A search for gravitational waves from the millisecond pulsar PSR 0437-4715 has been initiated using the bar detector NIOBE which is located at the University of Western Australia. We present a detailed report on the data analysis algorithm, called phase plane rotation, which will be used in this search. A discussion of the actual implementation of the algorithm is presented. The data analysis algorithm mentioned above has the advantage that it requires minimal changes to the already-existing data acquisition facility of NIOBE but, at the same time, it is as efficient as optimal filtering in detecting a signal. This search involves a very long coherent integration of the bar output which may stretch over a few years. With some planned improvements in the detector, a three-year integration should be able to put an upper limit of h ∼ 10−26 on the signal amplitude.
Mohanty, Soumya; Heng, I. S.; Blair, David; Dhurandhar, S.; Tovar, M.; and Ivanov, E., "A data analysis approach for detecting gravitational waves from PSR 0437-4715" (1998). Physics and Astronomy Faculty Publications and Presentations. 390.
Monthly Notices of the Royal Astronomical Society