Gravitational-Wave Detection Using Pulsars: Status of the Parkes Pulsar Timing Array Project

The first direct detection of gravitational waves may be made through observations of pulsars. The principal aim of pulsar timing-array projects being carried out worldwide is to detect ultra-low frequency gravitational waves (f ~10-9-10-8 Hz). Such waves are expected to be caused by coalescing supe...

Full description

Bibliographic Details
Main Authors: Hobbs, G., Bailes, M., Bhat, N., Burke-Spolaor, S., Champion, D., Coles, W., Hotan, Aidan
Format: Journal Article
Published: CSIRO 2009
Subjects:
Online Access:http://hdl.handle.net/20.500.11937/17672