  During 2015 and 2016, the Laser Interferometer Gravitational-Wave Observatory
(LIGO) conducted a three-month observing campaign. These observations delivered
the first direct detection of gravitational waves from binary black hole
mergers. To search for these signals, the LIGO Scientific Collaboration uses
the PyCBC search pipeline. To deliver science results in a timely manner, LIGO
collaborated with the Open Science Grid (OSG) to distribute the required
computation across a series of dedicated, opportunistic, and allocated
resources. To deliver the petabytes necessary for such a large-scale
computation, our team deployed a distributed data access infrastructure based
on the XRootD server suite and the CernVM File System (CVMFS). This data access
strategy grew from simply accessing remote storage to a POSIX-based interface
underpinned by distributed, secure caches across the OSG.
