The data associated with the "S5: Probing the Milky Way and Magellanic Clouds potentials with the 6-D map of the Orphan-Chenab stream" paper. We provide * the Stan models used to extract stellar stream properties The measurement of radial velocity, stream track on the the sky, proper motions and stream densities for Orphan-Chenab. The list of candidate OC stream members from S5 and other surveys. The best fit stream N-body model the posterior chains from the stream/potential model. The enclosed mass profiles for LMC and MW (figure 15 and 17 of the paper)