is supported by an Australian Research Council Future Fellowship. This work was performed on the swinSTAR supercomputer at the Swinburne University of Technology.