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We report a search for gravitational waves from the inspiral, merger andringdown of binary black holes (BBH) with total mass between 25 and 100 solarmasses, in data taken at the LIGO and Virgo observatories between July 7, 2009and October 20, 2010. The maximum sensitive distance of the detectors over thisperiod for a (20,20) Msun coalescence was 300 Mpc. No gravitational wavesignals were found. We thus report upper limits on the astrophysicalcoalescence rates of BBH as a function of the component masses for non-spinningcomponents, and also evaluate the dependence of the search sensitivity oncomponent spins aligned with the orbital angular momentum. We find an upperlimit at 90% confidence on the coalescence rate of BBH with non-spinningcomponents of mass between 19 and 28 Msun of 3.3 \times 10^-7 mergers /Mpc^3/yr.

Search for Gravitational Waves from Binary Black Hole Inspiral, Merger and Ringdown in LIGO-Virgo Data from 2009-2010