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Table of Contents
Introduction
Characterizing Gravitational Wave Stochastic Background Anisotropy with Pulsar Timing Arrays
The Effect of Small Pulsar Distance Variations in Stochastic GW
Observing the Dynamics of Supermassive Black Hole Binaries with Pulsar Timing
Conclusions
Appendix
Bibliography.
Characterizing Gravitational Wave Stochastic Background Anisotropy with Pulsar Timing Arrays
The Effect of Small Pulsar Distance Variations in Stochastic GW
Observing the Dynamics of Supermassive Black Hole Binaries with Pulsar Timing
Conclusions
Appendix
Bibliography.