Journal Title
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Publisher
Springer, Berlin, Heidelberg
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Authors: George Hobbs
Publish Date: 2011
Volume: , Issue: , Pages: 229-245
Abstract
Pulsar timing array projects are carrying out high precision observations of millisecond pulsars with the aim of detecting ultralow frequency ~ 109 to 108 Hz gravitational wavesWe show how unambiguous detections of such waves can be obtained by identifying a signal that is correlated between the timing of different pulsars Here we describe the ongoing observing projects the expected sources of gravitational waves the processing of the data and the implications of current results
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