Detection and localization of single-source gravitational waves with pulsar timing arrays

Pulsar timing arrays (PTAs) can be used to search for very low frequency (\(10^{-9}\)--\(10^{-7}\) Hz) gravitational waves (GWs). In this paper we present a general method for the detection and localization of single-source GWs using PTAs. We demonstrate the effectiveness of this new method for thre...

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Veröffentlicht in:	arXiv.org 2015-03
Hauptverfasser:	Xing-Jiang, Zhu, Wen, Linqing, Hobbs, George, Zhang, Yilin, Wang, Yan, Madison, Dustin R, Manchester, Richard N, Kerr, Matthew, Rosado, Pablo A, Wang, Jingbo
Format:	Artikel
Sprache:	eng
Schlagworte:	Binary stars Circular orbits Data transmission Eccentric orbits Gravitation Gravitational waves Localization Physics - Astrophysics of Galaxies Physics - General Relativity and Quantum Cosmology Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Pulsars Time domain analysis Very Low Frequencies
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