Prospects for gravitational wave astronomy with next generation large-scale pulsar timing arrays
Instrumentation and Methods for Astrophysics
2018-04-04 v1
Abstract
Next generation radio telescopes, namely the Five-hundred-meter Aperture Spherical Telescope (FAST) and the Square Kilometer Array (SKA), will revolutionize the pulsar timing arrays (PTAs) based gravitational wave (GW) searches. We review some of the characteristics of FAST and SKA, and the resulting PTAs, that are pertinent to the detection of gravitational wave signals from individual supermassive black hole binaries.
Keywords
Cite
@article{arxiv.1711.04435,
title = {Prospects for gravitational wave astronomy with next generation large-scale pulsar timing arrays},
author = {Yan Wang and Soumya D. Mohanty},
journal= {arXiv preprint arXiv:1711.04435},
year = {2018}
}
Comments
6 pages, 1 figure; to be published in the proceedings of the 12-th Amaldi conference on gravitational waves (Pasadena, CA, July 2016)