Brooks, A.Hosken, D.Munch, J.Ottaway, D.Veitch, P.Abbott, B.Abbott, R.Adhikari, R.Ajith, P.Allen, B.Allen, G.Amin, R.Anderson, S.Anderson, W.Arain, M.Araya, M.Armandula, H.Armor, P.Aso, Y.Aston, S.et al.2010-08-092010-08-092009Physical Review D: Particles, Fields, Gravitation and Cosmology, 2009; 80(4):7101-1-7101-51550-79981550-2368http://hdl.handle.net/2440/59649We report on a search for gravitational waves from coalescing compact binaries, of total mass between 2 and 35M⊙, using LIGO observations between November 14, 2006 and May 18, 2007. No gravitational-wave signals were detected. We report upper limits on the rate of compact binary coalescence as a function of total mass. The LIGO cumulative 90%-confidence rate upper limits of the binary coalescence of neutron stars, black holes and black hole-neutron star systems are 1.4×10-2, 7.3×10-4 and 3.6×10-3  yr-1 L10-1, respectively, where L10 is 1010 times the blue solar luminosity.en©2009 American Physical SocietyJournal article002009244410.1103/PhysRevD.80.0471010002696414001162-s2.0-7004910043137713Ottaway, D. [0000-0001-6794-1591]Veitch, P. [0000-0002-2597-435X]