During 2015 and 2016, the Laser Interferometer Gravitational-Wave Observatory (LIGO) conducted a three-month observing campaign. ese observations delivered the rst direct detection of gravitational waves from binary black hole mergers. To search for these signals, the LIGO Scienti c 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 largescale computation, our team deployed a distributed data access infrastructure based on the XRootD server suite and the CernVM File System (CVMFS). is data access strategy grew from simply accessing remote storage to a POSIX-based interface underpinned by distributed, secure caches across the OSG.Historically, the OSG has focused on providing a high-level computational services such as the dynamic creation of batch systems across multiple sites utilizing the pilot model [17]. In the pilot model, a central factory performs remote submission of batch jobs