Description

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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.

About the Author

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Chiara Mingarelli received a BSc Double Honours Mathematics and Physics from Carleton University (Ottawa, Canada; 2006), an MSc in Astrophysics and Cosmology from the University of Bologna, (Bologna, Italy; 2009) and a PhD from the University of Birmingham (Birmingham, UK; 2014). She currently holds a Marie Curie International Outgoing Fellowship--a competitive 3-year prize fellowship funded by the European Union.