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Supplemental information for a Letter reporting the rate of binary black hole(BBH) coalescences inferred from 16 days of coincident Advanced LIGOobservations surrounding the transient gravitational wave signal GW150914. Inthat work we reported various rate estimates whose 90\% credible intervals fellin the range $2$--$600 \, \mathrm{Gpc}^{-3} \mathrm{yr}^{-1}$. Here we givedetails of our method and computations, including information about our searchpipelines, a derivation of our likelihood function for the analysis, adescription of the astrophysical search trigger distribution expected frommerging BBHs, details on our computational methods, a description of theeffects and our model for calibration uncertainty, and an analytic method ofestimating our detector sensitivity that is calibrated to our measurements.

Supplement: The Rate of Binary Black Hole Mergers Inferred from Advanced LIGO Observations Surrounding GW150914