We report the identification of extended tidal debris potentially associated with the globular cluster NGC 3201 , using the RAVE catalogue .
We find the debris stars are located at a distance range of 1-7 kpc based on the forthcoming RAVE distance estimates .
The derived space velocities and integrals of motion show interesting connections to NGC 3201 , modulo uncertainties in the proper motions .
Three stars , which are among the 4 most likely candidates for NGC 3201 tidal debris , are separated by 80 ^ { \circ } on the sky yet are well matched by the 12 Gyr , [ Fe/H ] = -1.5 isochrone appropriate for the cluster .
This is the first time tidal debris around this cluster has been reported over such a large spatial extent , with implications for the clusterÕs origin and dynamical evolution .