  We demonstrate the implementation of a sensitive search pipeline for
gravitational waves from coalescing binary black holes whose components have
spins aligned with the orbital angular momentum. We study the pipeline recovery
of simulated gravitational wave signals from aligned-spin binary black holes
added to real detector noise, comparing the pipeline performance with
aligned-spin filter templates to the same pipeline with non-spinning filter
templates. Our results exploit a three-parameter phenomenological waveform
family that models the full inspiral-merger-ringdown coalescence and treats the
effect of aligned spins with a single effective spin parameter \chi. We
construct template banks from these waveforms by a stochastic placement method
and use these banks as filters in the recently-developed gstlal search
pipeline. We measure the observable volume of the analysis pipeline for binary
black hole signals with total mass in [15,25] solar masses and \chi in [0,
0.85]. We find an increase in observable volume of up to 45% for systems with
0.2 <= \chi <= 0.85 with almost no loss of sensitivity to signals with 0 <=
\chi <= 0.2. We demonstrate this analysis on 25.9 days of data obtained from
the Hanford and Livingston detectors in LIGO's fifth observation run.
