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We report on the first joint search for gravitational waves by the TAMA andLIGO collaborations. We looked for millisecond-duration unmodelledgravitational-wave bursts in 473 hr of coincident data collected during early2003. No candidate signals were found. We set an upper limit of 0.12 events perday on the rate of detectable gravitational-wave bursts, at 90% confidencelevel. From simulations, we estimate that our detector network was sensitive tobursts with root-sum-square strain amplitude above approximately 1-3x10^{-19}Hz^{-1/2} in the frequency band 700-2000 Hz. We describe the details of thiscollaborative search, with particular emphasis on its advantages anddisadvantages compared to searches by LIGO and TAMA separately using the samedata. Benefits include a lower background and longer observation time, at somecost in sensitivity and bandwidth. We also demonstrate techniques forperforming coincidence searches with a heterogeneous network of detectors withdifferent noise spectra and orientations. These techniques include usingcoordinated signal injections to estimate the network sensitivity, and tuningthe analysis to maximize the sensitivity and the livetime, subject toconstraints on the background.Comment: 15 pages, 11 figures, to be submitted to Phys Rev D. Updated author  lis

Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts