Top: distribution in the sky around Virgo of the Sgr debris in the models of Law & Majewski (2010). The polygon indicates the region studied in this work. Bottom: velocity and distance of model particles (crosses) and RRLS (asterisks) within the box indicated above. Stars in each one of the 5 kinematical groups detected here are shown with their corresponding symbol (Table 8). The two RRLS at distances >40 kpc were taken from Vivas et al. (2005). Rectangle indicates the approximate location of another kinematical group found by Brink et al. (2010) and Casey et al. (2012).