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Paper: Prospects of Gravitational Wave Detection Using Pulsar Timing Array for Chinese Future Telescopes
Volume: 502, Frontiers in Radio Astronomy and FAST Early Sciences Symposium 2015
Page: 19
Authors: Lee, K. J.
Abstract: In this paper, we estimate the sensitivity of gravitational wave (GW) detection for future Chinese pulsar timing array (PTA) projects. The calculation of sensitivity is based on the well-known Crámer-Rao bound idea. The red noise and dispersion measure (DM) variation noise has be included in the modeling. We demonstrate that the future Chinese telescope can be very valuable for future PTA experiments and GW detection efforts.
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