Overview

A new window of astronomy, employing Gravitational Waves, opened in the last decade. While such waves of kiloHertz frequencies have been discovered and are being used for astrophysical studies, low frequency waves are being detected, consisting of rapidly spinning massive and compact neutron stars called Pulsar Timing arrays. This field attracts numerous undergraduate and graduate students, but the complex data analysis required for these experiments, as well as understanding of associated statistical concepts, present a barrier for students to meaningfully contribute in this growing field. The focus of the book is to introduce the concepts and tools required for low frequency Gravitational wave (GW) astronomy to undergraduate and graduate students, as well as research scientists from other fields who may be interested in low frequency GW research or pulsar timing techniques. Key Features: A unique compendium for reference targeted at early researchers wanting to familiarize themselves with gravitational wave astronomy in general and nano-Hertz gravitational wave astronomy in particular. Suitable also for hands-on teaching and learning experience in advanced elective courses for graduate students as well as in student workshops organised by the IPTA and individual PTAs as well as individual groups involved in PTA experiments. Useful reference for astronomers/experts outside the field of nano-Hertz Gravitational waves astronomy to get a feel for this rapidly evolving field. Case studies and Jupyter notebooks drawn from the best practices currently adopted in these experiments.

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