A search for gravitational waves from the millisecond pulsar PSR 0337-4715
has been initiated using the bar detector NIOBE which is located at the Uni
versity of Western Australia, We present a detailed report on the data anal
ysis algorithm, called phase plane rotation, which will be used in this sea
rch. A discussion of the actual implementation of the algorithm is presente
d. The data analysis algorithm mentioned above has the advantage that it re
quires minimal changes to the already-existing data acquisition facility of
NIOBE but, at the same time, it is as efficient as optimal filtering in de
tecting a signal. This search involves a very long coherent integration of
the bar output which may stretch over a few years. With some planned improv
ements in the detector, a three-year integration should be able to put an u
pper limit of h similar to 10(-26) on the signal amplitude.