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One of the most exciting prospects for the LISA gravitational waveobservatory is the detection of gravitational radiation from the inspiral of acompact object into a supermassive black hole. The large inspiral parameterspace and low amplitude of the signal makes detection of these sourcescomputationally challenging. We outline here a first cut data analysis schemethat assumes realistic computational resources. In the context of this scheme,we estimate the signal-to-noise ratio that a source requires to pass ourthresholds and be detected. Combining this with an estimate of the populationof sources in the Universe, we estimate the number of inspiral events that LISAcould detect. The preliminary results are very encouraging -- with the baselinedesign, LISA can see inspirals out to a redshift z=1 and should detect over athousand events during the mission lifetime.Comment: 15 pages, 1 figure, to appear in GWDAW 8 proceeding

Event rate estimates for LISA extreme mass ratio capture sources