The LIGO Scientific Collaboration is currently engaged in the first search
for binary black hole inspiral signals in real data. We are using the data from
the second LIGO science run and we focus on inspiral signals coming from binary
systems with component masses between 3 and 20 solar masses. We describe the
analysis methods used and report on preliminary estimates for the sensitivities
of the LIGO instruments during the second science run.Comment: 10 pages, 2 figures. Added references for section 2, corrected figure
1. To appear in CQG, in a special issue on the proceedings of the 9th Annual
Gravitational Wave Data Analysis Workshop (GWDAW), Annecy, France, Dec. 200