  We discuss a method of coincidence analysis to search for gravitational waves
from inspiraling compact binaries using the data of two laser interferometer
gravitational wave detectors. We examine the allowed difference of the wave's
parameters estimated by each detector to obtain good detection efficiency. We
also discuss a method to set an upper limit to the event rate from the results
of the coincidence analysis. For the purpose to test above methods, we
performed a coincidence analysis by applying these methods to the real data of
TAMA300 and LISM detectors taken during 2001. We show that the fake event rate
is reduced significantly by the coincidence analysis without losing real events
very much. Results of the test analysis are also given.
