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We report the identification of extended tidal debris potentially associatedwith the globular cluster NGC 3201, using the RAVE catalogue. We find thedebris stars are located at a distance range of 1-7 kpc based on theforthcoming RAVE distance estimates. The derived space velocities and integralsof motion show interesting connections to NGC 3201, modulo uncertainties in theproper motions. Three stars, which are among the 4 most likely candidates forNGC 3201 tidal debris, are separated by 80 degrees on the sky yet are wellmatched 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 oversuch a large spatial extent, with implications for the cluster$'$s origin anddynamical evolution.

Identification of Globular Cluster Stars in RAVE data II: Extended tidal debris around NGC 3201